07.01.2014 Views

PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute

PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute

PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Using the same arguments as above, it is not hard to see that the deviation from u 1 = u 2<br />

is also mild. Again, u 1 = u 2 is satisfied when h ′ 6 = 0 and h ′′<br />

6 = 0. Since h 6 = 0 is<br />

also required for |v 1 | = |v 2 | to be satisfied, we conclude that exact µ − τ symmetry for<br />

neutrinos demands that h 6 = 0, h ′ 6 = 0 and h′′ 6 = 0 simultaneously.<br />

Finally, from the last minimization condition (6.56) we get the solution,<br />

|v c | 2 = 1<br />

4h 3<br />

[<br />

2h 6 (|v 2 | 2 −|v 1 | 2 )+2h ′′<br />

6 (u2 2 −u2 1 )−2l′′ 1 (u2 1 +u2 2 )+2h 1<br />

−2h 4 (|v 1 | 2 +|v 2 | 2 )−8u 1 u 2 l 1 −2l 4 v 2 ]<br />

. (6.67)<br />

We next use use the condition (6.67) to estimate the cut-off scale Λ. Since h 1 define<br />

in Eq. (6.48) gives the square of the mass of the φ e fields, it could be large. The other<br />

couplings h 3 , l 1 , l 4 , h 4 , h ′′<br />

6 , l′′ 1 andh 6 aredimensionless andcanbeassumed tohave roughly<br />

the same order of magnitude which should be much much smaller than h 1 . Dividing both<br />

sides of Eq. (6.67) by Λ 2 and using |v 1 | 2 ≃ |v 2 | 2 = 10 −3 eV 2 , vc ≃ Λ 2×10−2 , u 1,2<br />

≃ Λ 10−1<br />

and hence ( v 1,2<br />

Λ )2 ≪ ( vc<br />

Λ )2 < ( u2 2 −u2 1) < ( u 1,2<br />

Λ 2 Λ )2 , we get 9<br />

Λ 2 ≃<br />

h 1<br />

×10 2 GeV 2 . (6.68)<br />

4l 1 +2l 1<br />

′′<br />

The coupling h 1 has mass dimension 2 and in principle could be large. As an example, if<br />

wetakeh 1 inTeVrange, forexample ifwetake √ h 1 = 10TeV, thenthecut-offscaleofthe<br />

theory is fixed as 10 2 TeV, where we have taken l 1 and l ′′<br />

1 ≃ O(1). From u 1<br />

Λ<br />

= u 2<br />

Λ<br />

∼ 10 −1<br />

and vc ∼ Λ 10−2 , we then obtain u 1,2 = 10 TeV and v c = 1 TeV. The constraints from<br />

the lepton masses themselves do not impose any restriction on the cut-off scale and the<br />

VEVs. One can obtain estimates on them only through limits on the masses of the Higgs.<br />

For instance, from Eqs. (6.38) and (6.39) one could in principle estimate u by measuring<br />

the difference between doubly charged Higgs masses. This could then be combined with<br />

the neutrino data to get Λ, and finally use the charged lepton masses to get v c .<br />

Since we consider a model with triplet Higgs to generate Majorana neutrino masses,<br />

it is pertinent to make some comments regarding breaking of lepton number and possible<br />

creation of a massless goldstone called Majoron [26]. It is possible to break lepton number<br />

explicitly by giving a lepton number to the fields ξ. In that case one would not break<br />

lepton number spontaneously and there would be no Majoron.<br />

These VEV alignments have been obtained by assuming no effect of renormalization<br />

group running. However, it is understood that the running from the high scale where<br />

S 3 is broken to the electroweak scale where the masses are generated, will modify the<br />

9 h 6 ,h ′′<br />

6=0 is motivated from µ−τ symmetry, which together with ( v1<br />

Λ )2 ≪ ( vc<br />

Λ )2 < ( u1<br />

Λ )2 can also lead<br />

to Eq. 6.68. Even for a mild breaking of µ−τ which leads to (u 2 2 −u2 1 ) ≪ u2 1,2 , the equation is valid.<br />

163

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!