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{{WikiProject Elements
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{{WikiProject Elements|isotope=yes|importance=Low|isotopes=yes}}
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==Low Half-life values of OO63Eu144 and OO63Eu140==
|importance=Low
|isotopes=yes}}
This article is part of [[Wikipedia:Wikiproject Isotopes]]. Please keep style and phrasings consistent across the set of pages. For later reference and improved reliability, data from all considered multiple sources is collected here. References are denoted by these letters:
*('''A''') G. Audi, O. Bersillon, J. Blachot, A.H. Wapstra. [http://amdc.in2p3.fr/web/nubase_en.html The Nubase2003 evaluation of nuclear and decay properties], Nuc. Phys. A 729, pp. 3-128 (2003). — Where this source indicates a speculative value, the # mark is also applied to values with weak assignment arguments from other sources, if grouped together. An asterisk after the A means that a comment of some importance may be available in the original.
*('''B''') National Nuclear Data Center, Brookhaven National Laboratory, information extracted from the [http://www.nndc.bnl.gov/nudat2/ NuDat 2.1 database]. (Retrieved Sept. 2005, from the code of the popup boxes).
*('''C''') David R. Lide (ed.), Norman E. Holden in ''CRC Handbook of Chemistry and Physics, 85th Edition'', online version. CRC Press. Boca Raton, Florida (2005). Section 11, Table of the Isotopes. — The CRC uses rounded numbers with implied uncertainties, where this concurs with the range of another source it is treated as exactly equal in this comparison.
*('''D''') More specific level data from reference B's ''Levels and Gammas database''.
*('''E''') Same as B but excitation energy replaced with that from D.


