Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio ef...
Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
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Author / Creator
Camilletti, A , Chiesa, L , Ricigliano, G , Perego, A , Lippold, L C , Padamata, S , Bernuzzi, S , Radice, D , Logoteta, D and Guercilena, F M
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
GW190425 was the second gravitational wave (GW) signal compatible with a binary neutron star (BNS) merger detected by the Advanced LIGO and Advanced Virgo detectors. Since no electromagnetic counterpart was identified, whether the associated kilonova was too dim or the localisation area too broad is still an open question. We simulate 28 BNS merger...
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Full title
Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
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Record Identifier
TN_cdi_proquest_journals_2649831750
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2649831750
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2204.05336
