Jump to content

Seesaw mechanism: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
bypassing redirect
Zapientus (talk | contribs)
mNo edit summary
 
(39 intermediate revisions by 27 users not shown)
Line 1: Line 1:
In the [[Grand Unified Theory|theory of grand unification]] of [[particle physics]], and, in particular, in theories of [[neutrino]] masses and [[neutrino oscillation]], the '''seesaw mechanism''' is a generic model used to understand the relative sizes of observed neutrino masses, of the order of [[electronvolt|eV]], compared to those of [[quark]]s and charged [[lepton]]s, which are millions of times heavier.
In the [[Grand Unified Theory|theory of grand unification]] of [[particle physics]], and, in particular, in theories of [[neutrino]] masses and [[neutrino oscillation]], the '''seesaw mechanism''' is a generic model used to understand the relative sizes of observed neutrino masses, of the order of [[electronvolt|eV]], compared to those of [[quark]]s and charged [[lepton]]s, which are millions of times heavier. The name of the seesaw mechanism was given by [[Tsutomu Yanagida]] in a Tokyo conference in 1981.


There are several types of models, each extending the [[Standard Model]]. The simplest version, type 1, extends the Standard Model by assuming two or more additional right-handed neutrino fields
There are several types of models, each extending the [[Standard Model]]. The simplest version, "Type 1", extends the Standard Model by assuming two or more additional right-handed neutrino fields
inert under the electroweak interaction,{{efn|
inert under the electroweak interactions,<ref>It is possible to generate two light but massive neutrinos with only one right-handed neutrino, but the resulting spectra are generally not viable.</ref> and the existence of a very large mass scale. This allows the mass scale to be identifiable with the postulated scale of grand unification.
It is possible to generate two low-mass neutrinos with only one right-handed neutrino, but the resulting mass spectra are generally not viable.
}}
and the existence of a very large mass scale. This allows the mass scale to be identifiable with the postulated scale of grand unification.


== Type 1 seesaw ==
== Type 1 seesaw ==
This model produces a light neutrino, for each of the three known neutrino flavors, and a corresponding very heavy [[neutrino]] for each flavor, which has yet to be observed.
This model produces a light neutrino, for each of the three known neutrino flavors, and a corresponding very heavy [[neutrino]] for each flavor, which has yet to be observed.


The simple mathematical principle behind the seesaw mechanism is the following property of any 2×2 [[Matrix (mathematics)|matrix]]
The simple mathematical principle behind the seesaw mechanism is the following property of any 2×2 [[Matrix (mathematics)|matrix]] of the form
:<math>A = \begin{pmatrix}0&M\\M&B\end{pmatrix} \text{,}</math>
: <math> A = \begin{pmatrix} 0 & M \\
M & B \end{pmatrix} .</math>
where ''B'' is taken to be much larger than ''M''.
It has two [[eigenvalue]]s:
: <math>\lambda_{(+)} = \frac{B + \sqrt{ B^2 + 4 M^2 }}{2} ,</math>
and
: <math>\lambda_{(-)} = \frac{B - \sqrt{ B^2 + 4 M^2 } }{2} .</math>
The [[geometric mean]] of <math>\lambda_{(+)}</math> and <math>\lambda_{(-)} </math> equals <math>\left| M \right|</math>, since the [[determinant]] <math> \lambda_{(+)} \; \lambda_{(-)} = -M^2 </math>.


Thus, if one of the eigenvalues goes up, the other goes down, and vice versa. This is the point of the name "[[seesaw]]" of the mechanism.
It has two very disproportionate [[eigenvalue]]s:
:<math>\lambda_\pm = \frac{B\pm \sqrt{B^2+4M^2}}{2} \text{.}</math>
The larger eigenvalue, ''λ''<sub>+</sub>, is approximately equal to {{mvar|B}}, while the smaller eigenvalue is approximately equal to
:<math>\lambda_- \approx -\frac{M^2}B.</math>
Thus, |''M'' | is the [[geometric mean]] of ''λ''<sub>+</sub> and {{math| −''λ''<sub>−</sub>}}, since the [[determinant]] equals {{nowrap|''λ''<sub>+</sub>''λ''<sub>−</sub> {{=}} −''M'' <sup>2</sup>}}.