The reported half-lives do not agree with the half-life trend line of the rest of the 63Eu Europium OO type isotopes.[[User:WFPM|WFPM]] ([[User talk:WFPM|talk]]) 23:42, 21 April 2013 (UTC)
Z N refs symbol half-life spin excitation energy
63 67 A |Eu-130 |1.1(5) ms |2+#
63 67 B |Eu-130 |0.9(+5-3) ms |(1+)
63 67 C |Eu-130 |0.9 ms |
63 68 AB |Eu-131 |17.8(19) ms |3/2+
63 68 C |Eu-131 |~26. ms |
63 69 A |Eu-132 |100# ms |
63 69 B |Eu-132 |200# ms |
63 70 A |Eu-133 |200# ms |11/2-#
63 70 B |Eu-133 |~1 s |
63 71 ABC |Eu-134 |0.5(2) s |
63 72 A |Eu-135 |1.5(2) s |11/2-#
63 72 BC |Eu-135 |1.5(2) s |
63 73 AB |Eu-136 |3.3(3) s |(7+)
63 73 C |Eu-136 |~3.9 s |1+
63 73 A |Eu-136m |3.8(3) s |(3+) |0(500)# keV
63 73 E |Eu-136m |3.8(3) s |(3+) |Y keV
63 73 D |Eu-136m |3.3(3) s |(7+) |X keV
63 73 C |Eu-136m |~3.2 s |7+
63 74 A |Eu-137 |8.4(5) s |11/2-#
63 74 B |Eu-137 |11(2) s |(11/2-)
63 74 C |Eu-137 |11. s |11/2-
63 75 AB |Eu-138 |12.1(6) s |(6-)
63 75 C |Eu-138 |12. s |7+
63 76 AB |Eu-139 |17.9(6) s |(11/2)-
63 76 C |Eu-139 |18. s |
63 77 AB |Eu-140 |1.51(2) s |1+
63 77 C |Eu-140 |1.51 s |1-
63 77 A |Eu-140m |125(2) ms |5-# |210(15) keV
63 77 E |Eu-140m |125(2) ms |(5-) |185.3+X keV
63 77 C |Eu-140m |0.125 s |
63 78 AB |Eu-141 |40.7(7) s |5/2+
63 78 C |Eu-141 |40. s |5/2+
63 78 AE |Eu-141m |2.7(3) s |11/2- |96.45(7) keV
63 78 C |Eu-141m |3.0 s |11/2-
63 79 AC |Eu-142 |2.36(10) s |1+
63 79 B |Eu-142 |2.34(12) s |1+
63 79 A |Eu-142m |1.223(8) min |8- |460(30) keV
63 79 E |Eu-142m |1.223(8) min |8- |0+X keV
63 79 C |Eu-142m |1.22 min |8-
63 80 AB |Eu-143 |2.59(2) min |5/2+
63 80 C |Eu-143 |2.62 min |5/2+
63 80 AD |Eu-143m |50.0(5) µs |11/2- |389.51(4) keV
63 81 ABC |Eu-144 |10.2(1) s |1+
63 81 AD |Eu-144m |1.0(1) µs |(8-) |1127.6(6) keV
63 82 ABC |Eu-145 |5.93(4) d |5/2+
63 82 A |Eu-145m |490 ns |11/2- |716.0(3) keV
63 82 D |Eu-145m |490(30) ns |11/2- |716.0(3) keV
63 83 AB |Eu-146 |4.61(3) d |4-
63 83 C |Eu-146 |4.57 d |4-
63 83 AD |Eu-146m |235(3) µs |9+ |666.37(16) keV
63 84 AB |Eu-147 |24.1(6) d |5/2+
63 84 C |Eu-147 |24.4 d |5/2+
63 85 ABC |Eu-148 |54.5(5) d |5-
63 86 ABC |Eu-149 |93.1(4) d |5/2+
63 87 AB |Eu-150 |36.9(9) a |5(-)
63 87 C |Eu-150 |36. a |5-
63 87 A |Eu-150m |12.8(1) h |0- |42.1(5) keV
63 87 E |Eu-150m |12.8(1) h |0- |42.1 keV
63 87 C |Eu-150m |12.8 h |0-
63 88 ABC |Eu-151 |5×1018 a |5/2+
63 88 AD |Eu-151m |58.9(5) µs |11/2- |196.245(10) keV
63 89 A |Eu-152 |13.537(6) a |3-
63 89 BC |Eu-152 |13.506(6) a |3-
63 89 AE |Eu-152m1|9.3116(13) h |0- |45.5998(4) keV
63 89 C |Eu-152m1|9.30 h |0-
63 89 D |Eu-152m2|0.94(8) µs |1- |65.2969(4) keV
63 89 D |Eu-152m3|165(10) ns |1+ |78.2331(4) keV
63 89 D |Eu-152m4|384(10) ns |4+ |89.8496(4) keV
63 89 AE |Eu-152m5|96(1) min |8- |147.86(10) keV
63 89 C |Eu-152m5|1.60 h |8-
63 90 ABC |Eu-153 |STABLE |5/2+
63 91 A |Eu-154 |8.593(4) a |3-
63 91 BC |Eu-154 |8.590(3) a |3-
63 91 AE |Eu-154m1|46.3(4) min |(8-) |145.3(3) keV
63 91 C |Eu-154m1|46.1 min |8-
63 91 D |Eu-154m2|2.2(1) µs |2+ |68.1702(4) keV
63 92 AC |Eu-155 |4.7611(13) a |5/2+
63 92 B |Eu-155 |4.753(14) a |5/2+
63 93 AB |Eu-156 |15.19(8) d |0+
63 93 C |Eu-156 |15.2 d |1+
63 94 AB |Eu-157 |15.18(3) h |5/2+
63 94 C |Eu-157 |15.13 h |(5/2+)
63 95 ABC |Eu-158 |45.9(2) min |(1-)
63 96 AB |Eu-159 |18.1(1) min |5/2+
63 96 C |Eu-159 |18.1 min |(5/2+)
63 97 A |Eu-160 |38(4) s |1(-)
63 97 B |Eu-160 |38(4) s |1
63 97 C |Eu-160 |38. s |(0-)
63 98 A |Eu-161 |26(3) s |5/2+#
63 98 B |Eu-161 |26(3) s |
63 98 C |Eu-161 |27. s |
63 99 ABC |Eu-162 |10.6(10) s |
63 100 A |Eu-163 |6# s |5/2+#
63 100 B |Eu-163 |6# s |
63 101 A |Eu-164 |2# s |
63 101 B |Eu-164 |~2 s |
63 102 A |Eu-165 |1# s |5/2+#
63 102 B |Eu-165 |~1 s |
63 103 A |Eu-166 |400# ms |
63 103 B |Eu-166 |~0.4 s |
63 104 A |Eu-167 |200# ms |5/2+#
63 104 B |Eu-167 |~0.2 |s


