TY - CONF
T1 - Binary neutron star mergers of quark matter based nuclear equations of state
AU - Kedia, Atul
AU - Mathews, Grant
AU - Kim, Hee Il
AU - Suh, In Saeng
N1 - Publisher Copyright:
© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
PY - 2022/2/24
Y1 - 2022/2/24
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85183874649&partnerID=8YFLogxK
U2 - 10.1051/epjconf/202226011004
DO - 10.1051/epjconf/202226011004
M3 - Paper
AN - SCOPUS:85183874649
T2 - 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Y2 - 21 September 2021 through 25 September 2021
ER -