Thermal leptogenesis in brane world cosmology

Nobuchika Okada and Osamu Seto
Phys. Rev. D 73, 063505 – Published 10 March 2006

Abstract

The thermal leptogenesis in brane world cosmology is studied. In brane world cosmology, the expansion law is modified from the four-dimensional standard cosmological one at high temperature regime in the early universe. As a result, the well-known upper bound on the lightest light neutrino mass induced by the condition for the out-of-equilibrium decay of the lightest heavy neutrino, m˜1103eV, can be moderated to be m˜1103eV×(M1/Tt)2 in the case of TtM1 with the lightest heavy neutrino mass (M1) and the “transition temperature” (Tt), at which the modified expansion law in brane world cosmology is smoothly connecting with the standard one. This implies that the degenerate mass spectrum of the light neutrinos can be consistent with the thermal leptogenesis scenario. Furthermore, as recently pointed out, the gravitino problem in supersymmetric case can be solved if the transition temperature is low enough Tt1067GeV. Therefore, even in the supersymmetric case, thermal leptogenesis scenario can be successfully realized in brane world cosmology.

  • Received 29 July 2005

DOI:https://doi.org/10.1103/PhysRevD.73.063505

©2006 American Physical Society

Authors & Affiliations

Nobuchika Okada*

  • Theory Division, KEK, Oho 1-1, Tsukuba, Ibaraki 305-0801, Japan Department of Particle and Nuclear Physics, The Graduate University for Advanced Studies (Sokendai), Oho 1-1, Tsukuba, Ibaraki 305-0801, Japan

Osamu Seto

  • Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QJ, United Kingdom

  • *Electronic address: okadan@post.kek.jp
  • Electronic address: O.Seto@sussex.ac.uk

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Issue

Vol. 73, Iss. 6 — 15 March 2006

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