== How would {{chem|153|Eu}} decay to a much less stable isotope, {{chem|149|Pm}}? ==
[[User:Femto|Femto]] 12:35, 15 November 2005 (UTC)


Because {{chem|149|Pm}} is way too unstable, so shouldn't {{chem|153|Eu}} be stable too? [[Special:Contributions/80.98.179.160|80.98.179.160]] ([[User talk:80.98.179.160|talk]]) 07:06, 26 March 2018 (UTC)
===Talk===
:This is pretty normal: the obvious example is that <sup>238</sup>U (half-life 4.468 × 10<sup>9</sup> years) decays to <sup>234</sup>Th (half-life 24.1 days). The important thing is that the system of <sup>149</sup>Pm plus an alpha particle is a lower-energy arrangement of 63 protons and 90 neutrons than a single <sup>153</sup>Eu nucleus (just look at the binding energies), and so the decay is energetically allowed. Of course, it is kinetically hindered for other reasons. The beta-instability of <sup>149</sup>Pm has nothing to do with it. [[User:Double sharp|Double sharp]] ([[User talk:Double sharp|talk]]) 07:15, 26 March 2018 (UTC)
----
::It may be worthy noting that <sup>149</sup>Pm also has a greater alpha decay energy (1.135 MeV) than <sup>153</sup>Eu (0.273 MeV). Roughly speaking, <sup>149</sup>Pm has 3 more protons than the alpha-stable nuclide <sup>146</sup>Ce, while <sup>153</sup>Eu has only 2 more protons than the alpha-stable <sup>151</sup>Pm.
::In the example of <sup>238</sup>U-<sup>234</sup>Th this is not the case (4.270 MeV for <sup>238</sup>U vs. 3.672 MeV for <sup>234</sup>Th). Of course lower alpha decay energy does not necessarily mean longer alpha decay partial half-life: <sup>231</sup>Th has an alpha decay energy of 4.213 MeV and partial half-life 2.91×10<sup>7</sup> years, compared to 4.678 MeV and 7.04×10<sup>8</sup> years for <sup>235</sup>U. [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 00:55, 24 November 2023 (UTC)
Because <sup>153</sup>Eu have a larger mass than a combination of <sup>149</sup>Pm and <sup>4</sup>He (atomic mass of <sup>153</sup>Eu is 152.9212303, atomic mass of <sup>149</sup>Pm is 148.918334, atomis of <sup>4</sup>He is 4.002602) but the kenetic energy of alpha particle in this case is quite small meaning the half-life is quite large[[User:Cristiano Toàn|Cristiano Toàn]] ([[User talk:Cristiano Toàn|talk]]) 08:54, 16 May 2022 (UTC)


