Minimally modeled characterization method of postmerger gravitational wave emission from binary neutron star coalescences

Gravitational waves emitted during the coalescence of binary neutron star systems carry information about the equation of state describing the extremely dense matter inside neutron stars. In particular, the equation of state determines the fate of the binary after the merger: a prompt collapse to bl...

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Bibliographic Details
Main Authors Tringali, Maria Concetta, Puecher, Anna, Lazzaro, Claudia, Ciolfi, Riccardo, Drago, Marco, Giacomazzo, Bruno, Vedovato, Gabriele, Prodi, Giovanni Andrea
Format Journal Article
LanguageEnglish
Published 25.04.2023
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