In applying this model to neutrinos, <math> B </math> is taken to be much larger than <math> M .</math>
''If one of the eigenvalues goes up, the other goes down, and vice versa.'' This is the point of the name "[[seesaw]]" of the mechanism.
Then the larger eigenvalue, <math>\lambda_{(+)},</math> is approximately equal to <math> B ,</math> while the smaller eigenvalue is approximately equal to
: <math> \lambda_- \approx -\frac{M^2}{B} .</math>


This mechanism serves to explain why the [[neutrino]] masses are so small.<ref name=Minkowski-1977-1biln-μ/><ref>[[Tsutomu Yanagida|Yanagida, T.]] (1979). "Horizontal gauge symmetry and masses of neutrinos", Proceedings: Workshop on the Unified Theories and the Baryon Number in the Universe: published in KEK Japan, February 13-14, 1979, Conf. Proc. C7902131, p.95- 99.</ref><ref>{{Cite journal |last=Yanagida |first=Tsutomu |date=1979-12-01 |title=Horizontal symmetry and mass of the $t$ quark |url=https://link.aps.org/doi/10.1103/PhysRevD.20.2986 |journal=Physical Review D |volume=20 |issue=11 |pages=2986–2988 |doi=10.1103/PhysRevD.20.2986|bibcode=1979PhRvD..20.2986Y }}</ref><ref name=GellMann-1979/><ref name=Yanagida-1980-HorizSym/><ref name=Glashow-1979-NATO/><ref name=Mohapatra-Senjanovic-1980/><ref name=Schechter-Valle-1980/>
This mechanism serves to explain why the [[neutrino]] masses are so small.<ref name="Minkowski1977">{{cite journal|author=P. Minkowski|authorlink=Peter Minkowski|doi=10.1016/0370-2693(77)90435-X|title=μ --> e γ at a Rate of One Out of 1-Billion Muon Decays?|bibcode = 1977PhLB...67..421M|year=1977|journal=Physics Letters B|volume=67|issue=4|pages=421 }}</ref><ref name="Gell-Mann1979">[[Murray Gell-Mann|M. Gell-Mann]], [[Pierre Ramond|P. Ramond]] and [[Richard Slansky|R. Slansky]], in ''Supergravity'', ed. by D. Freedman and P. Van Nieuwenhuizen, North Holland, Amsterdam (1979), pp. 315-321. ISBN 044485438X</ref><ref name="Yanagida1980" >{{cite journal|journal=Progress of Theoretical Physics|volume=64|issue=3|pages=1103–1105|year=1980|author=T. Yanagida|doi=10.1143/PTP.64.1103|title=Horizontal Symmetry and Masses of Neutrinos}}</ref><ref name="MohapatraSenjanovic1980" >{{cite journal|journal=Phys. Rev. Lett.|volume=44|issue=14|pages=912–915|year=1980|author=[[Rabindra Mohapatra|R. N. Mohapatra]], G. Senjanovic|doi=10.1103/PhysRevLett.44.912|title=Neutrino Mass and Spontaneous Parity Nonconservation|bibcode = 1980PhRvL..44..912M }}</ref><ref name="SchechterValle1980" >{{cite journal|journal=Phys. Rev.|volume=22|issue=9|pages=2227–2235|year=1980|author=J. Schechter, [[José W. F. Valle]] |doi=10.1103/PhysRevD.22.2227|title=Neutrino masses in SU(2) ⊗ U(1) theories|bibcode = 1980PhRvD..22.2227S|last2=Valle|first2=J. }}</ref> The matrix ''A'' is essentially the [[mass matrix]] for the neutrinos. The [[Majorana spinor|Majorana]] mass component ''B'' is comparable to the [[GUT scale]] and violates lepton number; while the components [[Dirac spinor|Dirac]] mass ''M'', are of order of the much smaller [[electroweak scale]], the ''VEV'' below. The smaller eigenvalue λ<sub>−</sub> then leads to a very small neutrino mass comparable to {{val|1|ul=eV}}, which is in qualitative accord with experiments, sometimes regarded as supportive evidence for the framework of Grand Unified Theories.
The matrix {{mvar|A}} is essentially the [[mass matrix]] for the neutrinos. The [[Majorana spinor|Majorana]] mass component <math> B </math> is comparable to the [[GUT scale]] and violates lepton number conservation; while the [[Dirac spinor|Dirac]] mass components <math> M </math> are of order of the much smaller [[electroweak scale]], called the VEV or ''vacuum expectation value'' below. The smaller eigenvalue <math> \lambda_{(-)} </math> then leads to a very small neutrino mass, comparable to {{val|1|ul=eV}}, which is in qualitative accord with experiments—sometimes regarded as supportive evidence for the framework of Grand Unified Theories.