:At the order of 10<sup>140</sup> years as stated in [https://arxiv.org/pdf/1908.11458.pdf]. [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 06:25, 28 October 2023 (UTC)
== What theory? ==
Theoretical decay chain of <sup>153</sup>Eu:<sup>153</sup>Eu => <sup>149</sup>Pm => <sup>149</sup>Sm => <sup>145</sup>Nd => <sup>141</sup>Ce => <sup>141</sup>Pm (the last nuclide contains 82 neutrons, magic number). Both <sup>149</sup>Sm and <sup>145</sup>Nd has theoretical half-life shorter than <sup>128</sup>Te's half-life
It was: "<sup>151</sup>Eu was recently found to be unstable to [[alpha decay]] with [[half-life]] of <math>5_{-3}^{+11}\times 10^{18}</math> yr, '''in reasonable agreement with theoretical predictions.'''"
I have taken the latter part out, because it doesn't say what theory is meant. <small>—Preceding [[Wikipedia:Signatures|unsigned]] comment added by [[User:Phr en|Phr en]] ([[User talk:Phr en|talk]] • [[Special:Contributions/Phr en|contribs]]) 09:02, 29 February 2008 (UTC)</small><!-- Template:Unsigned --> <!--Autosigned by SineBot-->


:No, the main decay mode of <sup>153</sup>Eu would be <sup>12</sup>C or <sup>14</sup>C cluster decay; see [https://en.wikipedia.org/wiki/Talk:Cluster_decay#Theoretical_calculation_of_cluster_decays_for_mass_numbers_152-165,_201-205 here]. So the theoretical decay chain would be <sup>153</sup>Eu → <sup>139</sup>La → <sup>107</sup>Tc → ... → <sup>107</sup>Ag → <sup>91</sup>Y → <sup>91</sup>Zr (stable) or <sup>153</sup>Eu → <sup>141</sup>La → <sup>141</sup>Ce → <sup>141</sup>Pr → <sup>125</sup>Sb → <sup>125</sup>Te → <sup>93</sup>Sr → ... → <sup>93</sup>Nb → <sup>57</sup>Mn → <sup>57</sup>Fe (stable). The decay modes for beta-stable nuclides in these two chains are all cluster decays. [[Special:Contributions/14.52.231.91|14.52.231.91]] ([[User talk:14.52.231.91|talk]]) 04:02, 29 August 2024 (UTC)
==Low Half-life values of OO63Eu144 and OO63Eu140==


== Could <sup>150</sup>Eu possibly undergo β- decay to <sup>150</sup>Gd? ==
The reported half-lives do not agree with the half-life trend line of the rest of the 63Eu Europium OO type isotopes.[[User:WFPM|WFPM]] ([[User talk:WFPM|talk]]) 23:42, 21 April 2013 (UTC)


This is energetically allowed, and also we observe a 89% probability of the β- decay of <sup>150m</sup>Eu. However, just like to case of <sup>98</sup>Tc whose decay to <sup>98</sup>Mo is unknown, do we know that it is impossible, or it's just we haven't observed that mode of decay? [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 00:26, 11 October 2023 (UTC)
== How would {{chem|153|Eu}} decay to a much less stable isotope, {{chem|149|Pm}}? ==
[[User:Cristiano Toàn|Cristiano Toàn]] ([[User talk:Cristiano Toàn|talk]]) 14:37, 11 February 2024 (UTC). [[User:Cristiano Toàn|Cristiano Toàn]] ([[User talk:Cristiano Toàn|talk]]) 14:37, 11 February 2024 (UTC)Theoretical decay chain of <sup>153</sup>Eu:<sup>153</sup>Eu => <sup>149</sup>Pm => <sup>149</sup>Sm => <sup>145</sup>Nd => <sup>141</sup>Ce => <sup>141</sup>Pm (the last nuclide contains 82 neutrons, magic number). Both <sup>149</sup>Sm and <sup>145</sup>Nd has theoretical half-life shorter than <sup>128</sup>Te's half-life


Because {{chem|149|Pm}} is way too unstable, so shouldn't {{chem|153|Eu}} be stable too? [[Special:Contributions/80.98.179.160|80.98.179.160]] ([[User talk:80.98.179.160|talk]]) 07:06, 26 March 2018 (UTC)
:The 3<sup>-</sup> state of <sup>150</sup>Gd is as high as [https://www.nndc.bnl.gov/nudat3/getdataset.jsp?nucleus=150Gd&unc=NDS 1134.297 keV], and the 4<sup>+</sup> state 1288.42 keV, while the theoretical decay energy of <sup>150</sup>Eu (5<sup>-</sup> state) to <sup>150</sup>Gd is only 972 keV. [[Special:Contributions/14.52.231.91|14.52.231.91]] ([[User talk:14.52.231.91|talk]]) 04:14, 29 August 2024 (UTC)

