Wikipedia:Reference desk/Mathematics: Difference between revisions
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[[Category:Wikipedia resources for researchers]] |
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[[Category:Wikipedia help forums]] |
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[[Category:Wikipedia reference desk|Mathematics]] |
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= November 29 = |
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{{Wikipedia:Reference_desk/Archives/Mathematics/2010 January 8}} |
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== In [[finite fields]] of large characteristics, what does prevent shrinking the modulus field size down to their larger order in order to solve discrete logarithms ? == |
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{{Wikipedia:Reference_desk/Archives/Mathematics/2010 January 9}} |
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In the recent years, several algorithms were proposed to leverage elliptic curves for lowering the degree of a finite field and thus allow to solve discrete logairthm modulo their largest suborder/subgroup instead of the original far larger finite field. https://arxiv.org/pdf/2206.10327 in part conduct a survey about those methods. Espescially since I don’t see why a large chararcteristics would be prone to fall in the trap being listed by the paper. |
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{{Wikipedia:Reference_desk/Archives/Mathematics/2010 January 10}} |
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I do get the whole ''small characteristics'' alogrithms complexity makes those papers unsuitable for computing discrete logarithms in finite fields of large charateristics, but what does prevent applying the ''descent/degree shrinking part'' to large characteristics ? [[Special:Contributions/2A01:E0A:401:A7C0:68A8:D520:8456:B895|2A01:E0A:401:A7C0:68A8:D520:8456:B895]] ([[User talk:2A01:E0A:401:A7C0:68A8:D520:8456:B895|talk]]) 11:00, 29 November 2024 (UTC) |
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= January 11 = |
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:Try web search for Lim-Lee small subgroup attack. [[Special:Contributions/2601:644:8581:75B0:0:0:0:C426|2601:644:8581:75B0:0:0:0:C426]] ([[User talk:2601:644:8581:75B0:0:0:0:C426|talk]]) 23:09, 1 December 2024 (UTC) |
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::First the paper apply when no other information is known beside the 2 finite field’s elements and then this is different from https://arxiv.org/pdf/2206.10327. While Pollard rho can remain more efficient, if the subgroup is too large, then it’s still not enough fast. I’m talking about shrinking modulus size directly. [[Special:Contributions/2A01:E0A:401:A7C0:69D2:554C:93AF:D6AC|2A01:E0A:401:A7C0:69D2:554C:93AF:D6AC]] ([[User talk:2A01:E0A:401:A7C0:69D2:554C:93AF:D6AC|talk]]) 15:17, 2 December 2024 (UTC) |
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The problem with descent methods like the one described in large characteristic is that the complexity is <math>max(q,k)^{\log k}</math>. This is explained more clearly in [https://arxiv.org/pdf/1306.4244]. If the characteristic is small, then the problem is O(k) bits, and the complexity id pseudo-polynomial in the number of bits. If the characteristic is large, then the compexity is <math>q^{\log k}</math> which is exponential in the number of bits of q. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 16:36, 2 December 2024 (UTC) |
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== Perimeter of a trapezium == |
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:Are you sure ? I’m not talking about the complexity of the index calculus part like chosing the factor base or computing individual discrete logarithms or the linear algebra phase. Only about the part consisting of shrinking the modulus through lowering it’s degree… [[Special:Contributions/82.66.26.199|82.66.26.199]] ([[User talk:82.66.26.199|talk]]) 10:26, 3 December 2024 (UTC) |
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::The paper I cited above finds the intermediate polynomials by a brute force search in small degree, which is thus polynomial in q. The general heuristic is that the search for intermediate polynomials takes about as long as the index calculus phase. But it looks like no one has a really good way to do it. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 10:45, 3 December 2024 (UTC) |
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:::And [https://arxiv.org/pdf/2206.10327 in my case, elliptic curves are used] to lower the degree and thus the modulus instead of brutefore. The person who wrote the paper told me in fact the idea was developed initially for medium characteristics but refused to give details for large characteristics. [[Special:Contributions/82.66.26.199|82.66.26.199]] ([[User talk:82.66.26.199|talk]]) 11:06, 3 December 2024 (UTC) |
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:::: I'm not really convinced that the approach actually works. How are the elliptic curves constructed? The construction given is very implicit. I'm betting that if one actually writes out the details, it involves lifting something from the prime field. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 16:02, 3 December 2024 (UTC) |
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:::::Yes. My request to have more details wasn’t well received. https://sympa.inria.fr/sympa/arc/cado-nfs/2024-12/msg00002.html [[Special:Contributions/2A01:E0A:401:A7C0:5985:1F5D:4595:AA09|2A01:E0A:401:A7C0:5985:1F5D:4595:AA09]] ([[User talk:2A01:E0A:401:A7C0:5985:1F5D:4595:AA09|talk]]) 01:48, 4 December 2024 (UTC) |
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= November 30 = |
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What is the formular to find the perimeter of a trapezium <span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/202.170.37.10|202.170.37.10]] ([[User talk:202.170.37.10|talk]]) 03:31, 11 January 2010 (UTC)</span><!-- Template:UnsignedIP --> <!--Autosigned by SineBot--> |
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== Linear differential function == |
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:What information do you know? Often you know at least two of the four side lengths, and you can usually find the others by using the [[Pythagorean theorem]]. —[[User:Bkell|Bkell]] ([[User talk:Bkell|talk]]) 05:33, 11 January 2010 (UTC) |
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Differential [[Special:Contributions/102.213.69.166|102.213.69.166]] ([[User talk:102.213.69.166|talk]]) 04:35, 30 November 2024 (UTC) |
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:: [[Image:Trapezoid.svg|right|frame|A trapezoid]]''(Assuming that you mean the shape with two parallel sides, called a [[trapezoid]] in the USA)'' If you know the lengths of the parallel sides, the height, and the two angles at A and B, then the perimeter is just '''a + b + h(cosec + cosecB)'''.<br> As Bkell says, for other possibilities, you can often use "Pythagoras" or [[Trigonometry]] if you have enough information. <small>(Trivially, if you know the lengths of all four sides, just add them together!)</small> [[User:Dbfirs|''<font face="verdana"><font color="blue">D</font><font color="#00ccff">b</font><font color="#44ffcc">f</font><font color="66ff66">i</font><font color="44ee44">r</font><font color="44aa44">s</font></font>'']] 10:02, 11 January 2010 (UTC) |
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:What are you talking about? <span style="color: #000065; font-size: 5; font-family: monospace">‹[[User:Hamterous1|hamster717🐉]]› <sup>([[User talk:Hamterous1|discuss anything!🐹✈️]] • [[Special:Contributions/Hamterous1|my contribs🌌🌠]])</sup></span> 14:02, 30 November 2024 (UTC) |
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== Smoothness Scale In Number Theory == |
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Have there been any reasonably good attempts to refine the idea of relative smoothness of numbers? I'm looking for something like a scale that defines powers of 2 as 1 and primes as 0 (or the reverse), something that gives a pretty good--and increasingly better with size--relative smoothness by some reasonable consideration of it. Is the best out there what's essentially already in the [[smooth number]] article?[[User:Julzes|Julzes]] ([[User talk:Julzes|talk]]) 14:37, 11 January 2010 (UTC) |
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= January 12 = |
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== Normal Closures Qual. Exam == |
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= December 4 = |
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I'm stuck on the problem: Given a non-normal separable extension [E: F] = 4, bound the degree [K: F] of the |
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normal closure of E. [Bergman] from a grad. qual. exam http://www.math.harvard.edu/graduate/quals/topics/galois.pdf. Please help! I think that [K: F] is bounded by 8 by testing a couple of examples like F = Q, E = Q[a] where a<sup>4</sup> = 2 where the minimal polynomial of a over Q has a splitting field of degree 8 and other examples. Obviously [K: F] is bounded by 24, but I'm not sure that's what the question is after (I don't even know whether 24 is a strict bound, that you can get a normal closure of degree 24 in the problem). I haven't much experience with normal closures, but I don't believe I require it for this question. The other qual. exam problems in the link are dead easy and that's why this one question is bugging me. Thanks. <span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/122.109.42.56|122.109.42.56]] ([[User talk:122.109.42.56|talk]]) 06:25, 12 January 2010 (UTC)</span><!-- Template:UnsignedIP --> <!--Autosigned by SineBot--> |
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:I'm fairly certain that the bound 24 is optimal. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 11:11, 12 January 2010 (UTC) |
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::Can you show me how [E: F] = 4 can exist with [K: F] = 24? Thanks for your answer but I can't think of an explicit example of how the degree could get as high as 24. Why I'm unsure that the degree is 24, is because of the specificity of the problem ([E: F] = 4, and not [E: F] = n for any n), and that it's a qual. problem.<span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/122.109.42.56|122.109.42.56]] ([[User talk:122.109.42.56|talk]]) 11:15, 12 January 2010 (UTC)</span><!-- Template:UnsignedIP --> |
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:::Let <math>K=\mathbb Q(x_0,x_1,x_2,x_3)</math> (the field of rational functions in 4 variables, that is, the ''x<sub>i</sub>'' are algebraically independent). Any <math>\sigma\in\mathrm{Sym}_4</math> induces an automorphism of ''K'' by permuting the corresponding variables. Let ''F'' be the fixed field of all these automorphisms, and let ''E'' = ''F''(''x''<sub>0</sub>). The minimal polynomial of ''x''<sub>0</sub> over ''F'' is <math>f(x)=\prod_{i<4}(x-x_i)\,</math>, hence [''E'' : ''F''] = 4. The normal closure of ''E'' (i.e., the splitting field of ''f'' over ''F'') is ''K'', and the construction ensures Gal(''K''/''F'') = Sym<sub>4</sub>, hence [''K'' : ''F''] = 24. Of course, the same argument works for any ''n'', there's nothing special about 4. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 11:30, 12 January 2010 (UTC) |
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::::Maybe I should also stress that this ''F'' can be easily described explicitly, namely it is the field generated by the elementary symmetric polynomials: |
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:::::<math>{F=\mathbb Q(x_0+x_1+x_2+x_3,x_0x_1+x_0x_2+x_0x_3+x_1x_2+x_1x_3+x_2x_3,x_0x_1x_2+x_0x_1x_3+x_0x_2x_3+x_1x_2x_3,x_0x_1x_2x_3).}</math> |
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::::— [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 18:42, 12 January 2010 (UTC) |
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Thanks muchly so F can be chosen as the fixed field of that Galois group. Just to investigate furthur suppose F = Q. Is it then true that the bound of 8 is optimal? I've been basically looking at the problem for F = Q so that's probably why I wasn't thinking clearly but in the case F = Q my bound seems to work. Thanks.<span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/122.109.42.56|122.109.42.56]] ([[User talk:122.109.42.56|talk]]) 11:58, 12 January 2010 (UTC)</span><!-- Template:UnsignedIP --> |
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:Please, [[WP:SIG|sign your posts]], and don't remove signatures supplied by others without adequate replacement. This is a basic rule of conduct here. |
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== How much is this == |
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:No, you can get degree 24 even for ''F'' = '''Q'''. The problem is equivalent to asking for a normal extension ''K'' of '''Q''' such that Gal(''K''/'''Q''') = Sym<sub>4</sub>. This is a particular instance of the [[inverse Galois problem]]. While the general problem for arbitrary finite groups remains unsolved, many special cases are known, and in particular, one can always find such an extension for any Sym<sub>''n''</sub> (the argument is described at [[Inverse Galois problem#Symmetric and alternating groups]]; your polynomial is {{nowrap|''x''<sup>4</sup> − ''t''(''x'' + 1)}} for a suitably chosen rational number ''t''). — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 13:35, 12 January 2010 (UTC) |
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:If you're concerned about your IP address being visible, don't worry (or worry more, depending on how you look at it). Your IP address is publicly available in the [http://en.wikipedia.org/enwiki/w/index.php?title=Wikipedia:Reference_desk/Mathematics&action=history history page] (and this is common knowledge, so don't accuse me of further compromising your privacy). -- [[User:Meni Rosenfeld|Meni Rosenfeld]] ([[User Talk:Meni Rosenfeld|talk]]) 15:33, 12 January 2010 (UTC) |
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: <math>\sum_{k=0}^{n} (-1)^k</math> |
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:And if you are indeed concerned about your IP address being visible, the easy solution is to [[WP:REG|create an account]]. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 15:53, 12 January 2010 (UTC) |
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[[Special:Contributions/37.162.46.235|37.162.46.235]] ([[User talk:37.162.46.235|talk]]) 11:00, 4 December 2024 (UTC) |
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Sorry about that, I was just worried that people may find me out. I didn't know you were adding the signature, so I thought it was alright to remove it. Thanks for the help. <span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/122.109.42.151|122.109.42.151]] ([[User talk:122.109.42.151|talk]]) 02:15, 13 January 2010 (UTC)</span><!-- Template:UnsignedIP --> <!--Autosigned by SineBot--> |
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::1 for ''n'' even, 0 for ''n'' odd. For <math>n \to \infty</math> see [[Grandi's series]]. --[[User:Wrongfilter|Wrongfilter]] ([[User talk:Wrongfilter|talk]]) 11:18, 4 December 2024 (UTC) |
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:I hope this is not homework. Note that (for finite <math>n</math>) this is a [[Geometric series|finite geometric series]]. --[[User talk:Lambiam#top|Lambiam]] 21:51, 4 December 2024 (UTC) |
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== solution of differential equation of motion of a quarter car == |
