We propose a new mechanism for baryogenesis, in which baryon asymmetry is
generated by absorption of a new particle $X$ carrying baryon number onto
Primordial Black Holes (PBHs). Due to CP violation of $X$ and $X$
scattering with the plasma surrounding PBHs, the two conjugate particles are
differently absorbed by PBHs, leading to the production of an asymmetry in the
$X$ sector. The production is halted by PBH evaporation, after which the
asymmetry is transferred into the baryonic sector via $X$ decay. We show that
this mechanism can produce the correct amount of asymmetry without violating
the known constraints on PBHs concentration. Furthermore, we provide a
systematic study of the parameter space, identifying the regions leading to the
production of the correct baryon asymmetry.
Description
Absorption from Primordial Black Holes as source of baryon asymmetry
%0 Generic
%1 ambrosone2021absorption
%A Ambrosone, Antonio
%A Calabrese, Roberta
%A Fiorillo, Damiano F. G.
%A Miele, Gennaro
%A Morisi, Stefano
%D 2021
%K library
%T Absorption from Primordial Black Holes as source of baryon asymmetry
%U http://arxiv.org/abs/2106.11980
%X We propose a new mechanism for baryogenesis, in which baryon asymmetry is
generated by absorption of a new particle $X$ carrying baryon number onto
Primordial Black Holes (PBHs). Due to CP violation of $X$ and $X$
scattering with the plasma surrounding PBHs, the two conjugate particles are
differently absorbed by PBHs, leading to the production of an asymmetry in the
$X$ sector. The production is halted by PBH evaporation, after which the
asymmetry is transferred into the baryonic sector via $X$ decay. We show that
this mechanism can produce the correct amount of asymmetry without violating
the known constraints on PBHs concentration. Furthermore, we provide a
systematic study of the parameter space, identifying the regions leading to the
production of the correct baryon asymmetry.
@misc{ambrosone2021absorption,
abstract = {We propose a new mechanism for baryogenesis, in which baryon asymmetry is
generated by absorption of a new particle $X$ carrying baryon number onto
Primordial Black Holes (PBHs). Due to CP violation of $X$ and $\overline{X}$
scattering with the plasma surrounding PBHs, the two conjugate particles are
differently absorbed by PBHs, leading to the production of an asymmetry in the
$X$ sector. The production is halted by PBH evaporation, after which the
asymmetry is transferred into the baryonic sector via $X$ decay. We show that
this mechanism can produce the correct amount of asymmetry without violating
the known constraints on PBHs concentration. Furthermore, we provide a
systematic study of the parameter space, identifying the regions leading to the
production of the correct baryon asymmetry.},
added-at = {2021-06-24T08:21:22.000+0200},
author = {Ambrosone, Antonio and Calabrese, Roberta and Fiorillo, Damiano F. G. and Miele, Gennaro and Morisi, Stefano},
biburl = {https://www.bibsonomy.org/bibtex/287afe636f8505b893d68b38f1e8fa06b/gpkulkarni},
description = {Absorption from Primordial Black Holes as source of baryon asymmetry},
interhash = {e06bf3589a8739cb6e3673cac183dc67},
intrahash = {87afe636f8505b893d68b38f1e8fa06b},
keywords = {library},
note = {cite arxiv:2106.11980Comment: 7 pages, 3 figures},
timestamp = {2021-06-24T08:21:22.000+0200},
title = {Absorption from Primordial Black Holes as source of baryon asymmetry},
url = {http://arxiv.org/abs/2106.11980},
year = 2021
}