2003/09/17 by Xiao-Jun Bi, Bo Feng, Bi, Xiao-Jun +3
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0309195
28 pages, 12 figures; new references added
arxiv created 2003/09/19 · arxiv updated 2009/12/01
In this paper we study double scalar neutrino inflation in the minimal supersymmetric seesaw model in light of WMAP. Inflation in this model is firstly driven by the heavier sneutrino field N2 and then the lighter field N1. we will show that with the mass ratio 6\lesssim M2/M1 \lesssim 10 the model predicts a suppressed primordial scalar spectrum around the largest scales and the predicted CMB TT quadrupole is much better suppressed than the single sneutrino model. So this model is more favored than the single sneutrino inflation model. We then consider the implications of the model on the reheating temperature, leptogenesis and lepton flavor violation. Our results show that the seesaw parameters are constrained strongly by the reheating temperature, together with the requirement by a successful inflation. The mixing between the first generation and the other two generations in the right-handed neutrino sector is tiny. The rates of lepton flavor violating processes in our scenario depend on only 4 unknown seesaw parameters through a 'reduced' seesaw formula, besides Ue3 and the supersymmetric parameters. We find that the branching ratio of μ→ e γ is generally near the present experimental limit, while \rm Br(τ→ μγ) is around O(10-10 - 10-9).