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= December 6 = |
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Where can i find a solution of differential equation of motion of a quarter car? <span style="font-size: smaller;" class="autosigned">—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[Special:Contributions/113.199.176.179|113.199.176.179]] ([[User talk:113.199.176.179|talk]]) 17:04, 12 January 2010 (UTC)</span><!-- Template:UnsignedIP --> <!--Autosigned by SineBot--> |
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:What equation is that? And what is a "quarter car", anyway? — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 17:25, 12 January 2010 (UTC) |
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::"Quarter car model" gets a lot of Google hits (but I haven't read them !). [[User:Gandalf61|Gandalf61]] ([[User talk:Gandalf61|talk]]) 17:29, 12 January 2010 (UTC) |
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::Something like [[Quarter Midget racing]], may be? --[[User:CiaPan|CiaPan]] ([[User talk:CiaPan|talk]]) 18:16, 12 January 2010 (UTC) |
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== Is there anything that would prevent peforming Weil Descent on binary curves of large characteristics ? == |
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:The only thing you can look at by only looking at a quarter of a car is the suspension of one wheel, i.e. disregarding all effects (lateral, turning, anti-roll bar, drag etc.) which require knowledge of the other wheels or the body. The page [[Vehicle dynamics]] links to [[Tuned mass damper]] which may be what you need.--<small>[[User:JohnBlackburne|JohnBlackburne]]</small><sup>[[User_talk:JohnBlackburne|words]]</sup><sub style="margin-left:-5.0ex;">[[Special:Contributions/JohnBlackburne|deeds]]</sub> 18:45, 12 January 2010 (UTC) |
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The ghs attack involve creating an hyperlliptic curve cover for a given binary curve. The reason the attack fails most of the time is the resulting genus grows exponentially relative to the curve’s degree. |
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: [[Drag race]]s are traditionally a quarter mile... -- [[User:Coneslayer|Coneslayer]] ([[User talk:Coneslayer|talk]]) 20:05, 13 January 2010 (UTC) |
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We don’t hear about the attack on finite fields of large characteristics since such curves are already secure by being prime. '''However, I notice a few protocol relies on the discrete logarithm security on curves with 400/500 bits modulus resulting from extension fields of characteristics that are 200/245bits long'''. |
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== Locally invertible function from R^2 to R == |
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Since the degree is most of the time equal to 3 or 2, is there anything that would prevent creating suitable hyperelliptic cover for such curves in practice ? [[Special:Contributions/2A01:E0A:401:A7C0:28FE:E0C4:2F97:8E08|2A01:E0A:401:A7C0:28FE:E0C4:2F97:8E08]] ([[User talk:2A01:E0A:401:A7C0:28FE:E0C4:2F97:8E08|talk]]) 12:09, 6 December 2024 (UTC) |
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Hi all, |
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= December 7 = |
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I want to show that for <math>f(x,y)=(x,x^3+y^3-3xy)</math>, and <math>C=\{(x,y):x^3+y^3-3xy=0\}</math>, f is locally invertible around each point of C except (0,0) and <math>(2^\frac{2}{3},2^\frac{1}{3})</math>, i.e. show that there are open sets U and V about any <math>(x_0,y_0)</math> in C (but for the aforementioned 2 points) such that f maps bijectively: U<math>\to</math>V. Could anyone give me a hand? I've tried saying f(a,b)=f(c,d), so a=c, and then if b is not equal to d, we get 3a=<math>b^2+bd+d^2</math>, and I'm not sure where to go from here or whether I am indeed going in the right direction. I haven't actually used the fact that we're local to points where the second coordinate of f(x,y) is 0, and I can't really see what makes the above 2 points special either. Could anyone give me a hand finishing this off? |
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== Mathematical operation navigation templates == |
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I also want to find the derivative of the inverse function (locally) - what would be the neatest way to find this? |
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{{hat|collapse=no|reason=RDBury is right, this discussion belongs at [[Wikipedia talk:WikiProject Mathematics#Navigation templates for mathematical operations|Wikipedia talk:WikiProject Mathematics]]}} |
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Many, many thanks! [[User:Spamalert101|Spamalert101]] ([[User talk:Spamalert101|talk]]) 20:09, 12 January 2010 (UTC) |
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If anyone with some mathematical expertise is interested, I'd appreciate some additional input at [[Talk:Exponentiation#funny table at end]]. The question is whether our articles on various mathematical operations could use a [[Wikipedia:Navigation template|navigational template]] (aka "{{tl|Navbox}}"). Our [[Exponentiation]] article tried to use {{tl|Mathematical expressions}} for this purpose, but it doesn't really work. I've created {{tl|Mathematical operations}} as a potential alternative, but the categorization and presentation I've created is probably naïve. (The whole effort may or not be worth it at all.) —[[User:scs|scs]] ([[User talk:scs|talk]]) 00:36, 7 December 2024 (UTC) |
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:[[Wikipedia talk:WikiProject Mathematics]] is a better forum for this kind of thing, since it's focused on Wikipedia's mathematical articles. --[[User:RDBury|RDBury]] ([[User talk:RDBury|talk]]) 04:07, 7 December 2024 (UTC) |
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:: {{Re|RDBury}} Excellent point. Thanks. —[[User:scs|scs]] ([[User talk:scs|talk]]) 13:49, 7 December 2024 (UTC) |
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{{hab}} |
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= December 8 = |
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:[[Jacobian matrix and determinant]] might be a good place to start. Basically the Jacobian gives you the linear transformation that your function looks like locally. The two points you mentioned are the points on C where the Jacobian determinant is zero. The derivative of the inverse function at a point will be the inverse of the Jacobian there. Note that won't work when the determinant is zero. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 21:58, 12 January 2010 (UTC) |
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:Just want to add, if the Jacobian determinant is zero that doesn't necessarily imply a problem, but those are the places where things can potentially go wrong. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 00:16, 13 January 2010 (UTC) |
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== For each positive integer <math>n</math>, which primes <math>p</math> are still primes in the ring <math>Z[e^{\frac{\pi i}{n}}]</math>? == |
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:To be precise, if the Jacobian is zero at a point, the map is not locally invertible there ''in the C<sup>1</sup> sense'', that is with a C<sup>1</sup> local inverse. So, to give a complete answer to the question as you stated it, now you just have to look more closely at the two points where the Jacobian determinant vanishes (as Rckrone sais, the Jacobian determinant being zero doesn't necessarily imply that the map is not locally bijective there). For instance, the map is not locally bijective at (0,0), because e.g. for any 0 < ε < 1 there are at least two distinct solutions (x<sub>1</sub>,y<sub>1</sub>) and (x<sub>2</sub>,y<sub>2</sub>) of f(x,y) = (ε,0) close to (0,0), namely with x<sub>1</sub> = x<sub>2</sub> = ε and 0 < y<sub>1</sub> < ε<sup>1/2 </sup> < y<sub>2</sub> < 2ε<sup>1/4</sup> (just look at the sign of y<sup>3</sup> - 3εy + ε<sup>3</sup>). Can you see how to do the other point? (It is also possible a more detailed geometric description of the local structure of C at these points, of course) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 08:24, 13 January 2010 (UTC) |
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::That's great - thanks all, i've got it now :) [[User:Spamalert101|Spamalert101]] ([[User talk:Spamalert101|talk]]) 13:46, 13 January 2010 (UTC) |
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For each positive integer <math>n</math>, which primes <math>p</math> are still primes in the ring <math>Z[e^{\frac{\pi i}{n}}]</math>? When <math>n=1</math>, <math>Z[e^{\frac{\pi i}{n}}]</math> is the original integer ring, when <math>n=2</math>, <math>Z[e^{\frac{\pi i}{n}}]</math> is the ring of [[Gaussian integer]]s, when <math>n=3</math>, <math>Z[e^{\frac{\pi i}{n}}]</math> is the ring of [[Eisenstein integer]]s, and the primes in the [[Gaussian integer]]s are the primes <math>p \equiv 3 \mod 4</math>, and the primes in the [[Eisenstein integer]]s are the primes <math>p \equiv 2 \mod 3</math>, but how about larger <math>n</math>? [[Special:Contributions/218.187.66.163|218.187.66.163]] ([[User talk:218.187.66.163|talk]]) 04:50, 8 December 2024 (UTC) |
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== Estimating number ratios == |
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:A minuscule contribution: for <math>n=4,</math> the natural Gaussian primes <math>3</math> and <math>7</math> are composite: |
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For instance 2.68:1 ratio, if I want to round to nearst 0-5-0 should 2.68 round up to 3 or it should round to 2.5 if I'm douing halfway rounding scale. For 3.04:1 to estimating sentence is it could be cite as more than 3 times xx and vice versa, or 3.04 is usually said like about 3 times the xx vice versa since 3.04:1 is only 4 cents past 3?--[[Special:Contributions/209.129.85.4|209.129.85.4]] ([[User talk:209.129.85.4|talk]]) 20:26, 12 January 2010 (UTC) |
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:*<math>3=(1-\omega-\omega^2)(1+\omega^2+\omega^3).</math> |
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:*<math>7=(2-\omega+2\omega^2)(2-2\omega^2-\omega^3).</math> |
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:So <math>11</math> is the least remaining candidate. --[[User talk:Lambiam#top|Lambiam]] 09:00, 8 December 2024 (UTC) |
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::It is actually easy to see that <math>7</math> is composite, since <math>2</math> is a perfect square: |
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:::<math>2=i(1-i)^2=\omega^2(1-\omega^2)^2.</math> |
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::Hence, writing <math>\sqrt2</math> by abuse of notation for <math>\omega(1-\omega^2),</math> we have: |
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:::<math>\begin{alignat}{2}7&=(3+\sqrt2)(3-\sqrt2)\\&=(2\sqrt2+1)(2\sqrt2-1)\\&=(5+3\sqrt2)(5-3\sqrt2)\\&=(4\sqrt2+5)(4\sqrt2-5).\end{alignat}</math> |
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::More in general, any natural number that can be written in the form <math>|2a^2-b^2|,a,b\in\mathbb N,</math> is not prime in <math>\mathbb Z[e^{\pi i/4}].</math> This also rules out the Gaussian primes <math>23,</math> <math>31,</math> <math>47,</math> <math>71</math> and <math>79.</math> --[[User talk:Lambiam#top|Lambiam]] 11:50, 8 December 2024 (UTC) |
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:::So which primes <math>p</math> are still primes in the ring <math>Z[e^{\frac{\pi i}{4}}]</math>? How about <math>Z[e^{\frac{\pi i}{5}}]</math> and <math>Z[e^{\frac{\pi i}{6}}]</math>? [[Special:Contributions/220.132.216.52|220.132.216.52]] ([[User talk:220.132.216.52|talk]]) 06:32, 9 December 2024 (UTC) |
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::::As I wrote, this is only a minuscule contribution. We do not do research on command; in fact, we are actually not supposed to do any original research here. --[[User talk:Lambiam#top|Lambiam]] 09:23, 9 December 2024 (UTC) |
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::Moreover, <math>-2</math> is also a perfect square. (As in the Gaussian integers, the additive inverse of a square is again a square.) So natural numbers of the form <math>2a^2+b^2</math> are also composite. This further rules out <math>11,</math> <math>19,</math> <math>43,</math> <math>59,</math> <math>67</math> and <math>83.</math> A direct proof that, e.g., <math>11</math> is composite: <math>11=(1+\omega^2+3\omega^3)(1-3\omega-\omega^2).</math> There are no remaining candidates below <math>100</math> and I can in fact not find any larger ones either. This raises the conjecture: |
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::: |
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:::''Every prime number can be written in one of the three forms <math>a^2+b^2,</math> <math>2a^2+b^2</math> and <math>|2a^2-b^2|.</math>'' |
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::: |
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::Is this a known theorem? If true, no number in <math>\mathbb Z[e^{\pi i/4}]</math> is a natural prime. (Note that countless composite numbers cannot be written in any of these forms; to mention just a few: <math>15, 1155, 2491.</math>) --[[User talk:Lambiam#top|Lambiam]] 11:46, 9 December 2024 (UTC) |
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: I'll state things a little more generally, in the cyclotomic field <math>\mathbb Q[e^{2\pi i /n}]</math>. (Your n is twice mine.) A prime q factors as <math>q = (q_1\cdots q_r)^{e_r}</math>, where each <math>q_i</math> is a prime ideal of the same degree <math>f</math>, which is the least positive integer such that <math>q^f \equiv 1\pmod n</math>. (We have assumed that q does not divide n, because if it did, then it would ramify and not be prime. Also note that we have to use ideals, because the cyclotomic ring is not a UFD.) In particular, <math>q</math> stays prime if and only if <math>q</math> generates the group of units modulo <math>n</math>. When n is a power of two times an odd composite, the group of units is not cyclic, and so the answer is ''never''. When n is a prime or twice a prime, the answer is when q is a primitive root mod n. If n is 4 times a power of two times a prime, the answer is ''never''. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 11:08, 8 December 2024 (UTC) |
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:It's unclear to me what you are asking; maybe you will find something helpful at [[rounding]]. If I were to choose between rounding 2.68 to either 2.5 or to 3, I would likely choose to round to the nearer number. As for your second question, it is correct to say that 3.04 is more than 3 and it is also correct to say that 3.04 is about 3, so either sentence is correct. Eric. [[Special:Contributions/131.215.159.171|131.215.159.171]] ([[User talk:131.215.159.171|talk]]) 09:14, 13 January 2010 (UTC) |
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::For your <math>n</math>, <math>n=3</math> and <math>n=6</math> are the same, as well as <math>n=5</math> and <math>n=10</math>, this is why I use <math>e^{\frac{\pi i}{n}}</math> instead of <math>e^{\frac{2 \pi i}{n}}</math>. [[Special:Contributions/61.229.100.34|61.229.100.34]] ([[User talk:61.229.100.34|talk]]) 20:58, 8 December 2024 (UTC) |
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::Also, what is the [[class number (number theory)|class number]] of the [[cyclotomic field]] <math>Q[e^{\frac{\pi i}{n}}]</math>? Let <math>\gamma(n)</math> be the [[class number (number theory)|class number]] of the [[cyclotomic field]] <math>Q[e^{\frac{\pi i}{n}}]</math>, I only know that: |
