| Issue |
EPJ Web Conf.
Volume 274, 2022
XVth Quark Confinement and the Hadron Spectrum Conference (ConfXV)
|
|
|---|---|---|
| Article Number | 01013 | |
| Number of page(s) | 10 | |
| Section | 1 - Plenary Presentations | |
| DOI | https://doi.org/10.1051/epjconf/202227401013 | |
| Published online | 22 December 2022 | |
https://doi.org/10.1051/epjconf/202227401013
Neutron Star Mergers and the Quark Matter Equation of State
1 Department of Physics and Astronomy, Center for Astrophysics, University of Notre Dame, Notre Dame, IN 46556, USA
2 Center for Quantum Spacetime, Sogang University, Seoul 04107, Korea
3 Center for Research Computing, University of Notre Dame, Notre Dame, IN 46556, USA
* e-mail: gmathews@nd.edu
† e-mail: atulkedia93@gmail.com
‡ e-mail: khizetta@sogang.ac.kr
§ e-mail: isuh@nd.edu
Published online: 22 December 2022
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.
© The Authors, published by EDP Sciences, 2022
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