Binary Neutron-Star Mergers with a Crossover Transition to Quark Matter

Grant J. Mathews, Atul Kedia, Hee Il Kim, In Saeng Suh

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Article number410
JournalUniverse
Volume9
Issue number9
DOIs
StatePublished - Sep 2023

Funding

H.I.K. graciously thanks Jinho Kim and Chunglee Kim for continuous support. This manuscript has in part been authored by UT-Battelle, LLC under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy. The publisher, by accepting the article for publication, acknowledges that the U.S. Government retains a non-exclusive, paid up, irrevocable, world-wide license to publish or reproduce the published form of the manuscript, or allow others to do so, for U.S. Government purposes. Software used was as follows The Einstein Toolkit (Ref. []; https://einsteintoolkit.org , accessed on 28 August 2023), LORENE (Refs. [,]), PyCactus ( https://bitbucket.org/GravityPR/pycactus , accessed on 28 August 2023), and TOVsolver ( https://github.com/amotornenko/TOVsolver , accessed on 28 August 2023). Work at the Center for Astrophysics of the University of Notre Dame is supported by the U.S. Department of Energy under Nuclear Theory Grant No. DE-FG02-95-ER40934. This research was supported in part by the Notre Dame Center for Research Computing through the high performance computing resources. The work of H.I.K. was supported by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education through the Center for Quantum Spacetime (CQUeST) of Sogang University (Grant No. NRF-2020R1A6A1A03047877). This research used resources of the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725.

FundersFunder number
CQUeST
Center for Quantum Spacetime
Notre Dame Center for Research Computing
U.S. Department of EnergyDE-FG02-95-ER40934
Office of ScienceDE-AC05-00OR22725
Sogang UniversityNRF-2020R1A6A1A03047877
Ministry of Education
National Research Foundation of Korea

    Keywords

    • equation of state
    • gravitational waves
    • neutron stars
    • quark matter

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