Merger and Postmerger of Binary Neutron Stars with a Quark-Hadron Crossover Equation of State.
Sign Up to like & getrecommendations! Published in 2022 at "Physical review letters"
DOI: 10.1103/physrevlett.129.181101
Abstract: Fully general-relativistic binary-neutron-star (BNS) merger simulations with quark-hadron crossover (QHC) equations of state (EOS) are studied for the first time. In contrast to EOS with purely hadronic matter or with a first-order quark-hadron phase transition… read more here.
Keywords: binary neutron; quark hadron; eos; postmerger ... See more keywords
Long-term postmerger simulations of relativistic star coalescence: Formation of toroidal remnants and gravitational wave afterglow
Sign Up to like & getrecommendations! Published in 2019 at "International Journal of Modern Physics D"
DOI: 10.1142/s0218271819500263
Abstract: It has been estimated that a significant proportion of binary neutron star merger events produce long-lived massive remnants supported by differential rotation and subject to rotational instabilities. To examine formation and oscillation of rapidly rotating… read more here.
Keywords: gravitational wave; term postmerger; postmerger; toroidal ... See more keywords