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 fieldsinert under the electroweak interaction,and the existence of a very large mass scale. This allows the mass scale to be identifiable with the postulated scale of grand unification.
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
A=\begin{pmatrix}0&M\\ M&B\end{pmatrix}.
λ(+)=
B+\sqrt{B2+4M2 | |
λ(-)=
B-\sqrt{B2+4M2 | |
}{2} |
.
λ(+)
λ(-)
\left|M\right|
λ(+) λ(-)=-M2
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,
B
M.
λ(+),
B,
λ- ≈ -
M2 | |
B |
.
This mechanism serves to explain why the neutrino masses are so small.[1] [2] The matrix is essentially the mass matrix for the neutrinos. The Majorana mass component
B
M
λ(-)
The 2×2 matrix 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.
\chi,
\ell,
L=\begin{pmatrix}\chi\ \ell\end{pmatrix},
η
There are now three ways to form Lorentz covariant mass terms, giving either
\tfrac{1}{2}B'\chi\alpha\chi\alpha,
1 | |
2 |
Bη\alphaη\alpha, or Mη\alpha\chi\alpha,
1 | |
2 |
\begin{pmatrix}\chi&η\end{pmatrix} \begin{pmatrix}B'&M\\ M&B\end{pmatrix} \begin{pmatrix}\chi\\ η\end{pmatrix}.
The parameter is forbidden by electroweak gauge symmetry, and can only appear after the symmetry has been spontaneous broken by a Higgs mechanism, like the Dirac masses of the charged leptons. In particular, since has weak isospin like the Higgs field, and
η
l{L}yuk=yηL\epsilonH*+...
This means that is naturally of the order of the vacuum expectation value of the standard model Higgs field,
the vacuum expectation value (VEV)
v ≈ 246 GeV, |\langleH\rangle| = v/\sqrt{2}
Mt=l{O}\left(v/\sqrt{2}\right) ≈ 174 GeV,
y ≈ 1
y\gg1
The parameter
B'
A
The large size of can be motivated in the context of grand unification. In such models, enlarged gauge symmetries may be present, which initially force
B=0
B ≈ MGUT ≈
1015~GeV, |
M ≈ 100 GeV
λ(-) ≈ 0.01 eV.
\nu ≈ \chi-
M | |
B |
η.