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Neutron Stars with Baryon Number Violation, Probing Dark Sectors
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The neutron lifetime anomaly has been used to motivate the introduction of new physics with hidden-sector particles coupled to baryon number, and on which neutron stars provide powerful constraints. Although the neutron lifetime anomaly may eventually prove to be of mundane origin, we use it as motivation for a broader review of the ways that baryon number violation, be it real or apparent, and dark sectors can intertwine and how neutron star observables, both present and future, can constrain them.
Forward citations
Cited by 2 Pith papers
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Dark-matter induced neutron-antineutron oscillations
True QCD axion dark matter cannot induce observable neutron-antineutron oscillations, because its Goldstone nature forces competing axionless baryon-number-violating effects that are already ruled out.
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Melvin--Bonnor and Bertotti--Robinson spacetimes with Baryonic charge
For magnetized Melvin–Bonnor black holes, the paper derives a closed analytic relation between the mass parameter and a regularized baryonic charge, claimed to be linear at large mass.
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