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Equation of state (EOS) insensitive relations, so-called universal relations, between the neutron star (NS) compactness, its multipolar tidal deformability coefficients, and between the tidal parameters for binary systems are essential to break degeneracies in gravitational wave data analysis.
1903
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C. E. Rhoades, Jr. and R. Ruffini, Maximum mass of a neutron star, Phys. Rev. Lett. 32
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F. Douchin and P. Haensel, A unified equation of state of dense matter and neutron star structure, Astron. Astrophys. 380
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T. Damour and A. Nagar, Relativistic tidal properties of neutron stars, Phys. Rev. D 80
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K. Yagi and N. Yunes, Binary Love Relations, Class. Quant. Grav. 33
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2010
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J. M. Lattimer, The nuclear equation of state and neutron star masses, Ann. Rev. Nucl. Part. Sci. 62
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2018
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2018
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K. Yagi, Multipole Love Relations, Phys. Rev. D 89
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J. S. Speagle, dynesty: a dynamic nested sampling package for estimating Bayesian posteriors and evidences, Monthly Notices of the Royal Astronomical Society 493
2020
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