Long-term postmerger simulations of relativistic star coalescence: Formation of toroidal remnants and gravitational wave afterglow
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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