== Possible alpha decay of <sup>144,145,146,149</sup>Eu ==

According to [https://iopscience.iop.org/article/10.1088/1402-4896/ac1a4d], <sup>146</sup>Eu (''N'' = 83) and <sup>149</sup>Eu (''N'' = 86) should respectively have a partial alpha decay half-life of at least 10<sup>22</sup> years and 10<sup>9</sup> years. <sup>149</sup>Eu has similar alpha decay energy as its decay product (2.40 MeV for <sup>149</sup>Eu and 2.32 MeV for <sup>145</sup>Pm), and <sup>146</sup>Eu has lower decay energy than '''''<sup>151</sup>Eu''''' (1.60 MeV vs. 1.96 MeV).

As for <sup>144</sup>Eu (''N'' = 81) and <sup>145</sup>Eu (''N'' = 82), they have respectively an alpha decay energy of 0.16 MeV and 0.10 MeV, which are much too low, so their partial alpha decay half-lives should be long beyond imagination. [[Special:Contributions/129.104.241.214|129.104.241.214]] ([[User talk:129.104.241.214|talk]]) 06:14, 24 October 2023 (UTC)

== disagreement between beginning and table ==

Beginning of the article states that <sup>152m2</sup>Eu has a half-life of 96 min, but the table states that it's false and that it's actually <sup>152m5</sup>Eu with a half-life of 96 min. [[Special:Contributions/24.115.255.37|24.115.255.37]] ([[User talk:24.115.255.37|talk]]) 20:49, 19 May 2024 (UTC)

:Fixed, as given in {{tl|NUBASE2020}}; thanks for catching this. <sup>[[User:ComplexRational|'''<span style="color:#0039a6">Complex</span>''']]</sup>/<sub>[[User talk:ComplexRational|'''<span style="color:#000000">Rational</span>''']]</sub> 21:02, 19 May 2024 (UTC)
::you're welcome. [[Special:Contributions/24.115.255.37|24.115.255.37]] ([[User talk:24.115.255.37|talk]]) 22:25, 19 May 2024 (UTC)

Latest revision as of 09:39, 7 September 2024

Low Half-life values of OO63Eu144 and OO63Eu140

[edit]

The reported half-lives do not agree with the half-life trend line of the rest of the 63Eu Europium OO type isotopes.WFPM (talk) 23:42, 21 April 2013 (UTC)[reply]

How would 153
Eu
decay to a much less stable isotope, 149
Pm
?

[edit]

Because 149
Pm
is way too unstable, so shouldn't 153
Eu
be stable too? 80.98.179.160 (talk) 07:06, 26 March 2018 (UTC)[reply]

This is pretty normal: the obvious example is that 238U (half-life 4.468 × 109 years) decays to 234Th (half-life 24.1 days). The important thing is that the system of 149Pm plus an alpha particle is a lower-energy arrangement of 63 protons and 90 neutrons than a single 153Eu nucleus (just look at the binding energies), and so the decay is energetically allowed. Of course, it is kinetically hindered for other reasons. The beta-instability of 149Pm has nothing to do with it. Double sharp (talk) 07:15, 26 March 2018 (UTC)[reply]
It may be worthy noting that 149Pm also has a greater alpha decay energy (1.135 MeV) than 153Eu (0.273 MeV). Roughly speaking, 149Pm has 3 more protons than the alpha-stable nuclide 146Ce, while 153Eu has only 2 more protons than the alpha-stable 151Pm.
In the example of 238U-234Th this is not the case (4.270 MeV for 238U vs. 3.672 MeV for 234Th). Of course lower alpha decay energy does not necessarily mean longer alpha decay partial half-life: 231Th has an alpha decay energy of 4.213 MeV and partial half-life 2.91×107 years, compared to 4.678 MeV and 7.04×108 years for 235U. 129.104.241.214 (talk) 00:55, 24 November 2023 (UTC)[reply]