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::* <math>\gamma(n)=1</math> for <math>n=1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 24, 25, 27, 30, 33, 35, 42, 45</math> (is there any other such <math>n</math>)? |
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::* If <math>m</math> divides <math>n</math>, then <math>\gamma(m)</math> also divides <math>\gamma(n)</math>, thus we can let <math>\varphi(n)=\prod_{d|n}\gamma(n)^{\mu(n/d)}</math> |
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::* For prime <math>p</math>, <math>p</math> divides <math>\varphi(p)</math> if and only if <math>p</math> is [[irregular prime|Bernoulli irregular prime]] |
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::* For prime <math>p</math>, <math>p</math> divides <math>\varphi(2p)</math> if and only if <math>p</math> is [[irregular prime|Euler irregular prime]] |
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::* <math>\varphi(n)=1</math> for <math>n=1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 24, 25, 27, 30, 33, 35, 42, 45</math> (is there any other such <math>n</math>)? |
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::* <math>\varphi(n)</math> is prime for <math>n=23, 26, 28, 32, 36, 37, 38, 39, 40, 43, 46, 49, 51, 53, 54, 63, 64, 66, 69, 75, 81, 96, 105, 118, 128, ...</math> (are there infinitely many such <math>n</math>?) |
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::Is there an algorithm to calculate <math>\gamma(n)</math> quickly? [[Special:Contributions/61.229.100.34|61.229.100.34]] ([[User talk:61.229.100.34|talk]]) 21:14, 8 December 2024 (UTC) |
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== Can we say anything special about every pair of functions f,g, satisfying f(g(x))=f(x) for every x? == |
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::I was also unclear about what you were asking. It is not usual to round to the nearest half, but if you really need to do this, then any value more than .00 and less than .25 gets rounded down, and so does any value more than .50 and less than .75<br>For values from .25 up to .50, and values from .75 up to the next whole number, the convention is to round up. [[User:Dbfirs|''<font face="verdana"><font color="blue">D</font><font color="#00ccff">b</font><font color="#44ffcc">f</font><font color="66ff66">i</font><font color="44ee44">r</font><font color="44aa44">s</font></font>'']] 20:01, 13 January 2010 (UTC) |
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Especially, is there an accepted term for such a pair? |
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= January 13 = |
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Here are three simple examples, for two functions f,g, satisfying the above, and defined for every natural number: |
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== Cube root function on the space Mn of matrices == |
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Example #1: |
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Hi all: |
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:f is constant. |
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Example #2: |
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I've been asked by my supervisor to investigate the possibility of the existence of a continuous square root function in some open ball about the identity matrix in <math>M_n</math>; that is, a continuous function g, with <math>[g(A)]^2=A</math> for all matrices A in this open ball about I. Now I've used the inverse function theorem and the fact that <math>f(A)=A^2</math> is continuously differentiable about I to prove that the inverse of f exists and is continuous in some open ball about I (an I-ball, as it were - oh dear...), but I also managed to prove that you can't extend such a function to the whole space <math>M_n</math>, because a matrix like, for example, |
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:f(x)=g(x), and is the smallest even number, not greater than x. |
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Example #3: |
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[0,1 |
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:f(x)=1 if x is even, otherwise f(x)=2. |
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:g(x)=x+2. |
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[[Special:Contributions/2A06:C701:746D:AE00:ACFC:490:74C3:660|2A06:C701:746D:AE00:ACFC:490:74C3:660]] ([[User talk:2A06:C701:746D:AE00:ACFC:490:74C3:660|talk]]) 09:31, 8 December 2024 (UTC) |
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: One way to consider such a pair is dynamically. If you consider the dynamical system <math>x\mapsto g(x)</math>, then the condition can be stated as "<math>f</math> is constant on <math>g</math>-orbits". More precisely, let <math>D</math> be the domain of <math>f,g</math>, which is also the codomain of <math>g</math>. Define an equivalence relation on <math>D</math> by <math>x\sim y</math> if <math>g^a(x)=g^b(y)</math> for some positive integers <math>a,b</math>. Then <math>f</math> is simply a function on the set of equivalence classes <math>D/\sim</math> (=space of orbits). In ergodic theory, such a function <math>f</math> is thought of as an "observable" or "function of state", being the mathematical analog of a thermodynamic observable such as temperature. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 11:52, 8 December 2024 (UTC) |
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0,0] |
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::After you've mentioned temprature, could you explain what are f,g, as far as temprature is concerned? Additionally, could you give another useful example from physics for such a pair of functions? [[Special:Contributions/2A06:C701:746D:AE00:ACFC:490:74C3:660|2A06:C701:746D:AE00:ACFC:490:74C3:660]] ([[User talk:2A06:C701:746D:AE00:ACFC:490:74C3:660|talk]]) 19:49, 8 December 2024 (UTC) |
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:::This equation is just the definition of function ''g''. For instance if function ''f'' has the inverse function ''f''<sup>−1</sup> then we have ''g(x)=x''. [[User:Ruslik0|Ruslik]]_[[User Talk:Ruslik0|<span style="color:red">Zero</span>]] 20:23, 8 December 2024 (UTC) |
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::: If f is the temperature, and g is the evolution of an ensemble of particles in thermal equilibrium (taken at a single time, say one second later), then because temperature is a function of state, one has <math>f(x)=f(g(x))</math> for all ensembles x. Another example from physics is when <math>g</math> is a Hamiltonian evolution. Then the functions <math>f</math> with this property (subject to smoothness) are those that (Poisson) commute with the Hamiltonian, i.e. "constants of the motion". [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 20:33, 8 December 2024 (UTC) |
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::::Thx. [[Special:Contributions/2A06:C701:746D:AE00:ACFC:490:74C3:660|2A06:C701:746D:AE00:ACFC:490:74C3:660]] ([[User talk:2A06:C701:746D:AE00:ACFC:490:74C3:660|talk]]) 10:43, 9 December 2024 (UTC) |
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:Let <math>f</math> be a function from <math>X</math> to <math>Y</math> and <math>g</math> a function from <math>X</math> to <math>X.</math> Using the notation for [[function composition]], the property under discussion can concisely be expressed as <math>f\circ g=f.</math> An equivalent but verbose way of saying the same is that the [[preimage]] of any set <math>B \subseteq Y</math> under <math>f</math> is [[Closure (mathematics)|closed]] under the application of <math>g.</math> --[[User talk:Lambiam#top|Lambiam]] 08:54, 9 December 2024 (UTC) |
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::Thx. [[Special:Contributions/2A06:C701:746D:AE00:ACFC:490:74C3:660|2A06:C701:746D:AE00:ACFC:490:74C3:660]] ([[User talk:2A06:C701:746D:AE00:ACFC:490:74C3:660|talk]]) 10:43, 9 December 2024 (UTC) |
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== IEEE Xplore paper claim to acheive exponentiation inversion suitable for pairing in polynomial time. Is it untrustworthy ? == |
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has no square root (I don't know how to LaTeX a matrix, sorry!). However, I couldn't find any such matrix which has no cube root: does there exist then a continuous 'cube root' function which extends to the whole of <math>M_n</math>? (I presume that every matrix does have a cube root, and so a discontinuous function would be fairly trivial by defining it pointwise, right?) My intuition tells me that no such function should exist - but how would I go about proving it? If not, why am I wrong? |
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I just found https://ieeexplore.ieee.org/abstract/document/6530387. Given the multiplicative group factorization in the underlying finite field of a target bn curve, they claim to acheive exponentiation inversion suitable for pairing inversion in seconds on a 32 bits cpu. |
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Thanks in advance for any responses, [[User:Typeships17|Typeships17]] ([[User talk:Typeships17|talk]]) 13:57, 13 January 2010 (UTC) |
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:The claim that every matrix has a cube root sounds highly unlikely, and in fact I think that |
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::<math>A=\begin{pmatrix}0&1&0\\0&0&1\\0&0&0\end{pmatrix}</math> |
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:is a counterexample. Let us assume that ''B''<sup>3</sup> = ''A'', and write ''B'' = ''P''<sup>−1</sup>''CP'', where ''P'' is invertible, and ''C'' is in Jordan normal form. Note that ''A'' = ''P''<sup>−1</sup>''C''<sup>3</sup>''P''. If ''J'' is a Jordan block of ''C'' with eigenvalue λ, then ''J''<sup>3</sup> appears as a block of ''C''<sup>3</sup>, and it is a triangular matrix with λ<sup>3</sup> on the diagonal, hence λ<sup>3</sup> is an eigenvalue of ''A''. However, the only eigenvalue of ''A'' is 0, hence λ = 0. Thus ''C'' is a triangular matrix with 0 on the diagonal, hence ''C''<sup>3</sup> is a triangular matrix whose main diagonal as well as two adjacent shifted diagonals are zero. As it is a 3-by-3 matrix, it is in fact the zero matrix, thus ''A'' = ''P''<sup>−1</sup>''C''<sup>3</sup>''P'' = 0, a contradiction. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 14:48, 13 January 2010 (UTC) |
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:Actually, now that I think about it, your matrix <math>\begin{pmatrix}0&1\\0&0\end{pmatrix}</math> should have no cube root either, by pretty much the same argument. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 14:55, 13 January 2010 (UTC) |
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On 1 side, the paper is supposed to be peer reviewed by the iee Xplore journal and they give examples on 100 bits. On the other side, in addition to the claim, their algorithm 2 and 3 are very implicit, and as an untrained student, I fail to understand how to implement them, though I fail to understand things like performing a Weil descent. |
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:The way I see it is: if N is any nilpotent nxn matrix, then N<sup>n</sup>=0 (because of the normal form of nilpotent matrices, which is just their Jordan form. Check also PST's hint to a close question [[#Nilpotent homomorphisms|below]]). This fact implies a necessary condition on the existence of a p-th root of N. Indeed if X<sup>p</sup>=N then X is nilpotent too, hence X<sup>n</sup>=0, therefore N is more nilpotent than X: N<sup>k</sup>=0 as soon as kp≥n. In particular a nilpotent N such that N<sup>n-1</sup>≠0 (for instance the above mentioned [[shift matrix]]) has no root of any order p>1. (not even if you allow complex coefficients) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 15:34, 13 January 2010 (UTC) |
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Is the paper untrustworthy, or would it be possible to get code that can be run ? [[Special:Contributions/2A01:E0A:401:A7C0:152B:F56C:F8A8:D203|2A01:E0A:401:A7C0:152B:F56C:F8A8:D203]] ([[User talk:2A01:E0A:401:A7C0:152B:F56C:F8A8:D203|talk]]) 18:53, 8 December 2024 (UTC) |
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:Also recall that an analytic p-th root in the unit ball around the identity is provided by the [[binomial series]], that works in any Banach algebra A. You may also like to investigate the set of all square roots of the identity: it is an analytic submanifold of A (in general not connected); the tangent space at ''x'' is given by the closed linear subspace V of all ''v'' that anti-commute with ''x'', that is ''vx=-xv''. Note that A splits as A=V⊕W where W is the closed linear subspace of all ''w'' that commute with x. --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 16:16, 13 January 2010 (UTC) |
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About the paper, I agree to share the paper privately [[Special:Contributions/2A01:E0A:401:A7C0:152B:F56C:F8A8:D203|2A01:E0A:401:A7C0:152B:F56C:F8A8:D203]] ([[User talk:2A01:E0A:401:A7C0:152B:F56C:F8A8:D203|talk]]) 18:54, 8 December 2024 (UTC) |
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If ever you forget how to LaTeX a particular mathematical notation, go to the corresponding Wikipedia article, click the "edit page" tab, and observe how the LaTeX is done. By repeatedly following this procedure, you will quickly learn how to LaTeX the given notation. For instance, to LaTeX a matrix, go to [[Matrix (mathematics)]], and notice that some examples of matrices are given at the beginning of the article. Now, click the "edit page" tab at the top, and you can observe the exact LaTeX for the particular matrix shown. At this point, it should not be difficult to duplicate the LaTeX for other matrices. Of course, you can also see how the above posters have written matrices in LaTeX, in this instance, by simply editing this section and viewing the underlying <nowiki><math></math></nowiki>. --[[User:Point-set topologist|<font color="#000000">PS</font>]][[User talk:Point-set topologist|<font color="#000000">T</font>]] 03:36, 14 January 2010 (UTC) |
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= December 9 = |
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In fact, in this case, I can give you an example of how to LaTeX a particular matrix: |
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== If the [[Mersenne number]] 2^p-1 is prime, then must it be the smallest [[Mersenne prime]] == 1 mod p? == |
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Visible LaTeX: |
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If the [[Mersenne number]] 2^p-1 is prime, then must it be the smallest [[Mersenne prime]] == 1 mod p? (i.e. there is no prime q < p such that 2^q-1 is also a [[Mersenne prime]] == 1 mod p) If p is prime (no matter 2^p-1 is prime or not), 2^p-1 is always == 1 mod p. However, there are primes p such that there is a prime q < p such that 2^q-1 is also a [[Mersenne prime]] == 1 mod p: |
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<nowiki><math> |
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\begin{bmatrix} |
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1 & 9 & 13 \\ |
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20 & 55 & 4 |
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\end{bmatrix}. |
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</math></nowiki> |
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* 2^19-1 is [[Mersenne prime]] == 1 mod 73 (p=73, q=19) |
