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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triplet representation of A 4 ,<br />
l = (L e ,L µ ,L τ ) T ,<br />
where L α denotes the standard model lepton doublets. The right handed charged leptons<br />
e R , µ R and τ R are assumed to belong to the 1, 1 ′ and 1 ′′ representation respectively. The<br />
standard Higgs doublets H u and H d remain invariant under A 4 . The form of the A 4<br />
invariant Yukawa part of the Lagrangian is<br />
L Y = y e e R (φ T l)+y µ µ R (φ T l) ′ +y τ τ R (φ T l) ′′ +x a ξ(ll)+x ′ a ξ′ (ll) ′′ +x ′′<br />
a ξ′′ (ll) ′<br />
+x b (φ S ll)+h.c.+... (5.3)<br />
where, following [14] we have used the compact notation, y e e R (φ T l) ≡ y e e R (φ T l)H d /Λ,<br />
x a ξ(ll) ≡ x a ξ(lH u lH u )/Λ 2 and so on, and Λ is the cut-off scale of the theory. Here we<br />
adopt an effective field theory approach. We assume that φ S does not couple to charged<br />
leptons and φ T does not contribute to the Majorana mass matrix. These two additional<br />
features can be obtained by introducing extra abelian symmetries for example Z 3 [14].<br />
After the spontaneous breaking of A 4 followed by SU(2) L<br />
×U(1) Y<br />
, we get the mass terms<br />
for the charged leptons and neutrinos. Assuming the vacuum alignment<br />
the charged lepton mass matrix is given as<br />
⎛<br />
m cl = v dv T<br />
Λ<br />
〈φ T 〉 = (v T ,0,0) , (5.4)<br />
⎝<br />
⎞<br />
y e 0 0<br />
0 y µ 0 ⎠ , (5.5)<br />
0 0 y τ<br />
Note that we could also obtain a diagonal charged lepton mass matrix even if we assume<br />
that e R , µ R and τ R transform as 1 ′′ , 1 ′ and 1, and 〈φ T 〉 = (0,v T ,0) with appropriate<br />
change in the Yukawa Lagrangian. Similarly, e R , µ R and τ R transforming 1 ′ , 1 and 1 ′′ ,<br />
and 〈φ T 〉 = (0,0,v T ) could give us the same m cl .<br />
In the most general case, where all three one dimensional A 4 Higgs as well as φ S<br />
are present and we do not assume any particular vacuum alignment, the neutrino mass<br />
matrix looks like<br />
⎛<br />
m ν = m 0<br />
⎝ a+2b ⎞<br />
1/3 c−b 3 /3 d−b 2 /3<br />
c−b 3 /3 d+2b 2 /3 a−b 1 /3 ⎠ , (5.6)<br />
d−b 2 /3 a−b 1 /3 c+2b 3 /3<br />
where m 0 = v2 v<br />
u<br />
Λ<br />
b i = 2x<br />
Si<br />
b , a = 2x Λ a u, c = Λ 2x′′ a u′′ and d = Λ 2x′ a u′<br />
Λ<br />
VEVs as<br />
and we have written the<br />
〈φ S 〉 = (v S1 ,v S2 ,v S3 ), 〈ξ〉 = u, 〈ξ ′ 〉 = u ′ , 〈ξ ′′ 〉 = u ′′ , 〈H u,d 〉 = v u,d . (5.7)<br />
For simplicity, in this work we have considered all the Yukawa couplings as well as the<br />
parameters a,b,c and d as real.<br />
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