pith. sign in

arxiv: astro-ph/0009407 · v1 · submitted 2000-09-26 · 🌌 astro-ph

Gravitational waves, baryogenesis, and dark matter from primordial black holes

A. D. Dolgov , P. D. Naselsky , I. D. Novikov This is my paper
classification 🌌 astro-ph
keywords blackprimordialasymmetrybaryogenesisbaryoncosmologicaldarkdiscuss
0
0 comments X
read the original abstract

We discuss the hypothesis that the cosmological baryon asymmetry and entropy were produced in the early Universe by the primordial black hole (PBHs) evaporation.

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 2 Pith papers

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

  1. Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component

    hep-ph 2026-05 unverdicted novelty 7.0

    Accounting for the minimal mass spread of primordial black holes from gravitational collapse suppresses the Poltergeist GW background to the level of generic scalar-induced signals and reopens ultra-light PBH parameter space.

  2. Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist

    hep-ph 2026-05 unverdicted novelty 6.0

    Incorporating the general-relativity mass tail df_PBH/d ln M ∝ M^3.78 smooths PBH evaporation, suppresses the scalar-induced GW signal by orders of magnitude, and reopens the ultra-light PBH window for the hot Big Bang.