pith. machine review for the scientific record. sign in

arxiv: hep-ph/9606260 · v2 · submitted 1996-06-07 · ✦ hep-ph · astro-ph

Recognition: unknown

GUT Baryogenesis after Preheating

Authors on Pith no claims yet
classification ✦ hep-ph astro-ph
keywords baryogenesisbaryoninflationorderpreheatingasymmetrybosonbosons
0
0 comments X
read the original abstract

At the end of inflation the universe is frozen in a near zero-entropy state with energy density in a coherent scalar field and must be ``defrosted'' to produce the observed entropy and baryon number. We propose that the baryon asymmetry is generated by the decay of supermassive Grand Unified Theory (GUT) bosons produced non-thermally in a preheating phase after inflation. We show that baryogenesis is possible for an inflaton masses of order 10^{13} GeV and a GUT Higgs boson mass of order 10^{14} GeV, thus solving many drawbacks facing GUT baryogenesis in the old reheating scenario.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Analytic Approximations for Fermionic Preheating

    hep-ph 2026-04 unverdicted novelty 5.0

    Analytic approximations for fermion number density in λφ⁴ preheating scale as q^{1/2} for q ≲ 0.01 and q^{3/4} for q ≳ 10, with resonance peaks or half-filled Fermi spheres depending on the coupling.