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Appearance: |
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* 2^31-1 is [[Mersenne prime]] == 1 mod 151 (p=151, q=31) |
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* 2^61-1 is [[Mersenne prime]] == 1 mod 151 (p=151, q=61) |
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* 2^17-1 is [[Mersenne prime]] == 1 mod 257 (p=257, q=17) |
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* 2^31-1 is [[Mersenne prime]] == 1 mod 331 (p=331, q=31) |
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* 2^61-1 is [[Mersenne prime]] == 1 mod 331 (p=331, q=61) |
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* 2^127-1 is [[Mersenne prime]] == 1 mod 337 (p=337, q=127) |
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* 2^89-1 is [[Mersenne prime]] == 1 mod 353 (p=353, q=89) |
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* 2^89-1 is [[Mersenne prime]] == 1 mod 397 (p=397, q=89) |
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but for these primes p, 2^p-1 is not prime, and my question is: Is there a prime p such that 2^p-1 is a prime and there is a prime q < p such that 2^q-1 is also a [[Mersenne prime]] == 1 mod p? |
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<math> |
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\begin{bmatrix} |
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1 & 9 & 13 \\ |
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20 & 55 & 4 |
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\end{bmatrix}. |
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</math> |
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* If 2^11-1 is prime, then this is true, since 2^11-1 is == 1 mod 31 and 2^31-1 is prime, but 2^11-1 is not prime |
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For the matrix you mentioned, the following LaTeX works: |
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* If 2^23-1 or 2^67-1 is prime, then this is true, since 2^23-1 and 2^67-1 are == 1 mod 89 and 2^89-1 is prime, but 2^23-1 and 2^67-1 are not primes |
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* If 2^29-1 or 2^43-1 or 2^71-1 or 2^113-1 is prime, then this is true, since 2^29-1 and 2^43-1 and 2^71-1 and 2^113-1 are == 1 mod 127 and 2^127-1 is prime, but 2^29-1 and 2^43-1 and 2^71-1 and 2^113-1 are not primes |
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* If 2^191-1 or 2^571-1 or 2^761-1 or 2^1901-1 is prime, then this is true, since 2^191-1 and 2^571-1 and 2^761-1 and 2^1901-1 are == 1 mod 2281 and 2^2281-1 is prime, but 2^191-1 and 2^571-1 and 2^761-1 and 2^1901-1 are not primes |
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* If 2^1609-1 is prime, then this is true, since 2^1609-1 is == 1 mod 3217 and 2^3217-1 is prime, but 2^1609-1 is not prime |
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Another question: For any prime p, is there always a [[Mersenne prime]] == 1 mod p? [[Special:Contributions/220.132.216.52|220.132.216.52]] ([[User talk:220.132.216.52|talk]]) 19:03, 9 December 2024 (UTC) |
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Visible LaTeX: |
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: Neither question is easy. For the first, relations <math>2^{q-1}\equiv 1\pmod p</math> would imply that the integer 2 is not a primitive root mod p, and that its order divides <math>q-1</math> for the prime q. This is a sufficiently infrequent occurrence that it seems ''likely'' that all Mersenne numbers could be ruled out statistically, but not enough is known about their distribution. For the second, it is not even known if there are infinitely many Mersenne primes. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 19:23, 9 December 2024 (UTC) |
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<nowiki><math> |
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::I found that: 2^9689-1 is the smallest Mersenne prime == 1 mod 29, 2^44497-1 is the smallest Mersenne prime == 1 mod 37, 2^756839-1 is the smallest Mersenne prime == 1 mod 47, 2^57885161-1 is the smallest Mersenne prime == 1 mod 59, 2^4423-1 is the smallest Mersenne prime == 1 mod 67, 2^9941-1 is the smallest Mersenne prime == 1 mod 71, 2^3217-1 is the smallest Mersenne prime == 1 mod 97, 2^21701-1 is the smallest Mersenne prime == 1 mod 101, and none of the 52 known Mersenne primes are == 1 mod these primes p < 1024: 79, 83, 103, 173, 193, 197, 199, 227, 239, 277, 307, 313, 317, 349, 359, 367, 373, 383, 389, 409, 419, 431, 443, 461, 463, 467, 479, 487, 503, 509, 523, 547, 563, 587, 599, 613, 647, 653, 659, 661, 677, 709, 727, 733, 739, 743, 751, 757, 769, 773, 797, 809, 821, 823, 827, 829, 839, 853, 857, 859, 863, 887, 907, 911, 919, 929, 937, 941, 947, 971, 977, 983, 991, 1013, 1019, 1021 [[Special:Contributions/220.132.216.52|220.132.216.52]] ([[User talk:220.132.216.52|talk]]) 20:51, 9 December 2024 (UTC) |
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\begin{bmatrix} |
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::Also, |
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0 & 1 \\ |
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::* 2^19937-1 is [[Mersenne prime]] == 1 mod 2^16+1 |
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0 & 0 |
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::* 2^521-1 is [[Mersenne prime]] == 1 mod 2^13-1 |
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\end{bmatrix}. |
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::* 2^3021377-1 is [[Mersenne prime]] == 1 mod 2^17-1 |
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</math></nowiki> |
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::* 2^2281-1 is [[Mersenne prime]] == 1 mod 2^19-1 |
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::* 2^21701-1 is [[Mersenne prime]] == 1 mod 2^31-1 |
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::* 2^19937-1 is [[Mersenne prime]] == 1 mod 2^89-1 |
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::* 2^86243-1 is [[Mersenne prime]] == 1 mod 2^107-1 |
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::but none of these primes p has 2^p-1 is known to be prime, the status of 2^(2^89-1)-1 and 2^(2^107-1)-1 are still unknown (see [[double Mersenne number]]), but if at least one of them is prime, then will disprove this conjecture (none of the 52 known Mersenne primes are == 1 mod 2^61-1 or 2^127-1), I think that this conjecture may be as hard as the [[New Mersenne conjecture]]. [[Special:Contributions/220.132.216.52|220.132.216.52]] ([[User talk:220.132.216.52|talk]]) 20:55, 9 December 2024 (UTC) |
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::Also, for the primes p < 10000, there is a prime q < p such that 2^q-1 is also a [[Mersenne prime]] == 1 mod p only for p = 73, 151, 257, 331, 337, 353, 397, 683, 1321, 1613, 2113, 2731, 4289, 4561, 5113, 5419, 6361, 8191, 9649 (this sequence is not in [[OEIS]]), however, none of these primes p have 2^p-1 prime. [[Special:Contributions/220.132.216.52|220.132.216.52]] ([[User talk:220.132.216.52|talk]]) 02:23, 10 December 2024 (UTC) |
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= December 10 = |
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Appearance: |
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== More on the above conjecture == |
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<math> |
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\begin{bmatrix} |
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0 & 1 \\ |
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0 & 0 |
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\end{bmatrix}. |
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</math> |
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Above I posed: |
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It is simple if you try it a couple of times, and become accustomed to the LaTeX, but you are of course not obliged to do so (but just in case you wish to learn how to do so, I have included these tips). Hope this helps. --[[User:Point-set topologist|<font color="#000000">PS</font>]][[User talk:Point-set topologist|<font color="#000000">T</font>]] 03:43, 14 January 2010 (UTC) |
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:{{serif|'''Conjecture'''. ''Every prime number can be written in one of the three forms <math>a^2+b^2,</math> <math>2a^2+b^2</math> and <math>|2a^2-b^2|.</math>''}} |
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:And there's also [[Help:Formula]]. -- [[User:Meni Rosenfeld|Meni Rosenfeld]] ([[User Talk:Meni Rosenfeld|talk]]) 08:37, 14 January 2010 (UTC) |
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If true, it implies no natural prime is a prime in the ring <math>\mathbb Z[e^{\pi i/4}]</math>. |
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The absolute-value bars are not necessary. A number that can be written in the form <math>-(2a^2-b^2)</math> is also expressible in the form <math>+(2a^2-b^2).</math> |
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== finding the centre of a circle == |
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It turns out (experimentally; no proof) that a number that can be written in two of these forms can also be written in the third form. The conjecture is not strongly related to the concept of primality, as can be seen in this reformulation: |
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Firstly thanks for any help and if wiki has an article on this topic already then can you please point me in the right direction? |
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:{{serif|'''Conjecture'''. ''A natural number that cannot be written in any one of the three forms <math>a^2+b^2,</math> <math>2a^2+b^2</math> and <math>2a^2-b^2</math> is composite.}} |
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Anyway my problem is this i have a set of (x,y) co-ordinates randomly distributed inside a circle of radius R and i'd like to find out where the centre of the circle is. At best if we assume all points are evenly distributed over the circle then i guess calculating the mean of the (x,y)'s would yield the centre, but at worst, say all points clustered in one quadrant taking the straight mean would give a wrong answer. Is there a solution to this problem?--[[Special:Contributions/86.27.192.94|86.27.192.94]] ([[User talk:86.27.192.94|talk]]) 17:02, 13 January 2010 (UTC) |
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The first few numbers that cannot be written in any one of these three forms are |
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:<math>15,</math> <math>21,</math> <math>30,</math> <math>35,</math> <math>39,</math> <math>42,</math> <math>55,</math> <math>60,</math> <math>69,</math> <math>70,</math> <math>77,</math> <math>78,</math> <math>84,</math> <math>87,</math> <math>91,</math> <math>93,</math> <math>95.</math> |
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They are indeed all composite, but why this should be so is a mystery to me. What do <math>2310=2\times 3\times 5\times 7\times 11,</math> <math>5893=71\times 83</math> and <math>7429=17\times 19\times 23,</math> which appear later in the list, have in common? I see no pattern. |
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It seems furthermore that the [[primorial]]s, starting with <math>5\#=30,</math> make the list. (Checked up to <math>37\!\#=7420738134810.</math>) --[[User talk:Lambiam#top|Lambiam]] 19:23, 10 December 2024 (UTC) |
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:Without knowing the distribution, you cannot definitively state where the center is. By omitting points in one area of the circle, you have lost information and cannot recreate it. -- [[User:Kainaw|<font color='#ff0000'>k</font><font color='#cc0033'>a</font><font color='#990066'>i</font><font color='#660099'>n</font><font color='#3300cc'>a</font><font color='#0000ff'>w</font>]][[User talk:Kainaw|™]] 17:24, 13 January 2010 (UTC) |
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:No. If they are randomly distributed then the best you can do if find an expected value for the centre (whether that is the mean of the coordinates or not will depend on the details of the distribution). It would be unlikely that the points will be significantly skewed, so that expected centre should be close to the actual centre, but it is entirely possible for it to be a long way off. --[[User:Tango|Tango]] ([[User talk:Tango|talk]]) 17:27, 13 January 2010 (UTC) |
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:If you want something <s>non-random</s> ''defined as a function of the set of points'', then there is a unique closed disk of minimum radius containing your bounded set of points; it depends continuously on the set wrto the [[Hausdorff distance]]; it's indeed [[Lipschitz continuous]] of constant 1 --this is true in a Hilbert space too. --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 17:48, 13 January 2010 (UTC) |
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:Quick note, for those like me who are curious how numbers of the form <math>-(2a^{2}-b^{2})</math> can be written into a form of <math>2a^{2}-b^{2}</math>, note that <math>2a^{2} - b^{2} = (2a + b)^{2} - 2(a + b)^{2}</math>, and so <math>2a^{2} - b^{2} = -p \Rightarrow p = 2(a + b)^{2} - (2a + b)^{2}</math>. [[User:GalacticShoe|GalacticShoe]] ([[User talk:GalacticShoe|talk]]) 02:20, 11 December 2024 (UTC) |
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:Yet again Wikipedia has the answer - [[Smallest circle problem]]. [[User:Dmcq|Dmcq]] ([[User talk:Dmcq|talk]]) 18:44, 13 January 2010 (UTC) |
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:A prime is expressible as the sum of two squares if and only if it is congruent to <math>1 \!\!\!\pmod 4</math>, as per [[Fermat's theorem on sums of two squares]]. A prime is expressible of the form <math>2a^{2} + b^{2}</math> if and only if it is congruent to <math>1, 3 \!\!\pmod 8</math>, as per [[OEIS:A002479]]. And a prime is expressible of the form <math>2a^{2} - b^{2}</math> if and only if it is congruent to <math>1, 7 \!\!\pmod 8</math>, as per [[OEIS:A035251]]. Between these congruences, all primes are covered. [[User:GalacticShoe|GalacticShoe]] ([[User talk:GalacticShoe|talk]]) 05:59, 11 December 2024 (UTC) |
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:::: No, that's wrong. The "smallest circle problem" doesn't help here at all. Your comment seems very rash. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 05:07, 15 January 2010 (UTC) |
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::More generally, a number is ''not'' expressible as: |
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::That is really an answer to the OP's question, although it may be the best the we can do. The OP's circle has a fixed radius, though, so finding the smallest circle won't necessarily help. --[[User:Tango|Tango]] ([[User talk:Tango|talk]]) 18:54, 13 January 2010 (UTC) |
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::# <math>a^{2} + b^{2}</math> if it has a prime factor congruent to <math>3 \!\!\!\pmod 4</math> that is raised to an odd power (equivalently, <math>3, 7 \!\!\pmod 8</math>.) |
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:::<small>Sorry, I'm not sure I got what you meant: did you mean "That ''isn't'' "? Anyway. the OP question is interesting but clearly ill-posed. It's not even clear if R is known or not. So something has to be clarified and possibly changed. If the point is, ''to have a unique <s>non-random</s> solution'', then I suggested to modify the question as I wrote. --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 22:26, 13 January 2010 (UTC)</small> |