== Background ==
== Background ==
The 2×2 matrix ''A'' arises in a natural manner within the [[standard model]] by considering the most general mass matrix allowed by [[Gauge theory|gauge invariance]] of the standard model [[Action (physics)|action]], and the corresponding charges of the lepton- and neutrino fields.
The 2×2 matrix {{mvar|A}} arises in a natural manner within the [[standard model]] by considering the most general mass matrix allowed by [[Gauge theory|gauge invariance]] of the standard model [[Action (physics)|action]], and the corresponding charges of the lepton- and neutrino fields.


Let the [[Weyl spinor]] ''χ'' be the [[neutrino]] part of a [[Chirality (physics)|left-handed]] [[lepton]] [[Weak isospin|isospin]] [[Doublet state|doublet]] (the other part being the left-handed charged lepton),
Call the [[neutrino]] part of a [[Weyl spinor]] <math> \chi ,</math> a part of a [[Chirality (physics)|left-handed]] [[lepton]] [[weak isospin]] [[Doublet state|doublet]]; the other part is the left-handed charged lepton <math>\ell,</math>
:<math> L=\begin{pmatrix}\chi \\ \eta \end{pmatrix} ~,</math>
:<math> L = \begin{pmatrix} \chi \\ \ell \end{pmatrix} ,</math>
as it is present in the minimal [[standard model]] without neutrino masses, and let ''η'' be a postulated right-handed neutrino Weyl spinor which is a [[Singlet state|singlet]] under [[weak isospin]] (i.e. does not interact weakly, such as a [[sterile neutrino]]).
as it is present in the minimal [[standard model]] with neutrino masses omitted, and let <math>\eta</math> be a postulated right-handed neutrino Weyl spinor which is a [[Singlet state|singlet]] under [[weak isospin]] i.e. a neutrino that fails to interact weakly, such as a [[sterile neutrino]].


There are now three ways to form [[Lorentz covariance|Lorentz covariant]] mass terms, giving either
There are now three ways to form [[Lorentz covariance|Lorentz covariant]] mass terms, giving either
:<math>\frac{1}{2}\, B'\,\chi^\alpha \chi_\alpha \, \text{,}\quad \frac{1}{2}\,B\,\eta^\alpha\eta_\alpha \,\text{,}\quad\text{or} \quad M\,\eta^\alpha \chi_\alpha \,\text{,}</math>
: <math> \tfrac{1}{2} \, B' \, \chi^\alpha \chi_\alpha \, , \quad \frac{1}{2} \, B\, \eta^\alpha \eta_\alpha \, , \quad \mathrm{ or } \quad M \, \eta^\alpha \chi_\alpha \, ,</math>
and their [[complex conjugate]]s, which can be written as a [[quadratic form]],
and their [[complex conjugate]]s, which can be written as a [[quadratic form]],
: <math>
:<math>\frac{1}{2}\,\begin{pmatrix}\chi& \eta\end{pmatrix} \begin{pmatrix}B' & M \\ M& B\end{pmatrix}\begin{pmatrix}\chi\\ \eta\end{pmatrix}.</math>
\frac{1}{2} \, \begin{pmatrix} \chi & \eta \end{pmatrix}
Since the right-handed neutrino spinor is uncharged under all standard model gauge symmetries, ''B'' is a free parameter which can in principle take any arbitrary value.
\begin{pmatrix} B' & M \\
M & B \end{pmatrix}
\begin{pmatrix} \chi \\
\eta \end{pmatrix} .</math>
Since the right-handed neutrino spinor is uncharged under all standard model gauge symmetries, {{mvar|B}} is a free parameter which can in principle take any arbitrary value.