Because 153Eu have a larger mass than a combination of 149Pm and 4He (atomic mass of 153Eu is 152.9212303, atomic mass of 149Pm is 148.918334, atomis of 4He is 4.002602) but the kenetic energy of alpha particle in this case is quite small meaning the half-life is quite largeCristiano Toàn (talk) 08:54, 16 May 2022 (UTC)[reply]

At the order of 10140 years as stated in [1]. 129.104.241.214 (talk) 06:25, 28 October 2023 (UTC)[reply]

Theoretical decay chain of 153Eu:153Eu => 149Pm => 149Sm => 145Nd => 141Ce => 141Pm (the last nuclide contains 82 neutrons, magic number). Both 149Sm and 145Nd has theoretical half-life shorter than 128Te's half-life

No, the main decay mode of 153Eu would be 12C or 14C cluster decay; see here. So the theoretical decay chain would be 153Eu → 139La → 107Tc → ... → 107Ag → 91Y → 91Zr (stable) or 153Eu → 141La → 141Ce → 141Pr → 125Sb → 125Te → 93Sr → ... → 93Nb → 57Mn → 57Fe (stable). The decay modes for beta-stable nuclides in these two chains are all cluster decays. 14.52.231.91 (talk) 04:02, 29 August 2024 (UTC)[reply]

Could 150Eu possibly undergo β- decay to 150Gd?

[edit]

This is energetically allowed, and also we observe a 89% probability of the β- decay of 150mEu. However, just like to case of 98Tc whose decay to 98Mo is unknown, do we know that it is impossible, or it's just we haven't observed that mode of decay? 129.104.241.214 (talk) 00:26, 11 October 2023 (UTC) Cristiano Toàn (talk) 14:37, 11 February 2024 (UTC). Cristiano Toàn (talk) 14:37, 11 February 2024 (UTC)Theoretical decay chain of 153Eu:153Eu => 149Pm => 149Sm => 145Nd => 141Ce => 141Pm (the last nuclide contains 82 neutrons, magic number). Both 149Sm and 145Nd has theoretical half-life shorter than 128Te's half-life[reply]

The 3- state of 150Gd is as high as 1134.297 keV, and the 4+ state 1288.42 keV, while the theoretical decay energy of 150Eu (5- state) to 150Gd is only 972 keV. 14.52.231.91 (talk) 04:14, 29 August 2024 (UTC)[reply]

Possible alpha decay of 144,145,146,149Eu

[edit]

According to [2], 146Eu (N = 83) and 149Eu (N = 86) should respectively have a partial alpha decay half-life of at least 1022 years and 109 years. 149Eu has similar alpha decay energy as its decay product (2.40 MeV for 149Eu and 2.32 MeV for 145Pm), and 146Eu has lower decay energy than 151Eu (1.60 MeV vs. 1.96 MeV).

As for 144Eu (N = 81) and 145Eu (N = 82), they have respectively an alpha decay energy of 0.16 MeV and 0.10 MeV, which are much too low, so their partial alpha decay half-lives should be long beyond imagination. 129.104.241.214 (talk) 06:14, 24 October 2023 (UTC)[reply]

disagreement between beginning and table

[edit]

Beginning of the article states that 152m2Eu has a half-life of 96 min, but the table states that it's false and that it's actually 152m5Eu with a half-life of 96 min. 24.115.255.37 (talk) 20:49, 19 May 2024 (UTC)[reply]

Fixed, as given in {{NUBASE2020}}; thanks for catching this. Complex/Rational 21:02, 19 May 2024 (UTC)[reply]
you're welcome. 24.115.255.37 (talk) 22:25, 19 May 2024 (UTC)[reply]