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::# <math>2a^{2} + b^{2}</math> if it has a prime factor congruent to <math>5, 7 \!\!\pmod 8</math> that is raised to an odd power |
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:::Assuming the distribution is uniformly random, i.e. each point in the circle has an equal chance of being sampled, can we give good estimators of center and radius? I guess in that case the best estimator for the center would indeed be the mean (and it should be unbiased, I think). If we have the center, the distance to the farthest point is a lower bound for the radius. As the sample size goes towards infinity, it should also converge against the true radius. However, for any finite set it's bound to underestimate the true radius. I suspect we can do better... --[[User:Stephan Schulz|Stephan Schulz]] ([[User talk:Stephan Schulz|talk]]) 18:55, 13 January 2010 (UTC) |
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::# <math>2a^{2} - b^{2}</math> if it has a prime factor congruent to <math>3, 5 \!\!\pmod 8</math> that is raised to an odd power |
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::::The OP says the radius is R, which I interpreted as meaning R is known, so we only need to worry about the centre. Assuming a uniform distribution (which actually means any region of the circle has a probability of being sampled equal to the ratio of its area to the area of the whole circle - if you look at individual points you just get the probability for every point is zero, which doesn't tell you much) then I agree that the mean should be unbiased. --[[User:Tango|Tango]] ([[User talk:Tango|talk]]) 19:29, 13 January 2010 (UTC) |
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::It is easy to see why expressibility as any two of these forms leads to the third form holding, and also we can see why it's difficult to see a pattern in numbers that are expressible in none of these forms, in particular we get somewhat-convoluted requirements on exponents of primes in the factorization satisfying congruences modulo 8. [[User:GalacticShoe|GalacticShoe]] ([[User talk:GalacticShoe|talk]]) 06:17, 11 December 2024 (UTC) |
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:::::I'd still like to know if we can estimate the radius as well... |
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:::Thanks. Is any of this covered in some Wikipedia article? --[[User talk:Lambiam#top|Lambiam]] 10:06, 11 December 2024 (UTC) |
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::::I can imagine some sets of points where the mean is not going to be the best estimate. For example if I have the points (0,0), (1,0), (2,0) and (100,0), I don't think this provides any different information than if I had only the points (0,0) and (100,0). <s>Wouldn't you also need some prior distribution on what the radii of the circles tend to be?</s> [[Special:Contributions/67.100.146.151|67.100.146.151]] ([[User talk:67.100.146.151|talk]]) 21:14, 13 January 2010 (UTC) |
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Assume p is 3 mod 4. Suppose that (2|p)=1. Then <math>x^4+1\equiv (x^2+\lambda x +1)(x^2- \lambda x + 1)\pmod p</math> where <math>\lambda^2-2\equiv 0</math>. Because the cyclotomic ideal <math>(p, \zeta^2+ \lambda\zeta+1)</math> has norm <math>p^2</math> and is stable under the Galois action <math>\zeta\mapsto 1/\zeta</math> it is generated by a single element <math>a\zeta^2+b\zeta+a</math>, of norm <math>(2a^2-b^2)^2</math>. |
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:::::Sure, in non-trivial cases you can always find a sample that will mis-estimate the distribution. The charm of an unbiased estimator is that for a random sequence it will stolastically converge to the true value. --[[User:Stephan Schulz|Stephan Schulz]] ([[User talk:Stephan Schulz|talk]]) 21:40, 13 January 2010 (UTC) |
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::::::(the IP 67... is me.) <s>Actually I was wrong. The two cases give different information by merit of the fact that they have a different number of points.</s> But the idea still holds. A simple average is not the best you can do. |
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::::::::: I expect one could readily prove that on average the "simple average" performs considerably better than the center of the smallest disk enclosing the data. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 03:20, 14 January 2010 (UTC) |
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::::::Edit: Sorry, didn't notice that the OP specified that the radius is already known. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 22:42, 13 January 2010 (UTC) |
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If (2|p)=-1, then the relevant ideal is stable under <math>\zeta\mapsto -1/\zeta</math> and so is generated by <math>a\zeta^2+b\zeta-a</math>, of norm <math>(2a^2+ b^2)^2</math>. [[User:Tito Omburo|Tito Omburo]] ([[User talk:Tito Omburo|talk]]) 14:43, 11 December 2024 (UTC) |
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:We can find the region S<sub>R</sub> formed by the centers of all possible circles of radius R that enclose the points in the initial set (it'll be the intersection of the disks of radius R centered at each point in the set). I'm pretty sure there's an even distribution of where the center is likely to be in S<sub>R</sub>. We can think about if we pick a circle and then choose points at random, the chance of the points being clustered in one region of the circle is the same as it is in any other. So the average location of the center over all those possible circles should be the [[centroid]] of S<sub>R</sub>. I don't know if there's a straight forward way to calculate that though. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 22:50, 13 January 2010 (UTC) |
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::If I understand what you said, S<sub>R</sub> is the disk with the same center as the minimal disk, and radius R-r (r being the radius of the minimal disk). Correct?--[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 23:14, 13 January 2010 (UTC) |
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:::S<sub>R</sub> contains that disk of radius R-r, but I think it will generally be larger since a disk of radius R that contains the points in the set doesn't have to contain the minimal disk. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 23:48, 13 January 2010 (UTC) |
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::::<small>right :) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 00:04, 14 January 2010 (UTC)</small> |
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= December 11 = |
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A few points about the discussion above: |
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* Tango writes of an [[expected value]] of the center. The average location of observed points is the expected value only of the discrete distribution of the set of points actually observed; it's not the expected value of the center. Only if there's a prior distribution, and hence a posterior distribution, can you speak of an expected value of the center. |
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* The observed average is indeed [[unbiased estimator|unbiased]]. |
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* pma proposed unique smallest disk enclosing the observed points is not "non-random" if those observed points are random. |
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* One should be able to find confidence regions for the center; these would be large if the number of points is small. I'd have to work out details though. |
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: |
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[[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 03:16, 14 January 2010 (UTC) |
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::I think people (at least I was) were working under the assumption that the prior distribution of the center is an even distribution on '''R'''<sup>2</sup> (or on some really large closed disk if that makes more sense. As long as the points in the set aren't near the edge it doesn't matter). I'm not really sure confidence regions are really useful here, unless I'm misunderstanding the problem. There's a well defined region where the center could be, and the posterior probability is evenly distributed across it. Outside that region the probability is zero. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 05:14, 14 January 2010 (UTC) |
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:::::::: "posterior probability is evenly distributed across it" That is '''WRONG'''. I didn't even notice this comment the first time I commented. The posterior probability, with any reasonable prior, would be highly concentrated near the mean of the data points, and get less concentrated as you moved further away, and the distribution would have unbounded support unless the prior (i.e. pre-data) distribution had bounded support. Your comments are really seriously confused. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 05:04, 15 January 2010 (UTC) |
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:::::::::That's why I said "(or on some really large closed disk if that makes more sense. As long as the points in the set aren't near the edge it doesn't matter)". Obviously you can't really have an even distribution on the whole plane, but an even distribution on any large bounded region doesn't effect the outcome of the problem as long as the points are not within 2R of the edge of the region. We can essentially ignore its specific properties. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 05:33, 15 January 2010 (UTC) |
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::::: You seem confused. The uniform distribution on the whole plane is not a proper probability distribution; it assigns infinite measure to the whole space. I doubt that's what people assumed. I think they were assuming the DATA are uniformly distributed, not within the whole plane, but within the interior of the circle. That is NOT a prior distribution of the center of the circle. Given the data, the center of the circle COULD be anywhere in the plane, even quite remote from a disk-like cloud of data point, but that's improbable---it means by some accident all the points landed close together, far from the center. At any rate, "prior" and "posterior" refer to the probability distribution of the center, not of the data. Using frequentist methods, one wouldn't usually have prior and posterior distributions, but only a distribution of the data. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 04:54, 15 January 2010 (UTC) |
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::::::The only explanation I have for what you're saying is that you're thinking about a quite different problem than I am. Here is the problem as I understood it: You have some large large bounded region of the plane and you choose a point P at random according to an even distribution on the region. Then you draw a circle of radius R centered at P and pick some number of points at random from inside the circle according to a even distribution on that disk. Given that set of points and the radius R, describe the probability of where P lies. |
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::::::In the context of that problem, P cannot lie farther than R from any of the points in the set. It CAN'T be anywhere in the plane, rather it's restricted to the region S<sub>R</sub> that I described above. Moreover, the posterior distribution is an even distribution on S<sub>R</sub>. |
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::::::Maybe you are assuming that R is not given? In that case (a) you need to know a prior distribution of the values the radius can take in order to answer the question (as I said and then crossed out when I modified my interpretation of the question) and (b) the prior distribution for the location of P that I described makes less sense since the edge effects will always matter for any set of data points, unless the prior for the radius is bounded. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 05:33, 15 January 2010 (UTC) |
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:::::::: OK, I think I did neglect that fact that ''R'' is known. That apparently does simplify things a lot. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 07:18, 15 January 2010 (UTC) |
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:::<small>yea, this seems a pretty good description (what else could be said?) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 06:26, 14 January 2010 (UTC)</small> |
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Study a simplified problem first. Consider the one-dimensional case of points inside the interval ''a''<''x''<''a''+1, and estimate ''a''. [[User:Bo Jacoby|Bo Jacoby]] ([[User talk:Bo Jacoby|talk]]) 08:12, 14 January 2010 (UTC). |
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:OP here, thanks for the help so far if it helps i'll describe the actual situation, i initially said "taking point (A,B) get all data within a circle of radius R, now some time later (after losing track of the individual (A,B)), i have all the data points and would like to reconstruct the original (A,B), or even just the best guess at what it would be--[[Special:Contributions/86.27.192.94|86.27.192.94]] ([[User talk:86.27.192.94|talk]]) 08:37, 14 January 2010 (UTC) |
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::Well that gives a whole lot more information. You have a whole lot of points which weren't within radius R, so this circle of radius R must be somewhere in the gap between these two sets of points. For instance if you were choosing all towns of more than 10000 inhabitants within 10 miles of a point you might only get three towns and the towns you didn't choose might be as good or better at determining the point. |
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:::Where the problem given the points inside determines a convex polygon with curved sides of radius R within which the center must lie, excluding points means you have sides that bend the other way and the figure isn't convex. The corners where the curves intersect still form a convex figure though as far as I can see so it should be a fairly reasonable problem for a computer program. [[User:Dmcq|Dmcq]] ([[User talk:Dmcq|talk]]) 09:31, 14 January 2010 (UTC) |
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== Unique normal ultrafilter == |
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Sigh. OK, I wrote some comments neglecting the fact that ''R'' is known. '''But''' some of what's said about makes me think some people are confusing the terms "prior" and "posterior" with the distribution of the DATA given the location of the center. [[User:Michael Hardy|Michael Hardy]] ([[User talk:Michael Hardy|talk]]) 05:20, 15 January 2010 (UTC) |
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So I'm supposed to know the answer to this, I suppose, but I don't seem to :-) |
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:I think I'll sigh even deeper. If you consider the points which aren't included the possible positions of the centre with a fixed ''R'' needn't even be connected never mind anywhere near convex. If you have three points excluded at the corners of an equilateral triangle and one included point at the centre then with ''R'' = half the length of a side or a bit more you get four completely separate areas where the centre can be. [[User:Dmcq|Dmcq]] ([[User talk:Dmcq|talk]]) 09:29, 15 January 2010 (UTC) |
