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PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute

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theory. The fields which get integrated out can be either a gauge singlet neutrino field<br />

N R , or the SU(2) triplet field ∆ with hypercharge Y = +2, or an SU(2) triplet field Σ R<br />

with hypercharge Y = 0. Accordingly, the seesaw is characterized as type-I, type-II and<br />

type-IIIseesaw respectively. InFig. 2.3we present theFeynmandiagramofthefourpoint<br />

function LLHH. For the type-I seesaw, the coupling κ ij is Y T ν i<br />

Y νj<br />

M<br />

while for type-III and<br />

type-II seesaw the coupling κ ij is Y Σ T Y Σj i and Y ∆µ ∆<br />

respectively, where Y<br />

M M∆<br />

2 ν , Y Σ and Y ∆ are<br />

the Yukawa couplings and µ ∆ is the coupling between Higgs triplet ∆ and the standard<br />

model Higgs doublet H. Below, we discuss in detail the different seesaw mechanisms.<br />

Type-I Seesaw<br />

The standard model is extended by adding the gauge singlet right handed neutrino N R .<br />

The Majorana neutrino in this case is N = N R +NR C . The right handed neutrino being a<br />

gauge singlet, interacts only with the standard model lepton doublet L and the Higgs H<br />

via the Yukawa interaction,<br />

−L Y = Y ν ¯NR ˜H† L+ 1 2 M ¯N R N C R<br />

+h.c, (2.14)<br />

where ˜H = iσ 2 H ∗ and M is the lepton number violating mass term of the right handed<br />

neutrino N R . After the Higgs H takes vacuum expectation value v, the following neutrino<br />

mass matrix will be generated from Eq. (2.14),<br />

L m = 1 2<br />

( ) (<br />

ν<br />

C<br />

0 vYν<br />

T<br />

L<br />

N R<br />

vY ν M<br />

)(<br />

νL<br />

N C R<br />

)<br />

+h.c. (2.15)<br />

Assuming M ≫ vY ν , the diagonalization of the mass matrix gives two eigenvalues M and<br />

m ν ∼ m T D M−1 m D , where we have defined m D = vY ν . One can identify the eigenvalue M<br />

as the mass matrix of the heavy right handed neutrino and the later one m ν is the mass<br />

matrix of the standard model neutrinos.<br />

Type-II Seesaw<br />

Standard model neutrino masses can be generated by adding the SU(2) triplet Higgs<br />

to the standard model field contents [24]. The Higgs triplet ∆ has U(1) Y hypercharge<br />

Y = +2 and has the following Yukawa interaction,<br />

−L Y = Y ∆ L T Ciσ 2 ∆L+h.c (2.16)<br />

where the Higgs triplet ∆ is,<br />

(<br />

∆<br />

∆ =<br />

+ / √ 2 ∆ ++<br />

∆ 0 −∆ + / √ 2<br />

)<br />

. (2.17)<br />

21

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