Baryogenesis during reheating in natural inflation and comments on spontaneous baryogenesis

Alexandre Dolgov, Katherine Freese, Raghavan Rangarajan, and Mark Srednicki
Phys. Rev. D 56, 6155 – Published 15 November 1997
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Abstract

We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson (PNGB) whose interactions violate baryon number conservation. Our results are in disagreement with previous results in the original spontaneous baryogenesis models for the asymmetry produced by the decay of an oscillating scalar field with B-number-violating derivative couplings; we find that the net baryon number density is proportional to θi3, where θi is the amplitude of the PNGB field in natural inflation at the onset of reheating. While our calculation of the asymmetry is carried out in the context of natural inflation our approach is generally valid for baryogenesis models using decaying classical fields. We include a complete derivation of the number density of particles produced by the decay of a classical scalar field.

  • Received 18 April 1997

DOI:https://doi.org/10.1103/PhysRevD.56.6155

©1997 American Physical Society

Authors & Affiliations

Alexandre Dolgov

  • Teoretisk Astrofysik Center, Juliane Maries Vej 30, DK-2100, Copenhagen, Denmark

Katherine Freese

  • Physics Department, University of Michigan, Ann Arbor, Michigan 48109

Raghavan Rangarajan

  • Astroparticle Physics Group, Houston Advanced Research Center, The Mitchell Campus, The Woodlands, Texas 77381

Mark Srednicki

  • Department of Physics, University of California, Santa Barbara, California 93106

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Vol. 56, Iss. 10 — 15 November 1997

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