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"Everyone knows" that, in <math>L[U]</math>, [[Gödel's constructible universe]] relative to an [[ultrafilter]] <math>U</math> on some [[measurable cardinal]] <math>\kappa</math>, there is only a single [[normal ultrafilter]], namely <math>U</math> itself. See for example [[John R. Steel]]'s monograph [https://math.berkeley.edu/~steel/papers/comparisonlemma.03.07.22.pdf here], at Theorem 1.7. |
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:By the way using Bo Jacoby's very simple version of an interval of length 1 the midpoint of the interval containing the samples is a better estimate of the center of the interval than the mean - see [[Uniform_distribution_(continuous)#Estimation of midpoint]]. Generalizing to the circle case and ignoring any points outside I'd be pretty certain the center of the minimum circle would be a better estimate of the center than the mean though of course working out S<sub>R</sub> as above would give a better estimate. In fact just getting the midpoint of the minimum and maximum ''x'' and ''y'' values would probably be a good quick and dirty way of estimating the center. [[User:Dmcq|Dmcq]] ([[User talk:Dmcq|talk]]) 13:20, 15 January 2010 (UTC) |
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So I guess that must mean that the [[product measure]] <math>U\times U</math>, meaning you fix some identification between <math>\kappa\times\kappa</math> and <math>\kappa</math> and then say a set has measure 1 if measure 1 many of its vertical sections have measure 1, must ''not'' be normal. (Unless it's somehow just equal to <math>U</math> but I don't think it is.) |
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== Nilpotent homomorphisms == |
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But is there some direct way to see that? Say, a <s>continuous</s> function <math>f:\kappa\to\kappa</math> with <math>\forall\alpha f(\alpha)<\alpha</math> such that <s>the set of fixed points of <math>f</math> is not in the ultrafilter</s> no singleton has a preimage under <math>f</math> that's in the ultrafilter? I haven't been able to come up with it. --[[User:Trovatore|Trovatore]] ([[User talk:Trovatore|talk]]) 06:01, 11 December 2024 (UTC) |
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Let A∈Hom<sub>K</sub>(K<sup>n</sup>,K<sup>n</sup>) and n∈ℕ. Which consequences has the fact that A<sup>2</sup>=0? --[[Special:Contributions/84.61.151.145|84.61.151.145]] ([[User talk:84.61.151.145|talk]]) 17:50, 13 January 2010 (UTC) |
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:For instance, it has a [[nilpotent matrix#Classification|normal form]] with 2x2 blocks (plus some 1x1 0 blocks, at least one if n is odd), hence few 1's (at most n/2). --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 17:55, 13 January 2010 (UTC) |
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= December 12 = |
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What about Im(A) and Ker(A)? --[[Special:Contributions/84.61.151.145|84.61.151.145]] ([[User talk:84.61.151.145|talk]]) 18:03, 13 January 2010 (UTC) |
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:Of course Im(A) is included in ker(A) (so e.g. the quotient H=ker(A)/im(A) is well defined); further information may be seen via the normal form above. Now that you say it, I have a vague memory that somebody in some book defines a "module with differentiation" to be a module M with an endomorphism A such that A<sup>2</sup>=0, as an elementary example of [[chain complex]]. I think I saw it in Jacobson's "Basic Algebra II" (typical of it). --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 18:08, 13 January 2010 (UTC) |
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The way in which these questions were phrased suggests that they constitute homework. As pma has already confirmed that Im(''A'') is contained in Ker(''A''), the OP might like to consider the following exercise. If ''V'' is an ''n''-dimensional vector space over a field ''K'', and ''A'' is a linear transformation of ''V'' over ''K'' with the property that ''A''<sup>p</sup> = 0 for some ''p'', show that ''A''<sup>n</sup> = 0 (''n'' is the dimension of ''V'' over ''K''). A hint is hidden below, but make a solid attempt at the problem before viewing the hint to attain a satisfactory intuition of nilpotent transformations. |
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{{hidden |
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|(Click the "show" button at the right to see the hint or the "hide" button to hide it.) |
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|2= |
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''Prove that <math> \{0\} \subset \ker A \subset \ker A^2 \subset \ldots \subset \ker A^{p-1} \subset \ker A^p = V</math> is an ascending chain of subspaces (that each inclusion is indeed correct).''}} |
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Hope this helps but please note that in order to learn anything, you must show us that you have made an attempt at the problem. Simply firing questions at us in quick succession will not aid your intuition of nilpotent transformations. --[[User:Point-set topologist|<font color="#000000">PS</font>]][[User talk:Point-set topologist|<font color="#000000">T</font>]] 03:29, 14 January 2010 (UTC) |
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How to prove that K<sup>n</sup> has a basis B with <sub>B</sub>A<sub>B</sub>=<math>\begin{pmatrix} |
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0 & 0 \\ |
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I_r & 0 |
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\end{pmatrix}</math>, where r is the rank of A? --[[Special:Contributions/84.61.165.65|84.61.165.65]] ([[User talk:84.61.165.65|talk]]) 15:18, 14 January 2010 (UTC) |
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:If you trust the above normal form, note that the number of 2x2 blocks in it is ''r'', and that that matrix differs from the one you wrote only by a permutation of the base. If you want an independent proof, start with PST's hint. --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 20:30, 14 January 2010 (UTC) |
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Your most recent question suggests that you have not yet attempted to visualize the linear operator ''A''. Visualization can prove an important tool in determining canonical forms, and thus it may increase your chances of solving the questions you pose. Personally, I feel that your most recent question should not require a formal proof in that it is very intuitive; you need only formally pinpoint the intuition (which is done in my hint above). Since you are unable to solve it, either you do not have any intuition of ''A'' at all, or you do not know how to construct a mathematical proof. If the former, please read my hint and pma's responses carefully. If the latter, we cannot help you. If neither, it is very difficult to decide exactly that which you are asking, especially with the wording "How to prove...". I do not intend to discourage you from asking questions here but please provide context (rather than merely fire questions at us). --[[User:Point-set topologist|<font color="#000000">PS</font>]][[User talk:Point-set topologist|<font color="#000000">T</font>]] 03:26, 15 January 2010 (UTC) |
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== 35 degrees east == |
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Since [[Indo-Australian Plate]] said 35 degrees east and the total plate is 67 mm then how many meters north. If is 35 degrees east would east be 10 mm and north be 50 mm?--[[Special:Contributions/209.129.85.4|209.129.85.4]] ([[User talk:209.129.85.4|talk]]) 21:27, 13 January 2010 (UTC) |
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:Since the plate is moving 35 degrees east of north (that is, it's moving NNE), and moving at a rate of 67 mm per year, you can find how fast the plate is moving in both the East-West and North-South direction by drawing a [[right triangle]] (with the [[cathetus|legs]] lined up along the North-South and East-West directions, and a [[Hypotenuse]] of 67 mm/yr) and using [[trigonometry]] to determine the lengths of the legs. The plate is moving somewhat faster to the north than you guessed, and significantly faster to the east. Does someone know a good way to get a diagram in here? [[User:Buddy431|Buddy431]] ([[User talk:Buddy431|talk]]) 02:00, 14 January 2010 (UTC) |
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::Oh, you're talking about ''movement''! I couldn't get any sense at all out of the question. --[[User:ColinFine|ColinFine]] ([[User talk:ColinFine|talk]]) 08:18, 14 January 2010 (UTC) |
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:::Simplistic solution is that northwrds component of velocity is 67 cos(35 degrees) = 54.9 mm/yr and eastwards component is 67 sin(35 degrees) = 38.4 mm/yr. However, as the figure given for the plate's velocity is an average of small movements over a large geographic area and over a long period time, this notional calculation of northwards and eastwards components is probably over-simplifying a much more complex pattern of movement. Different places on the plate boundary may be moving at different rates. [[User:Gandalf61|Gandalf61]] ([[User talk:Gandalf61|talk]]) 10:58, 14 January 2010 (UTC) |
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= January 14 = |
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== An elementary homotopy equivalence == |
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Continuing with my attempts to grasp the basics of quotient spaces and homotopy, I find myself quickly running into trouble when trying to show that two simple spaces are homotopically equivalent. Consider, for example, the [http://books.google.com/books?id=G74V6UzL_PUC&pg=PA50 problem] of showing that the two spaces "''S''<sup>2</sup> with a straight line joining north and south poles" and "[[wedge sum]] of ''S''<sup>2</sup> with a circle" are homotopically equivalent. |
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I can intuitively see some vague ways of deforming these spaces into each other; for example, one can take the second space and imagine the circle standing inside ''S''<sup>2</sup> and joined at the north pole, and then quotient half the circle into the side of the sphere; the result should by rights be homeomorphic to the first space. But when it comes to actually writing down explicit maps or homotopies, I'm lost; the text (linked above) is rather light on examples, so it's not even clear what a correct solution would look like. How do topologists approach problems like this? — [[User:merge|<span style="color:#333">m</span><span style="color:#555">e</span><span style="color:#888">r</span><span style="color:#aaa">g</span><span style="color:#ccc">e</span>]] 12:30, 14 January 2010 (UTC) |
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:This is example 0.8 in Hatcher's ''Algebraic Topology'' (relevant chapter [http://www.math.cornell.edu/~hatcher/AT/ATch0.pdf here]). He does it by collapsing a curve in the sphere from N to S to a point, using some general technical lemmas to make this precise. [[User talk:Algebraist|Algebraist]] 13:17, 14 January 2010 (UTC) |
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::Hmm. Thanks for the reference, but it doesn't seem of much use for this problem; in Bredon's book, it's posed in Chapter 1 just after introducing the most basic definitions and properties of homotopy. There are certainly no CW-complexes in sight, and no propositions about homotopy equivalence of quotient spaces (at least that I can identify as such). — [[User:merge|<span style="color:#333">m</span><span style="color:#555">e</span><span style="color:#888">r</span><span style="color:#aaa">g</span><span style="color:#ccc">e</span>]] 16:23, 14 January 2010 (UTC) |
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::: Here's an approach that might help. Imagine the sphere as a (hollow) cube and line as a semicircular "handle" above two points near the centre of one face of the cube. Now apply a homotopy that moves the two points together while preserving the boundary of the cube - it should be reasonably easy to define an explicit formula to do this. Extend to the whole cube using the identity map on the other faces, and you're done (messy details left as an exercise..) <small>(Disclaimer - it's been a long time since I did this sort of thing)</small> [[User:AndrewWTaylor|AndrewWTaylor]] ([[User talk:AndrewWTaylor|talk]]) 17:16, 14 January 2010 (UTC) |
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:::Just because the approach of using CW complexes and a few technical lemmas isn't the ''intended'' approach of your text doesn't mean it can't be the ''best'' approach to such problems. Hatcher clearly thinks it is. [[User talk:Algebraist|Algebraist]] 17:28, 14 January 2010 (UTC) |
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:::: I have no opinion on what approach is best; just trying to solve the problem with the tools I've been given. — [[User:merge|<span style="color:#333">m</span><span style="color:#555">e</span><span style="color:#888">r</span><span style="color:#aaa">g</span><span style="color:#ccc">e</span>]] 19:31, 14 January 2010 (UTC) |
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:::: To AndrewWTaylor: Your homotopy takes place outside of both spaces, so with the same reasoning the OP's first space is homotopic to the sphere, which is impossible because one has a non-trivial fundamental group and the other doesn't. Correct me if I'm wrong I'm a novice. [[User:Money is tight|Money is tight]] ([[User talk:Money is tight|talk]]) 17:34, 14 January 2010 (UTC) |
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:I recall being messily taught this example in an introductory algebraic topology course - the lecturer used a (non-obvious) [[deformation retraction]] of both spaces onto a common space...but I can't fully recall what that was. Not that that matters really, since Brenon seems to want it done using basic definitions. [[User:Icthyos|Icthyos]] ([[User talk:Icthyos|talk]]) 19:19, 14 January 2010 (UTC) |
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::Heh. This section does contain definitions for deformation retracts and some homotopy properties of mapping cylinders, for what it's worth. :) If this problem is bad, the next two problems on the page must be much worse... — [[User:merge|<span style="color:#333">m</span><span style="color:#555">e</span><span style="color:#888">r</span><span style="color:#aaa">g</span><span style="color:#ccc">e</span>]] 19:31, 14 January 2010 (UTC) |
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:How about this: If X is the one-point union of the sphere and the circle at point x<sub>0</sub> and Y is the other space, let f:Y → X map the points on the closed left side of the Y sphere to x<sub>0</sub> and the rest of the Y sphere to the X sphere minus x<sub>0</sub>, and then the line gets mapped to the circle minus x<sub>0</sub> in the way you'd expect. Then let g:X → Y map the X sphere to the Y sphere identically with the point x<sub>0</sub> at the north pole and then map half of the circle to the line connecting the poles and the other half to a path along the left side of the sphere connecting the poles. I'm pretty sure fg and gf are homotopic to 1 but it might be annoying to show. [[User:Rckrone|Rckrone]] ([[User talk:Rckrone|talk]]) 22:10, 14 January 2010 (UTC) |
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::I've come up with a couple of ideas along these lines, but it always ends up seeming far from obvious how to even show the maps in question are continuous. — [[User:merge|<span style="color:#333">m</span><span style="color:#555">e</span><span style="color:#888">r</span><span style="color:#aaa">g</span><span style="color:#ccc">e</span>]] 23:35, 14 January 2010 (UTC) |
