Published 2022
| Version v1
Journal article
Binary neutron star mergers of quark matter based nuclear equations of state
- 1. Center for Astrophysics, Department of Physics, University of Notre Dame, Indiana (United States)
- 2. Center for Quantum Spacetime, Sogang University, Seoul 04107 (Korea, Republic of)
- 3. Center for Research Computing, University of Notre Dame, Indiana (United States)
Description
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 specically 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 specic emphasis on the quark matter EOS at the highest densities.
Availability note (English)
Available from https://www.epj-conferences.org/articles/epjconf/pdf/2022/04/epjconf_nic16th2022_11004.pdf; https://doaj.org/article/2a10f562541049978f738f3d00d039f4Additional details
Identifiers
Publishing Information
- Journal Title
- EPJ. Web of Conferences
- Journal Volume
- 260
- Journal Page Range
- vp.
- ISSN
- 2100-014X
Conference
- Title
- 16. International Symposium on Nuclei in the Cosmos
- Dates
- 21-25 Sep 2021
- Place
- Chengdu (China)
INIS
- Country of Publication
- France
- Country of Input or Organization
- France
- INIS RN
- 53090752
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COMPUTERIZED SIMULATION; DENSITY; EQUATIONS OF STATE; GRAVITATIONAL WAVES; HYDRODYNAMICS; NEUTRON STARS; NUCLEAR MATTER; QUARK MATTER; RELATIVISTIC RANGE; SIGNALS; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- ENERGY RANGE; EQUATIONS; FLUID MECHANICS; MATTER; MECHANICS; PHYSICAL PROPERTIES; SIMULATION; STARS