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arXiv · 2505.09190

Neutron Decay Anomaly and Its Effects on Neutron Star Properties

H. C. Das·G. F. Burgio
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Abstract

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 ($\geq 2 M_\odot$), the NICER mass-radius limits, and the tidal deformability constraint from the GW170817 event. The equation of states of the NS admixed with DM (DMANS) are calculated by incorporating the self-interactions between them. The macroscopic properties, such as mass, radius, and tidal deformability of the NSs, are obtained for HCD models along with five others by varying self-interaction strength. By combining NS observations with scattering cross-section constraints from galaxy clusters, we explore model-dependent trends in the DM self-interaction parameter space. While the quantitative bounds may vary with hadronic model choice, our analysis offers insights into the interplay between DM interactions and NS observables within the RMF framework.

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H. C. Das, G. F. Burgio. 2025-05-14. Neutron Decay Anomaly and Its Effects on Neutron Star Properties. https://doi.org/10.3390/universe11050159

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