EPJ Web Conf.
Volume 260, 2022The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
|Number of page(s)||4|
|Published online||24 February 2022|
Binary neutron star mergers of quark matter based nuclear equations of state
1 Center for Astrophysics, Department of Physics, University of Notre Dame, Indiana, USA
2 Center for Quantum Spacetime, Sogang University, Seoul 04107, Korea
3 Center for Research Computing, University of Notre Dame, Indiana, USA
Published online: 24 February 2022
With observations of gravitational wave signals from binary neutron star mergers (BNSM) by LIGO-Virgo-KAGRA (LVK) Collaboration and NICER, the nuclear equation of state (EOS) is becoming increasingly testable by complementary numerical simulations. Numerous simulations currently explore the EOS at different density regimes for the constituent neutron stars speciﬁcally narrowing the uncertainty in the sub-nuclear densities. In this paper we summarize the three-dimensional general relativistic-hydrodynamics based simulations of BNSMs for EOSs with a speciﬁc emphasis on the quark matter EOS at the highest densities.
© The Authors, published by EDP Sciences, 2022
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