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| Main Author: | |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2503.18416 |
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| _version_ | 1866913754169475072 |
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| author | Pozdnyakov, N. A. |
| author_facet | Pozdnyakov, N. A. |
| contents | Additional elementary species and primordial black holes are common candidates for dark matter. Their co-existence in the early Universe leads to accretion if particles are heavy. We solve equation of motion affected by expansion which enhances black hole growth rates. They depend upon particles freeze-out time rather than their mass. Taking into account friction we investigate recently suggested baryogenesis mechanism operating via scattering cross-section difference between particles and antiparticles on relativistic symmetric plasma. We find that asymmetry is accumulated at relatively small times which can be used to construct viable particle models. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_18416 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Accretion in very early Universe and charge asymmetry Pozdnyakov, N. A. Cosmology and Nongalactic Astrophysics Additional elementary species and primordial black holes are common candidates for dark matter. Their co-existence in the early Universe leads to accretion if particles are heavy. We solve equation of motion affected by expansion which enhances black hole growth rates. They depend upon particles freeze-out time rather than their mass. Taking into account friction we investigate recently suggested baryogenesis mechanism operating via scattering cross-section difference between particles and antiparticles on relativistic symmetric plasma. We find that asymmetry is accumulated at relatively small times which can be used to construct viable particle models. |
| title | Accretion in very early Universe and charge asymmetry |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2503.18416 |