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Neutron Star Mergers and the Quark Matter Equation of State
- Source :
- EPJ Web of Conferences, Vol 274, p 01013 (2022)
- Publication Year :
- 2022
- Publisher :
- EDP Sciences, 2022.
-
Abstract
- As neutron stars merge they can approach very high nuclear density. Here, we summarized recent results for the evolution and gravitational wave emission from binary-neutron star mergers using a a variety of nuclear equations of state with and without a crossover transition to quark matter. We discuss how the late time gravitational wave emission from binary neutron star mergers may possibly reveal the existence of a crossover transition to quark matter.
Details
- Language :
- English
- ISSN :
- 2100014X
- Volume :
- 274
- Database :
- Directory of Open Access Journals
- Journal :
- EPJ Web of Conferences
- Publication Type :
- Academic Journal
- Accession number :
- edsdoj.41f4840436df41b788691e63e1e72e8a
- Document Type :
- article
- Full Text :
- https://doi.org/10.1051/epjconf/202227401013