Matches in SemOpenAlex for { <https://semopenalex.org/work/W2897513152> ?p ?o ?g. }
- W2897513152 abstract "It was recently suggested that dark matter consists of ~GeV particles that carry baryon number and mix with the neutron. We demonstrate that this could allow for resonant dark matter-neutron oscillations in the early universe, at finite temperature, leading to low-scale baryogenesis starting from a primordial dark matter asymmetry. In this scenario, the asymmetry transfer happens around 30 MeV, just before big bang nucleosynthesis. We illustrate the idea using a model with a dark U(1)' gauge interaction, which has recently been suggested as a way of addressing the neutron lifetime anomaly. The asymmetric dark matter component of this model is both strongly self-interacting and leads to a suppression of matter density perturbations at small scales, allowing to mitigate the small-scale problems of cold dark matter cosmology. Future CMB experiments will be able to consistently probe, or firmly exclude, this scenario." @default.
- W2897513152 created "2018-10-26" @default.
- W2897513152 creator A5009912646 @default.
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- W2897513152 date "2019-02-19" @default.
- W2897513152 modified "2023-10-17" @default.
- W2897513152 title "Baryogenesis from neutron-dark matter oscillations" @default.
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- W2897513152 doi "https://doi.org/10.1103/physrevd.99.035024" @default.
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