The parameter ''M'' is forbidden by [[Electroweak interaction|electroweak gauge symmetry]], and can only appear after its [[spontaneous symmetry breaking|spontaneous breakdown]] through a [[Higgs mechanism]], like the Dirac masses of the charged leptons. In particular, since {{nowrap|''χ''''L''}} has [[weak isospin]] ½ like the [[Higgs field]] ''H'', and ''η'' has [[weak isospin]] 0, the mass parameter ''M'' can be generated from [[Yukawa interaction]]s with the [[Higgs field]], in the conventional standard model fashion,
The parameter {{mvar|M}} is forbidden by [[Electroweak interaction|electroweak gauge symmetry]], and can only appear after the symmetry has been [[spontaneous symmetry breaking|spontaneously broken]] by a [[Higgs mechanism]], like the Dirac masses of the charged leptons. In particular, since {{nowrap|{{mvar|χ}}{{mvar|L}}}} has [[weak isospin]] {{sfrac|1|2}} like the [[Higgs field]] {{mvar|H}}, and <math> \eta </math> has [[weak isospin]] 0, the mass parameter {{mvar|M}} can be generated from [[Yukawa interaction]]s with the [[Higgs field]], in the conventional standard model fashion,
:<math>\mathcal{L}_{yuk}=y \, \eta L \epsilon H^*+...</math>
: <math> \mathcal{L}_{yuk}=y \, \eta L \epsilon H^* + ... </math>
This means that ''M'' is [[Naturalness (physics)|naturally]] of the order of the [[vacuum expectation value]] of the standard model [[Higgs field]],
:<math>\text{VEV }v\approx 246 \text{ GeV}, \qquad\qquad |\langle H \rangle|= v/\sqrt{2}
</math>
:<math>M_t= O( v/\sqrt{2})\approx 174 \text{ GeV}~,</math>
if the dimensionless [[Yukawa interaction|Yukawa coupling]] is of order {{nowrap|''y'' ≈ 1}}. It can be chosen smaller consistently, but extreme values {{nowrap|''y'' ≫ 1}} can make the model [[Perturbation theory (quantum mechanics)|nonperturbative]].


This means that {{mvar|M}} is naturally of the order of the [[vacuum expectation value]] of the standard model [[Higgs field]],
The parameter ''B''', on the other hand, is forbidden, since no [[renormalizable]] singlet under [[weak hypercharge]] and [[weak isospin|isospin]] can be formed using these doublet components−−only a nonrenormalizable, dimension 5 term is allowed. This is the origin of the pattern and hierarchy of scales of the mass matrix ''A'' within the "type 1" seesaw mechanism.
: the [[vacuum expectation value]] (VEV)<math>\quad v \; \approx \; \mathrm{ 246 \; GeV }, \qquad \qquad | \langle H \rangle| \; = \; v / \sqrt{2} </math>
: <math> M_t = \mathcal{O} \left( v / \sqrt{2} \right) \; \approx \; \mathrm{ 174 \; GeV } ,</math>
if the dimensionless [[Yukawa interaction|Yukawa coupling]] is of order <math> y \approx 1 </math>. It can be chosen smaller consistently, but extreme values <math> y \gg 1 </math> can make the model [[Perturbation theory (quantum mechanics)|nonperturbative]].


