Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter

Fuente: arXiv

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Bibliographic Details
Main Authors:	Bhattacharya, Sulagna, Kapadia, Shasvath, Dasgupta, Basudeb
Format:	Preprint
Published:	2025
Subjects:	High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2507.15951