PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute
PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute
PHYS08200604017 Manimala Mitra - Homi Bhabha National Institute
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
The most important characteristics of our model are the following:<br />
1. Presence of µ-τ symmetry in Y Σ and M. This is expected to show-up in the flavor<br />
of the final state lepton coming directly from the Σ ±/0 decay vertex.<br />
2. Presence of two CP even neutral Higgses (h 0 and H 0 ), one CP odd neutral Higgs<br />
(A 0 ), and a pair of charged Higgs (H ± ).<br />
3. Predominant decay of the heavy fermions into light leptons, and h 0 , A 0 or H ± .<br />
Decays into H 0 and gauge bosons almost never happen.<br />
4. Very short lifetime for the heavy fermion due to the very large Yukawa couplings.<br />
5. Predominant decay of h 0 and A 0 into b¯b pairs 88-89% and 87% of the time, respectively.<br />
They decay also into τ¯τ 7-9% of the time.<br />
6. Very large lifetime of h 0 .<br />
7. The Higgs H ± decays into W ± h 0 and almost never into W ± H 0 .<br />
In what follows, we will use these model characteristics to identify the different final state<br />
channels atthecollider. Weidentify thepossiblechannels inthecollider forourmodeland<br />
calculate the respective effective cross-sections. The results are given in Tables 3.8, 3.9<br />
and 3.10. We will also discuss some of the most important channels and the characteristic<br />
backgrounds, if any, associated with them. In this section we have only given results for<br />
effective cross-sections for the decay of Σ ±/0<br />
1 with M Σ1 = 300 GeV. Results for the other<br />
heavy fermion generations can be similarly obtained. We have considered the light Higgs<br />
mass M h 0 = 40GeV, while calculating theeffective crosssections given inTable3.8, Table<br />
3.9 and Table 3.10. For the other choice M h 0=70 GeV, the effective cross section does not<br />
change significantly. However, as an example we have also calculated the effective cross<br />
section for few of the significant channels which have large cross section and tabulate<br />
them in Table 3.12 for the case M h 0 = 70 GeV.<br />
3.8.1 Signatures from Σ + Σ − decays<br />
We give in Table 3.8 the possible collider signatures coming from the decay of Σ + Σ −<br />
pairs, for our two Higgs doublet type-III seesaw model. In the last column we also give<br />
the corresponding effective cross-sections for these channels in units of fb. The final crosssectionscanbeobtainedonlyafterputtinginthevariouscutsandefficiencyfactors.<br />
These<br />
efficiency factors will have to be folded with the cross-sections given in Table 3.8 to get<br />
the final effective cross-sections for the various channels. We have not addressed these<br />
issues in this present work. Few clarifications on our notation is in order. Light charged<br />
leptons could be released in the final state through two ways: (i) from the decay of the<br />
65