The parameter <math> B' </math> on the other hand, is forbidden, since no [[renormalizable]] singlet under [[weak hypercharge]] and [[weak isospin|isospin]] can be formed using these doublet components &ndash; only a nonrenormalizable, dimension&nbsp;5 term is allowed. This is the origin of the pattern and hierarchy of scales of the mass matrix <math> A </math> within the "Type&nbsp;1" seesaw mechanism.
The large size of ''B'' can be motivated in the context of [[Grand unification theory|grand unification]]. In such models, enlarged [[Gauge theory|gauge symmetries]] may be present, which initially force {{nowrap|''B'' {{=}} 0}} in the unbroken phase, but generate a non vanishing large value {{nowrap|''B'' ≈ ''M''<sub>GUT</sub>}} ≈ 10<sup>15</sup> GeV, around the scale of their [[spontaneous symmetry breaking]], so, given an ''M'' ≈ 100 GeV, one has λ<sub>−</sub> ≈ 0.01 eV. A huge scale has thus induced a dramatically small neutrino mass for the eigenvector ''ν'' ≈ ''χ'' − ''(M/B) η'' .

The large size of {{mvar|B}} can be motivated in the context of [[Grand unification theory|grand unification]]. In such models, enlarged [[Gauge theory|gauge symmetries]] may be present, which initially force <math> B = 0 </math> in the unbroken phase, but generate a large, non-vanishing value <math> B \approx M_\mathsf{GUT} \approx \mathrm{10^{15}~GeV},</math> around the scale of their [[spontaneous symmetry breaking]]. So given a mass <math>M \approx \mathrm{ 100 \; GeV }</math> one has <math>\lambda_{(-)} \; \approx \; \mathrm{ 0.01 \; eV }.</math> A huge scale has thus induced a dramatically small neutrino mass for the eigenvector <math> \nu \approx \chi - \frac{\; M \;}{B} \eta .</math>


== See also ==
== See also ==
Line 50: Line 62:
* [[Spinor]]
* [[Spinor]]


==References==
== Footnotes ==
{{notelist|1}}
<references/>

== References ==
{{reflist|25em|refs=

<ref name=GellMann-1979>
{{cite book
|first1=M. |last1=Gell-Mann |author1-link=Murray Gell-Mann
|first2=P. |last2=Ramond |author2-link=Pierre Ramond
|first3=R. |last3=Slansky |author3-link=Richard Slansky
|year=1979
|title=Supergravity
|editor1-first=D. |editor1-last=Freedman
|editor2-first=P. |editor2-last=van Nieuwenhuizen
|publisher=North Holland
|place=Amsterdam, NL
|pages=315–321
|isbn=044485438X
}}
</ref>

<ref name=Glashow-1979-NATO>
{{cite journal
|first=S.L. |last=Glashow |author-link=Sheldon Glashow
|year=1980
|title=The future of elementary particle physics
|editor1-first=Maurice |editor1-last=Lévy
|editor2-first=Jean-Louis |editor2-last=Basdevant
|editor3-first=David |editor3-last=Speiser
|editor4-first=Jacques |editor4-last=Weyers
|editor5-first=Raymond |editor5-last=Gastmans
|editor6-first=Maurice |editor6-last=Jacob
|journal=NATO Sci. Ser. B
|volume=61 |pages=687
|doi=10.1007/978-1-4684-7197-7
|isbn=978-1-4684-7199-1
}}
</ref>

<ref name=Minkowski-1977-1biln-μ>
{{cite journal
|first=P. |last=Minkowski |author-link=Peter Minkowski
|year=1977
|title={{nobr|μ → e ''γ''}} at a rate of one out of 1&nbsp;billion muon decays?
|bibcode=1977PhLB...67..421M
|journal=Physics Letters B
|volume=67 |issue=4 |page=421
|doi=10.1016/0370-2693(77)90435-X
}}
</ref>

<ref name=Mohapatra-Senjanovic-1980>
{{cite journal
|first1=R.N. |last1=Mohapatra |author1-link=Rabindra Mohapatra
|first2=G. |last2=Senjanovic |author2-link=Goran Senjanović
|year=1980
|title=Neutrino mass and spontaneous parity non-conservation
|journal=Phys. Rev. Lett.
|volume=44 |issue=14 |pages=912–915
|doi=10.1103/PhysRevLett.44.912
|bibcode=1980PhRvL..44..912M
}}
</ref>

