Journal
INTERNATIONAL JOURNAL OF MODERN PHYSICS E
Volume 29, Issue 7, Pages -Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S0218301320300076
Keywords
Neutron star equation of state; dense nuclear matter; low-mass X-ray binaries; gravitational waves
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Funding
- National Research Foundation of Korea (NRF) [NRF-2016R1A5A1013277, NRF-2018R1D1A1B07048599, NRF-2019R1C1C1010571, NRF-2017R1D1A1B03029020, NRF-2018R1A5A1025563]
- Max Planck Society
- Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) [279384907 - SFB 1245]
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This paper reviews the properties of neutron stars based on the recent multi-messenger observations including electromagnetic waves from the low-mass X-ray binaries and gravitational waves from the merger of neutron star binaries. Based on these observations, we investigate theoretical models for dense nuclear matter and discuss their implications to the neutron star observations such as mass, radius, cooling, and tidal deformability. We also discuss the uncertainties in the neutron star cooling, neutron star properties with Bayesian approaches, and an expansion scheme applied to the nuclear energy density functional theory.
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