Effects of Neutron-Antineutron Transitions in Neutron Stars
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.
Authors
- Rabindra N. Mohapatra (ORCID: https://orcid.org/0000-0003-0128-9160)
- S. Nussinov
- I. Goldman (ORCID: https://orcid.org/0000-0001-6200-7898)
- Robert Shrock (ORCID: https://orcid.org/0000-0001-6541-0893)
Institutions
- Tel Aviv University (IL)
- Stony Brook University (US)
- University of Maryland, College Park (US)
Publication Details
- Journal
- Physical Review Letters
- Published
- 2025-02-04
- DOI
- https://doi.org/10.1103/physrevlett.134.052701
- Citations
- 2
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 2.31
Funders
- National Science Foundation