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Neutron Decay Anomaly and Its Effects on Neutron Star Properties

We investigate the effects of dark matter (DM) on neutron star (NS) properties using the neutron decay anomaly model within the relativistic mean-field (RMF) framework. Three nucleonic models (HCD0–HCD2) are developed, satisfying astrophysical constraints such as the maximum NS mass (≥<inline-formul...

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Bibliográfalaš dieđut
Váldodahkkit: H. C. Das, G. F. Burgio
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: MDPI AG 2025-05-01
Ráidu:Universe
Fáttát:
Liŋkkat:https://www.mdpi.com/2218-1997/11/5/159
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