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• W1552854258 abstract "We demonstrate by a large set of merger simulations for symmetric binary neutron stars (NSs) that there is a tight correlation between the frequency peak of the postmerger gravitational-wave (GW) emission and the physical properties of the nuclear equation of state (EoS), e.g. expressed by the radius of the maximum-mass Tolman-Oppenheimer-Volkhoff configuration. Therefore, a single measurement of the peak frequency of the postmerger GW signal will constrain the NS EoS significantly. For plausible optimistic merger-rate estimates a corresponding detection with Advanced LIGO is likely to happen within an operation time of roughly a year." @default.
• W1552854258 created "2016-06-24" @default.
• W1552854258 creator A5013266043 @default.
• W1552854258 creator A5018418874 @default.
• W1552854258 date "2012-01-05" @default.
• W1552854258 modified "2023-10-18" @default.
• W1552854258 title "Measuring Neutron-Star Properties via Gravitational Waves from Neutron-Star Mergers" @default.
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• W1552854258 doi "https://doi.org/10.1103/physrevlett.108.011101" @default.
• W1552854258 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/22304250" @default.
• W1552854258 hasPublicationYear "2012" @default.
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