Leptogenesis, primordial gravitational waves, and PBH-induced reheating

We explore the possibility of producing the observed matter-antimatter asymmetry of the Universe uniquely from the evaporation of primordial black holes (PBHs) that are formed in an inflaton-dominated background. Considering the inflaton <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mo stretchy="false">(</a:mo><a:mi>ϕ</a:mi><a:mo stretchy="false">)</a:mo></a:math> to oscillate in a monomial potential <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>V</e:mi><e:mo stretchy="false">(</e:mo><e:mi>ϕ</e:mi><e:mo stretchy="false">)</e:mo><e:mo>∝</e:mo><e:msup><e:mi>ϕ</e:mi><e:mi>n</e:mi></e:msup></e:math>, we show, it is possible to obtain the desired baryon asymmetry via vanilla leptogenesis from evaporating PBHs of initial mass <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mo>≲</i:mo><i:mn>10</i:mn><i:mtext> </i:mtext><i:mtext> </i:mtext><i:mi mathvariant="normal">g</i:mi></i:math>. We find that the allowed parameter space is heavily dependent on the shape of the inflaton potential during reheating (determined by the exponent of the potential <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:mi>n</l:mi></l:math>), the energy density of PBHs (determined by <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"><n:mi>β</n:mi></n:math>), and the nature of the coupling between the inflaton and the Standard Model. To complete the minimal gravitational framework, we also include in our analysis the gravitational leptogenesis setup through inflaton scattering via exchange of graviton, which opens up an even larger window for PBH mass, depending on the background equation of state. We finally illustrate that such gravitational leptogenesis scenarios can be tested with upcoming gravitational wave (GW) detectors, courtesy of the blue-tilted primordial GW with inflationary origin, thus paving a way to probe a PBH-induced reheating together with leptogenesis. Published by the American Physical Society 2024

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Journal
Physical review. D/Physical review. D.
Published
2024-08-26
DOI
https://doi.org/10.1103/physrevd.110.043528
Citations
20
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
6.63

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article

Leptogenesis, primordial gravitational waves, and PBH-induced reheating

Md Riajul Haque, Yann Mambrini, Suruj Jyoti Das, Basabendu Barman
20 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
6.63
article

Leptogenesis, primordial gravitational waves, and PBH-induced reheating

Md Riajul Haque, Yann Mambrini, Suruj Jyoti Das, Basabendu Barman
article en
20 citations

Abstract

We explore the possibility of producing the observed matter-antimatter asymmetry of the Universe uniquely from the evaporation of primordial black holes (PBHs) that are formed in an inflaton-dominated background. Considering the inflaton <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mo stretchy="false">(</a:mo><a:mi>ϕ</a:mi><a:mo stretchy="false">)</a:mo></a:math> to oscillate in a monomial potential <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>V</e:mi><e:mo stretchy="false">(</e:mo><e:mi>ϕ</e:mi><e:mo stretchy="false">)</e:mo><e:mo>∝</e:mo><e:msup><e:mi>ϕ</e:mi><e:mi>n</e:mi></e:msup></e:math>, we show, it is possible to obtain the desired baryon asymmetry via vanilla leptogenesis from evaporating PBHs of initial mass <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mo>≲</i:mo><i:mn>10</i:mn><i:mtext> </i:mtext><i:mtext> </i:mtext><i:mi mathvariant="normal">g</i:mi></i:math>. We find that the allowed parameter space is heavily dependent on the shape of the inflaton potential during reheating (determined by the exponent of the potential <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:mi>n</l:mi></l:math>), the energy density of PBHs (determined by <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"><n:mi>β</n:mi></n:math>), and the nature of the coupling between the inflaton and the Standard Model. To complete the minimal gravitational framework, we also include in our analysis the gravitational leptogenesis setup through inflaton scattering via exchange of graviton, which opens up an even larger window for PBH mass, depending on the background equation of state. We finally illustrate that such gravitational leptogenesis scenarios can be tested with upcoming gravitational wave (GW) detectors, courtesy of the blue-tilted primordial GW with inflationary origin, thus paving a way to probe a PBH-induced reheating together with leptogenesis. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(4)
Indian Institute of Technology Madras (IN), Université Paris-Saclay (FR), Institute for Basic Science (KR), SRM University (IN), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (FR)
Centre National de la Recherche Scientifique, Institute for Basic Science, Horizon 2020 Framework Programme, Science and Engineering Research Board
Openalex Percentile: Top 3%
Cosmology and Gravitation Theories
6.63
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