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:::Yeah, that's fairly similar to the attempt at a solution I provided - I was told it wasn't clear that the compositions of f and g were homotopic to the identity maps, then we moved on to some hand-waving. [[User:Icthyos|Icthyos]] ([[User talk:Icthyos|talk]]) 00:21, 15 January 2010 (UTC) |
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== Consecutive integers with same sum of proper divisors == |
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At one point, I was having trouble remembering the definition of [[Ruth-Aaron pair]]s, and that got me into some other interesting questions. |
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* Are there pairs of consecutive integers with the same sum of all their divisors? Yes. (14,15) and (206,207) are the first two such pairs; this is {{OEIS|A002961}}. |
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* What if we look only at proper divisors? (2,3) works and there are no others under 5,000. Note that this sum is always the same parity as the number itself, unless the number is a square or twice a square, so if we want two consecutive ones to be the same, then one of them must be of that type. Before I spend a lot of time programming this to at least start things off, it would be useful to know if there is already a result in the literature. |
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[[User:Matchups|Ma]]<sup>[[User talk:Matchups|t]]</sup><sub>[[Special:Contributions/Matchups|c]]</sub>[[User:Matchups|hups]] 14:48, 14 January 2010 (UTC) |
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= January 15 = |
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== Is there a name for this property of sets? == |
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Is there a name for the property of sets that its [[Axiom of union|union set]] is itself? For example, the [[Set-theoretic definition of natural numbers#The contemporary standard|natural numbers under the standard construction]] satisfy this property. --[[Special:Contributions/129.116.47.169|129.116.47.169]] ([[User talk:129.116.47.169|talk]]) 00:25, 15 January 2010 (UTC) |
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:I'd say that such a set is ordered by <math>\in</math> hence well ordered because it is explicitly required by ZF;<s> it's an ordinal.</s> --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 09:20, 15 January 2010 (UTC) |
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::No, it doesn't have to be an ordinal (nor do all ordinals qualify). For example ''V''<sub>ω</sub> has the desired property, but 1 (understood as <math>\{\emptyset\}</math>) does not; its union is just <math>\emptyset</math>. It would have to be a [[transitive set]], but not all transitive sets work (e.g. 1 again). I don't know of a specific name for the property. --[[User:Trovatore|Trovatore]] ([[User talk:Trovatore|talk]]) 09:26, 15 January 2010 (UTC) |
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:::ach I realized it and was just on the point of correcting it but you are too fast :-) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 09:31, 15 January 2010 (UTC) So we may rephrase the assumption on such a set X saying it's a transitive set without "maximal element" wrto the relation <math>\in</math> (into commas because <math>\in</math> needn't to be transitive as a relation on X; X has no maximal element wrto <math>\in</math> in the sense that for any <math>x \in X</math> there is <math>y \in X</math> such that <math>x\in y</math> ) --[[User:PMajer|pm]][[User talk:PMajer|<span style="color:blue;">a</span>]] 09:38, 15 January 2010 (UTC) |
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== Is a set that contains only itself hereditary? == |
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In the process of copyediting [[hereditary set]], I found myself writing the sentence |
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:''In [[non-well-founded set theories]] where such objects are allowed, a set that contains only itself is also a hereditary set.{{fact}}'' |
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It then occurred to me not only that this may or may not be true, but that it might not even be a meaningful statement. Consider the set E = {E}. By the definition of hereditary sets, if E is hereditary, then {E} is hereditary, which merely restates the initial premise. If E isn't hereditary, then E isn't hereditary, again restating the inital premise. I can't see how to get a better handle on this problem. Can anyone help? -- [[User:The Anome|The Anome]] ([[User talk:The Anome|talk]]) 14:59, 15 January 2010 (UTC) |
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:The usual way to unambiguously phrase such definitions in non-well-founded set theories is to define that ''A'' is a hereditary xxx iff every object in the transitive closure of {''A''} is a xxx (note that this is equivalent to the inductive definition if the universe is well-founded). Your ''E'' is thus indeed a hereditary set. — [[User:EmilJ|Emil]] [[User talk:EmilJ|J.]] 15:09, 15 January 2010 (UTC) |
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::Thanks! Could you, or anyone else with good set theory knowledge, please update the [[hereditary set]] article to reflect this? I'm afraid I'm outside my area of competence here. -- [[User:The Anome|The Anome]] ([[User talk:The Anome|talk]]) 15:12, 15 January 2010 (UTC) |
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== Continuity of power functions == |
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How to prove the continuity of all functions f: ℝ→ℝ, f(x)=|x|^a, a>0, in x=0? --[[Special:Contributions/84.61.165.65|84.61.165.65]] ([[User talk:84.61.165.65|talk]]) 15:30, 15 January 2010 (UTC) |
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November 29
[edit]In finite fields of large characteristics, what does prevent shrinking the modulus field size down to their larger order in order to solve discrete logarithms ?
[edit]In the recent years, several algorithms were proposed to leverage elliptic curves for lowering the degree of a finite field and thus allow to solve discrete logairthm modulo their largest suborder/subgroup instead of the original far larger finite field. https://arxiv.org/pdf/2206.10327 in part conduct a survey about those methods. Espescially since I don’t see why a large chararcteristics would be prone to fall in the trap being listed by the paper.
I do get the whole small characteristics alogrithms complexity makes those papers unsuitable for computing discrete logarithms in finite fields of large charateristics, but what does prevent applying the descent/degree shrinking part to large characteristics ? 2A01:E0A:401:A7C0:68A8:D520:8456:B895 (talk) 11:00, 29 November 2024 (UTC)
- Try web search for Lim-Lee small subgroup attack. 2601:644:8581:75B0:0:0:0:C426 (talk) 23:09, 1 December 2024 (UTC)
- First the paper apply when no other information is known beside the 2 finite field’s elements and then this is different from https://arxiv.org/pdf/2206.10327. While Pollard rho can remain more efficient, if the subgroup is too large, then it’s still not enough fast. I’m talking about shrinking modulus size directly. 2A01:E0A:401:A7C0:69D2:554C:93AF:D6AC (talk) 15:17, 2 December 2024 (UTC)
The problem with descent methods like the one described in large characteristic is that the complexity is . This is explained more clearly in [1]. If the characteristic is small, then the problem is O(k) bits, and the complexity id pseudo-polynomial in the number of bits. If the characteristic is large, then the compexity is which is exponential in the number of bits of q. Tito Omburo (talk) 16:36, 2 December 2024 (UTC)
- Are you sure ? I’m not talking about the complexity of the index calculus part like chosing the factor base or computing individual discrete logarithms or the linear algebra phase. Only about the part consisting of shrinking the modulus through lowering it’s degree… 82.66.26.199 (talk) 10:26, 3 December 2024 (UTC)
- The paper I cited above finds the intermediate polynomials by a brute force search in small degree, which is thus polynomial in q. The general heuristic is that the search for intermediate polynomials takes about as long as the index calculus phase. But it looks like no one has a really good way to do it. Tito Omburo (talk) 10:45, 3 December 2024 (UTC)
- And in my case, elliptic curves are used to lower the degree and thus the modulus instead of brutefore. The person who wrote the paper told me in fact the idea was developed initially for medium characteristics but refused to give details for large characteristics. 82.66.26.199 (talk) 11:06, 3 December 2024 (UTC)
- I'm not really convinced that the approach actually works. How are the elliptic curves constructed? The construction given is very implicit. I'm betting that if one actually writes out the details, it involves lifting something from the prime field. Tito Omburo (talk) 16:02, 3 December 2024 (UTC)
- Yes. My request to have more details wasn’t well received. https://sympa.inria.fr/sympa/arc/cado-nfs/2024-12/msg00002.html 2A01:E0A:401:A7C0:5985:1F5D:4595:AA09 (talk) 01:48, 4 December 2024 (UTC)
- I'm not really convinced that the approach actually works. How are the elliptic curves constructed? The construction given is very implicit. I'm betting that if one actually writes out the details, it involves lifting something from the prime field. Tito Omburo (talk) 16:02, 3 December 2024 (UTC)
- And in my case, elliptic curves are used to lower the degree and thus the modulus instead of brutefore. The person who wrote the paper told me in fact the idea was developed initially for medium characteristics but refused to give details for large characteristics. 82.66.26.199 (talk) 11:06, 3 December 2024 (UTC)
- The paper I cited above finds the intermediate polynomials by a brute force search in small degree, which is thus polynomial in q. The general heuristic is that the search for intermediate polynomials takes about as long as the index calculus phase. But it looks like no one has a really good way to do it. Tito Omburo (talk) 10:45, 3 December 2024 (UTC)
November 30
[edit]Linear differential function
[edit]Differential 102.213.69.166 (talk) 04:35, 30 November 2024 (UTC)
- What are you talking about? ‹hamster717🐉› (discuss anything!🐹✈️ • my contribs🌌🌠) 14:02, 30 November 2024 (UTC)
December 4
[edit]How much is this
[edit]37.162.46.235 (talk) 11:00, 4 December 2024 (UTC)
- 1 for n even, 0 for n odd. For see Grandi's series. --Wrongfilter (talk) 11:18, 4 December 2024 (UTC)
- I hope this is not homework. Note that (for finite ) this is a finite geometric series. --Lambiam 21:51, 4 December 2024 (UTC)
December 6
[edit]Is there anything that would prevent peforming Weil Descent on binary curves of large characteristics ?
[edit]The ghs attack involve creating an hyperlliptic curve cover for a given binary curve. The reason the attack fails most of the time is the resulting genus grows exponentially relative to the curve’s degree.
We don’t hear about the attack on finite fields of large characteristics since such curves are already secure by being prime. However, I notice a few protocol relies on the discrete logarithm security on curves with 400/500 bits modulus resulting from extension fields of characteristics that are 200/245bits long.
Since the degree is most of the time equal to 3 or 2, is there anything that would prevent creating suitable hyperelliptic cover for such curves in practice ? 2A01:E0A:401:A7C0:28FE:E0C4:2F97:8E08 (talk) 12:09, 6 December 2024 (UTC)
December 7
[edit]Mathematical operation navigation templates
[edit]RDBury is right, this discussion belongs at Wikipedia talk:WikiProject Mathematics |
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The following discussion has been closed. Please do not modify it. |
If anyone with some mathematical expertise is interested, I'd appreciate some additional input at Talk:Exponentiation#funny table at end. The question is whether our articles on various mathematical operations could use a navigational template (aka "{{Navbox}}"). Our Exponentiation article tried to use {{Mathematical expressions}} for this purpose, but it doesn't really work. I've created {{Mathematical operations}} as a potential alternative, but the categorization and presentation I've created is probably naïve. (The whole effort may or not be worth it at all.) —scs (talk) 00:36, 7 December 2024 (UTC)
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December 8
[edit]For each positive integer , which primes are still primes in the ring ?
[edit]For each positive integer , which primes are still primes in the ring ? When , is the original integer ring, when , is the ring of Gaussian integers, when , is the ring of Eisenstein integers, and the primes in the Gaussian integers are the primes , and the primes in the Eisenstein integers are the primes , but how about larger ? 218.187.66.163 (talk) 04:50, 8 December 2024 (UTC)
- A minuscule contribution: for the natural Gaussian primes and are composite:
- So is the least remaining candidate. --Lambiam 09:00, 8 December 2024 (UTC)
- It is actually easy to see that is composite, since is a perfect square:
- Hence, writing by abuse of notation for we have:
- More in general, any natural number that can be written in the form is not prime in This also rules out the Gaussian primes and --Lambiam 11:50, 8 December 2024 (UTC)
- So which primes are still primes in the ring ? How about and ? 220.132.216.52 (talk) 06:32, 9 December 2024 (UTC)
- As I wrote, this is only a minuscule contribution. We do not do research on command; in fact, we are actually not supposed to do any original research here. --Lambiam 09:23, 9 December 2024 (UTC)
- So which primes are still primes in the ring ? How about and ? 220.132.216.52 (talk) 06:32, 9 December 2024 (UTC)
- Moreover, is also a perfect square. (As in the Gaussian integers, the additive inverse of a square is again a square.) So natural numbers of the form are also composite. This further rules out and A direct proof that, e.g., is composite: There are no remaining candidates below and I can in fact not find any larger ones either. This raises the conjecture:
- Every prime number can be written in one of the three forms and
- Is this a known theorem? If true, no number in is a natural prime. (Note that countless composite numbers cannot be written in any of these forms; to mention just a few: ) --Lambiam 11:46, 9 December 2024 (UTC)
- It is actually easy to see that is composite, since is a perfect square:
- I'll state things a little more generally, in the cyclotomic field . (Your n is twice mine.) A prime q factors as , where each is a prime ideal of the same degree , which is the least positive integer such that . (We have assumed that q does not divide n, because if it did, then it would ramify and not be prime. Also note that we have to use ideals, because the cyclotomic ring is not a UFD.) In particular, stays prime if and only if generates the group of units modulo . When n is a power of two times an odd composite, the group of units is not cyclic, and so the answer is never. When n is a prime or twice a prime, the answer is when q is a primitive root mod n. If n is 4 times a power of two times a prime, the answer is never. Tito Omburo (talk) 11:08, 8 December 2024 (UTC)
- For your , and are the same, as well as and , this is why I use instead of . 61.229.100.34 (talk) 20:58, 8 December 2024 (UTC)
- Also, what is the class number of the cyclotomic field ? Let be the class number of the cyclotomic field , I only know that:
- for (is there any other such )?
