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Author

Soham Singh

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Preprint Oct 2026

Neutron-star dark-matter limits measure the maximum-mass headroom

Neutron stars constrain dark matter that is present inside them, through their maximum mass and the tidal deformability. The standard approach adds a dark component to one nuclear equation of state (EoS) and compares the stars with pulsar masses and with GW170817, so each limit inherits an EoS dependence that has not b...

P. J. Kalita, Soham Singh, Pinku Routaray et al. · 0 citations

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