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Non-thermal WIMPy Baryogenesis with Primordial Black Hole
Authors
Ki-Young Choi
Jongkuk Kim
Erdenebulgan Lkhagvadorj
Publication date
27 September 2023
Publisher
View
on
arXiv
Abstract
We consider the possibility that the weakly interacting massive particles produced from the evaporation of primordial black hole can explain both the relic density of dark matter and the baryon asymmetry of the Universe, through their annihilation which violate B and CP-symmetry. We find that the primordial black hole with mass less than
1
0
7
g
10^7 {\rm g}
1
0
7
g
is a good candidate as an source of TeV dark matter with the total annihilation cross section
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a
Ο
β©
β²
1
0
β
7
Β
G
e
V
β
2
\left\langle\sigma_a \upsilon\right\rangle \lesssim 10^{-7} \ {\rm GeV}^{-2}
β¨
Ο
a
β
Ο
β©
β²
1
0
β
7
Β
GeV
β
2
and the B-violating scattering cross section
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Ο
B
Ο
β©
β²
2
Γ
1
0
β
9
Β
G
e
V
β
2
\left\langle\sigma_B \upsilon\right\rangle \lesssim 2\times 10^{-9} \ {\rm GeV^{-2}}
β¨
Ο
B
β
Ο
β©
β²
2
Γ
1
0
β
9
Β
Ge
V
β
2
. This large annihilation cross section of dark matter in this model would make it available to search them in the indirect search for dark matter such as gamma-ray or neutrino observations
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oai:arXiv.org:2309.16122
Last time updated on 10/12/2023