Binary Neutron-Star Mergers with a Crossover Transition to Quark Matter
- University of Notre Dame, IN (United States)
- Sogang Univ. Seoul (Korea, Republic of)
- University of Notre Dame, IN (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
This paper summarizes recent work on the possible gravitational-wave signal from binary neutron-star mergers in which there is a crossover transition to quark matter. Although this is a small piece of a much more complicated problem, we discuss how the power spectral density function may reveal the presence of a crossover transition to quark matter.
- Research Organization:
- Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Grant/Contract Number:
- AC05-00OR22725; FG02-95ER40934; FG02-95-ER40934
- OSTI ID:
- 1998816
- Alternate ID(s):
- OSTI ID: 2000331
- Journal Information:
- Universe, Vol. 9, Issue 9; ISSN 2218-1997
- Publisher:
- MDPICopyright Statement
- Country of Publication:
- United States
- Language:
- English
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