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Effects of Neutron-Antineutron Transitions in Neutron Stars

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arxiv 2408.14555 v1 pith:6R47TQXQ submitted 2024-08-26 hep-ph astro-ph.HE

Itzhak Goldman , Rabindra N. Mohapatra , Shmuel Nussinov , Robert Shrock This is my paper · ORCID
classification hep-phastro-ph.HE
keywords effectsneutronneutron-antineutronstarstransitionsanalyzebinarycooling
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We analyze effects of neutron-antineutron transitions in neutron stars, specifically on (i) cooling, (ii) rotation rate, and (iii) for binary pulsars, the increase in the orbital period. We show that these effects are negligibly small.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dark-matter induced neutron-antineutron oscillations

    hep-ph 2024-12 conditional novelty 7.0 of 10

    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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