<ref name=Schechter-Valle-1980>
{{cite journal
|first1=J. |last1=Schechter
|first2=J. |last2=Valle |author2-link=José W. F. Valle
|year=1980
|journal=Phys. Rev.
|volume=22 |issue=9 |pages=2227–2235
|doi=10.1103/PhysRevD.22.2227
|title=Neutrino masses in SU(2) ⊗ U(1) theories
|bibcode=1980PhRvD..22.2227S
}}
</ref>

<ref name=Yanagida-1980-HorizSym>
{{cite journal
|first=T. |last=Yanagida |author-link=Tsutomu Yanagida
|year=1980
|title=Horizontal symmetry and masses of neutrinos
|journal=Progress of Theoretical Physics
|volume=64 |issue=3 |pages=1103–1105
|doi=10.1143/PTP.64.1103 |doi-access=free
|bibcode=1980PThPh..64.1103Y
}}
</ref>

}}


==External links==
== External links ==
* {{cite web
* [http://www.quantumfieldtheory.info/TheSeesawMechanism.htm Seesaw Mechanism details]
|title=Seesaw Mechanism details
|website=quantumfieldtheory.info
|url=http://www.quantumfieldtheory.info/TheSeesawMechanism.htm
}}


{{DEFAULTSORT:Seesaw Mechanism}}
{{DEFAULTSORT:Seesaw Mechanism}}
[[Category:Particle physics]]
[[Category:Neutrinos]]
[[Category:Neutrinos]]
[[Category:Quantum field theory]]
[[Category:Physics beyond the Standard Model]]

Latest revision as of 15:48, 22 August 2024

In the theory of grand unification of particle physics, and, in particular, in theories of neutrino masses and neutrino oscillation, the seesaw mechanism is a generic model used to understand the relative sizes of observed neutrino masses, of the order of eV, compared to those of quarks and charged leptons, which are millions of times heavier. The name of the seesaw mechanism was given by Tsutomu Yanagida in a Tokyo conference in 1981.

There are several types of models, each extending the Standard Model. The simplest version, "Type 1", extends the Standard Model by assuming two or more additional right-handed neutrino fields inert under the electroweak interaction,[a] and the existence of a very large mass scale. This allows the mass scale to be identifiable with the postulated scale of grand unification.

Type 1 seesaw

[edit]

This model produces a light neutrino, for each of the three known neutrino flavors, and a corresponding very heavy neutrino for each flavor, which has yet to be observed.

The simple mathematical principle behind the seesaw mechanism is the following property of any 2×2 matrix of the form

It has two eigenvalues:

and

The geometric mean of and equals , since the determinant .

Thus, if one of the eigenvalues goes up, the other goes down, and vice versa. This is the point of the name "seesaw" of the mechanism.

In applying this model to neutrinos, is taken to be much larger than Then the larger eigenvalue, is approximately equal to while the smaller eigenvalue is approximately equal to

This mechanism serves to explain why the neutrino masses are so small.[1][2][3][4][5][6][7][8] The matrix A is essentially the mass matrix for the neutrinos. The Majorana mass component is comparable to the GUT scale and violates lepton number conservation; while the Dirac mass components are of order of the much smaller electroweak scale, called the VEV or vacuum expectation value below. The smaller eigenvalue then leads to a very small neutrino mass, comparable to eV, which is in qualitative accord with experiments—sometimes regarded as supportive evidence for the framework of Grand Unified Theories.

Background

[edit]

The 2×2 matrix A arises in a natural manner within the standard model by considering the most general mass matrix allowed by gauge invariance of the standard model action, and the corresponding charges of the lepton- and neutrino fields.

Call the neutrino part of a Weyl spinor a part of a left-handed lepton weak isospin doublet; the other part is the left-handed charged lepton

as it is present in the minimal standard model with neutrino masses omitted, and let be a postulated right-handed neutrino Weyl spinor which is a singlet under weak isospin – i.e. a neutrino that fails to interact weakly, such as a sterile neutrino.

