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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Main Authors | , , , , , , , |
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Format | Journal Article |
Language | English |
Published |
25.04.2023
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Subjects | |
Online Access | Get full text |
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