- If divides , then also divides , thus we can let
- For prime , divides if and only if is Bernoulli irregular prime
- For prime , divides if and only if is Euler irregular prime
- for (is there any other such )?
- is prime for (are there infinitely many such ?)
- Is there an algorithm to calculate quickly? 61.229.100.34 (talk) 21:14, 8 December 2024 (UTC)
Can we say anything special about every pair of functions f,g, satisfying f(g(x))=f(x) for every x?
[edit]Especially, is there an accepted term for such a pair?
Here are three simple examples, for two functions f,g, satisfying the above, and defined for every natural number:
Example #1:
- f is constant.
Example #2:
- f(x)=g(x), and is the smallest even number, not greater than x.
Example #3:
- f(x)=1 if x is even, otherwise f(x)=2.
- g(x)=x+2.
2A06:C701:746D:AE00:ACFC:490:74C3:660 (talk) 09:31, 8 December 2024 (UTC)
- One way to consider such a pair is dynamically. If you consider the dynamical system , then the condition can be stated as " is constant on -orbits". More precisely, let be the domain of , which is also the codomain of . Define an equivalence relation on by if for some positive integers . Then is simply a function on the set of equivalence classes (=space of orbits). In ergodic theory, such a function is thought of as an "observable" or "function of state", being the mathematical analog of a thermodynamic observable such as temperature. Tito Omburo (talk) 11:52, 8 December 2024 (UTC)
- After you've mentioned temprature, could you explain what are f,g, as far as temprature is concerned? Additionally, could you give another useful example from physics for such a pair of functions? 2A06:C701:746D:AE00:ACFC:490:74C3:660 (talk) 19:49, 8 December 2024 (UTC)
- This equation is just the definition of function g. For instance if function f has the inverse function f−1 then we have g(x)=x. Ruslik_Zero 20:23, 8 December 2024 (UTC)
- If f is the temperature, and g is the evolution of an ensemble of particles in thermal equilibrium (taken at a single time, say one second later), then because temperature is a function of state, one has for all ensembles x. Another example from physics is when is a Hamiltonian evolution. Then the functions with this property (subject to smoothness) are those that (Poisson) commute with the Hamiltonian, i.e. "constants of the motion". Tito Omburo (talk) 20:33, 8 December 2024 (UTC)
- After you've mentioned temprature, could you explain what are f,g, as far as temprature is concerned? Additionally, could you give another useful example from physics for such a pair of functions? 2A06:C701:746D:AE00:ACFC:490:74C3:660 (talk) 19:49, 8 December 2024 (UTC)
- Let be a function from to and a function from to Using the notation for function composition, the property under discussion can concisely be expressed as An equivalent but verbose way of saying the same is that the preimage of any set under is closed under the application of --Lambiam 08:54, 9 December 2024 (UTC)
IEEE Xplore paper claim to acheive exponentiation inversion suitable for pairing in polynomial time. Is it untrustworthy ?
[edit]I just found https://ieeexplore.ieee.org/abstract/document/6530387. Given the multiplicative group factorization in the underlying finite field of a target bn curve, they claim to acheive exponentiation inversion suitable for pairing inversion in seconds on a 32 bits cpu.
On 1 side, the paper is supposed to be peer reviewed by the iee Xplore journal and they give examples on 100 bits. On the other side, in addition to the claim, their algorithm 2 and 3 are very implicit, and as an untrained student, I fail to understand how to implement them, though I fail to understand things like performing a Weil descent.
Is the paper untrustworthy, or would it be possible to get code that can be run ? 2A01:E0A:401:A7C0:152B:F56C:F8A8:D203 (talk) 18:53, 8 December 2024 (UTC)
About the paper, I agree to share the paper privately 2A01:E0A:401:A7C0:152B:F56C:F8A8:D203 (talk) 18:54, 8 December 2024 (UTC)
December 9
[edit]If the Mersenne number 2^p-1 is prime, then must it be the smallest Mersenne prime == 1 mod p?
[edit]If the Mersenne number 2^p-1 is prime, then must it be the smallest Mersenne prime == 1 mod p? (i.e. there is no prime q < p such that 2^q-1 is also a Mersenne prime == 1 mod p) If p is prime (no matter 2^p-1 is prime or not), 2^p-1 is always == 1 mod p. However, there are primes p such that there is a prime q < p such that 2^q-1 is also a Mersenne prime == 1 mod p:
- 2^19-1 is Mersenne prime == 1 mod 73 (p=73, q=19)
- 2^31-1 is Mersenne prime == 1 mod 151 (p=151, q=31)
- 2^61-1 is Mersenne prime == 1 mod 151 (p=151, q=61)
- 2^17-1 is Mersenne prime == 1 mod 257 (p=257, q=17)
- 2^31-1 is Mersenne prime == 1 mod 331 (p=331, q=31)
- 2^61-1 is Mersenne prime == 1 mod 331 (p=331, q=61)
- 2^127-1 is Mersenne prime == 1 mod 337 (p=337, q=127)
- 2^89-1 is Mersenne prime == 1 mod 353 (p=353, q=89)
- 2^89-1 is Mersenne prime == 1 mod 397 (p=397, q=89)
but for these primes p, 2^p-1 is not prime, and my question is: Is there a prime p such that 2^p-1 is a prime and there is a prime q < p such that 2^q-1 is also a Mersenne prime == 1 mod p?
- If 2^11-1 is prime, then this is true, since 2^11-1 is == 1 mod 31 and 2^31-1 is prime, but 2^11-1 is not prime
- If 2^23-1 or 2^67-1 is prime, then this is true, since 2^23-1 and 2^67-1 are == 1 mod 89 and 2^89-1 is prime, but 2^23-1 and 2^67-1 are not primes
- If 2^29-1 or 2^43-1 or 2^71-1 or 2^113-1 is prime, then this is true, since 2^29-1 and 2^43-1 and 2^71-1 and 2^113-1 are == 1 mod 127 and 2^127-1 is prime, but 2^29-1 and 2^43-1 and 2^71-1 and 2^113-1 are not primes
- If 2^191-1 or 2^571-1 or 2^761-1 or 2^1901-1 is prime, then this is true, since 2^191-1 and 2^571-1 and 2^761-1 and 2^1901-1 are == 1 mod 2281 and 2^2281-1 is prime, but 2^191-1 and 2^571-1 and 2^761-1 and 2^1901-1 are not primes
- If 2^1609-1 is prime, then this is true, since 2^1609-1 is == 1 mod 3217 and 2^3217-1 is prime, but 2^1609-1 is not prime
Another question: For any prime p, is there always a Mersenne prime == 1 mod p? 220.132.216.52 (talk) 19:03, 9 December 2024 (UTC)
- Neither question is easy. For the first, relations would imply that the integer 2 is not a primitive root mod p, and that its order divides for the prime q. This is a sufficiently infrequent occurrence that it seems likely that all Mersenne numbers could be ruled out statistically, but not enough is known about their distribution. For the second, it is not even known if there are infinitely many Mersenne primes. Tito Omburo (talk) 19:23, 9 December 2024 (UTC)
- I found that: 2^9689-1 is the smallest Mersenne prime == 1 mod 29, 2^44497-1 is the smallest Mersenne prime == 1 mod 37, 2^756839-1 is the smallest Mersenne prime == 1 mod 47, 2^57885161-1 is the smallest Mersenne prime == 1 mod 59, 2^4423-1 is the smallest Mersenne prime == 1 mod 67, 2^9941-1 is the smallest Mersenne prime == 1 mod 71, 2^3217-1 is the smallest Mersenne prime == 1 mod 97, 2^21701-1 is the smallest Mersenne prime == 1 mod 101, and none of the 52 known Mersenne primes are == 1 mod these primes p < 1024: 79, 83, 103, 173, 193, 197, 199, 227, 239, 277, 307, 313, 317, 349, 359, 367, 373, 383, 389, 409, 419, 431, 443, 461, 463, 467, 479, 487, 503, 509, 523, 547, 563, 587, 599, 613, 647, 653, 659, 661, 677, 709, 727, 733, 739, 743, 751, 757, 769, 773, 797, 809, 821, 823, 827, 829, 839, 853, 857, 859, 863, 887, 907, 911, 919, 929, 937, 941, 947, 971, 977, 983, 991, 1013, 1019, 1021 220.132.216.52 (talk) 20:51, 9 December 2024 (UTC)
- Also,
- 2^19937-1 is Mersenne prime == 1 mod 2^16+1
- 2^521-1 is Mersenne prime == 1 mod 2^13-1
- 2^3021377-1 is Mersenne prime == 1 mod 2^17-1
- 2^2281-1 is Mersenne prime == 1 mod 2^19-1
- 2^21701-1 is Mersenne prime == 1 mod 2^31-1
- 2^19937-1 is Mersenne prime == 1 mod 2^89-1
- 2^86243-1 is Mersenne prime == 1 mod 2^107-1
- but none of these primes p has 2^p-1 is known to be prime, the status of 2^(2^89-1)-1 and 2^(2^107-1)-1 are still unknown (see double Mersenne number), but if at least one of them is prime, then will disprove this conjecture (none of the 52 known Mersenne primes are == 1 mod 2^61-1 or 2^127-1), I think that this conjecture may be as hard as the New Mersenne conjecture. 220.132.216.52 (talk) 20:55, 9 December 2024 (UTC)
- Also, for the primes p < 10000, there is a prime q < p such that 2^q-1 is also a Mersenne prime == 1 mod p only for p = 73, 151, 257, 331, 337, 353, 397, 683, 1321, 1613, 2113, 2731, 4289, 4561, 5113, 5419, 6361, 8191, 9649 (this sequence is not in OEIS), however, none of these primes p have 2^p-1 prime. 220.132.216.52 (talk) 02:23, 10 December 2024 (UTC)
December 10
[edit]More on the above conjecture
[edit]Above I posed:
- Conjecture. Every prime number can be written in one of the three forms and
If true, it implies no natural prime is a prime in the ring .
The absolute-value bars are not necessary. A number that can be written in the form is also expressible in the form
It turns out (experimentally; no proof) that a number that can be written in two of these forms can also be written in the third form. The conjecture is not strongly related to the concept of primality, as can be seen in this reformulation:
- Conjecture. A natural number that cannot be written in any one of the three forms and is composite.
The first few numbers that cannot be written in any one of these three forms are
They are indeed all composite, but why this should be so is a mystery to me. What do and which appear later in the list, have in common? I see no pattern.
It seems furthermore that the primorials, starting with make the list. (Checked up to ) --Lambiam 19:23, 10 December 2024 (UTC)
- Quick note, for those like me who are curious how numbers of the form can be written into a form of , note that , and so . GalacticShoe (talk) 02:20, 11 December 2024 (UTC)
- A prime is expressible as the sum of two squares if and only if it is congruent to , as per Fermat's theorem on sums of two squares. A prime is expressible of the form if and only if it is congruent to , as per OEIS:A002479. And a prime is expressible of the form if and only if it is congruent to , as per OEIS:A035251. Between these congruences, all primes are covered. GalacticShoe (talk) 05:59, 11 December 2024 (UTC)
- More generally, a number is not expressible as:
- if it has a prime factor congruent to that is raised to an odd power (equivalently, .)
- if it has a prime factor congruent to that is raised to an odd power
- if it has a prime factor congruent to that is raised to an odd power
- It is easy to see why expressibility as any two of these forms leads to the third form holding, and also we can see why it's difficult to see a pattern in numbers that are expressible in none of these forms, in particular we get somewhat-convoluted requirements on exponents of primes in the factorization satisfying congruences modulo 8. GalacticShoe (talk) 06:17, 11 December 2024 (UTC)
- Thanks. Is any of this covered in some Wikipedia article? --Lambiam 10:06, 11 December 2024 (UTC)
- More generally, a number is not expressible as:
Assume p is 3 mod 4. Suppose that (2|p)=1. Then where . Because the cyclotomic ideal has norm and is stable under the Galois action it is generated by a single element , of norm .
If (2|p)=-1, then the relevant ideal is stable under and so is generated by , of norm . Tito Omburo (talk) 14:43, 11 December 2024 (UTC)
December 11
[edit]Unique normal ultrafilter
[edit]So I'm supposed to know the answer to this, I suppose, but I don't seem to :-)
"Everyone knows" that, in , Gödel's constructible universe relative to an ultrafilter on some measurable cardinal , there is only a single normal ultrafilter, namely itself. See for example John R. Steel's monograph here, at Theorem 1.7.
So I guess that must mean that the product measure , meaning you fix some identification between and and then say a set has measure 1 if measure 1 many of its vertical sections have measure 1, must not be normal. (Unless it's somehow just equal to but I don't think it is.)
But is there some direct way to see that? Say, a continuous function with such that the set of fixed points of is not in the ultrafilter no singleton has a preimage under that's in the ultrafilter? I haven't been able to come up with it. --Trovatore (talk) 06:01, 11 December 2024 (UTC)