There are now three ways to form Lorentz covariant mass terms, giving either

and their complex conjugates, which can be written as a quadratic form,

Since the right-handed neutrino spinor is uncharged under all standard model gauge symmetries, B is a free parameter which can in principle take any arbitrary value.

The parameter M is forbidden by electroweak gauge symmetry, and can only appear after the symmetry has been spontaneously broken by a Higgs mechanism, like the Dirac masses of the charged leptons. In particular, since χL has weak isospin 1/2 like the Higgs field H, and has weak isospin 0, the mass parameter M can be generated from Yukawa interactions with the Higgs field, in the conventional standard model fashion,

This means that M is naturally of the order of the vacuum expectation value of the standard model Higgs field,

the vacuum expectation value (VEV)

if the dimensionless Yukawa coupling is of order . It can be chosen smaller consistently, but extreme values can make the model nonperturbative.

The parameter on the other hand, is forbidden, since no renormalizable singlet under weak hypercharge and isospin can be formed using these doublet components – only a nonrenormalizable, dimension 5 term is allowed. This is the origin of the pattern and hierarchy of scales of the mass matrix within the "Type 1" seesaw mechanism.

The large size of B can be motivated in the context of grand unification. In such models, enlarged gauge symmetries may be present, which initially force in the unbroken phase, but generate a large, non-vanishing value around the scale of their spontaneous symmetry breaking. So given a mass one has A huge scale has thus induced a dramatically small neutrino mass for the eigenvector

See also

[edit]

Footnotes

[edit]
  1. ^ It is possible to generate two low-mass neutrinos with only one right-handed neutrino, but the resulting mass spectra are generally not viable.

References

[edit]
  1. ^ Minkowski, P. (1977). "μ → e γ at a rate of one out of 1 billion muon decays?". Physics Letters B. 67 (4): 421. Bibcode:1977PhLB...67..421M. doi:10.1016/0370-2693(77)90435-X.
  2. ^ Yanagida, T. (1979). "Horizontal gauge symmetry and masses of neutrinos", Proceedings: Workshop on the Unified Theories and the Baryon Number in the Universe: published in KEK Japan, February 13-14, 1979, Conf. Proc. C7902131, p.95- 99.
  3. ^ Yanagida, Tsutomu (1979-12-01). "Horizontal symmetry and mass of the $t$ quark". Physical Review D. 20 (11): 2986–2988. Bibcode:1979PhRvD..20.2986Y. doi:10.1103/PhysRevD.20.2986.
  4. ^ Gell-Mann, M.; Ramond, P.; Slansky, R. (1979). Freedman, D.; van Nieuwenhuizen, P. (eds.). Supergravity. Amsterdam, NL: North Holland. pp. 315–321. ISBN 044485438X.
  5. ^ Yanagida, T. (1980). "Horizontal symmetry and masses of neutrinos". Progress of Theoretical Physics. 64 (3): 1103–1105. Bibcode:1980PThPh..64.1103Y. doi:10.1143/PTP.64.1103.
  6. ^ Glashow, S.L. (1980). Lévy, Maurice; Basdevant, Jean-Louis; Speiser, David; Weyers, Jacques; Gastmans, Raymond; Jacob, Maurice (eds.). "The future of elementary particle physics". NATO Sci. Ser. B. 61: 687. doi:10.1007/978-1-4684-7197-7. ISBN 978-1-4684-7199-1.
  7. ^ Mohapatra, R.N.; Senjanovic, G. (1980). "Neutrino mass and spontaneous parity non-conservation". Phys. Rev. Lett. 44 (14): 912–915. Bibcode:1980PhRvL..44..912M. doi:10.1103/PhysRevLett.44.912.
  8. ^ Schechter, J.; Valle, J. (1980). "Neutrino masses in SU(2) ⊗ U(1) theories". Phys. Rev. 22 (9): 2227–2235. Bibcode:1980PhRvD..22.2227S. doi:10.1103/PhysRevD.22.2227.
[edit]