Gravitational wave emission in binary neutron star early post-merger within a dark environment

Using an effective Lagrangian model inspired by Takami et al. [1] we qualitatively study the early post-merger of a nearly symmetric binary Neutron Star (BNS) merger event with a non-vanishing ambient fraction of dark matter. For this we first mimic the dynamics of two oscillating Neutron Star (NS)...

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Bibliographic Details
Main Authors: D. Suárez-Fontanella, D. Barba-González, C. Albertus, M. Ángeles Pérez-García
Format: Article
Language:English
Published: Elsevier 2025-03-01
Series:Physics Letters B
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Online Access:http://www.sciencedirect.com/science/article/pii/S0370269325001182
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