PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute
PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute
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