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Tidal forces cause inspiralling binary neutron stars to deform, leaving a measurable imprint on the gravitational waves they emit.
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2013
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Andrea Maselli, Leonardo Gualtieri, and Valeria Ferrari, “Constraining the equation of state of nuclear matter with gravitational wave observations: Tidal deformability and tidal disruption,” Phys. Rev. D 88
2013
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2013
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Luc Blanchet, “Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries,” Living Reviews in Relativity 17
2014
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Marc Favata, “Systematic Parameter Errors in Inspiraling Neutron Star Binaries,” Phys. Rev. Lett. 112
2014
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2014
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K. Yagi, “Multipole Love relations,” Phys. Rev. D 89
2014
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2017
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Kent Yagi, “Erratum: Multipole love relations [phys. rev. d 89, 043011 (2014)],” Phys. Rev. D 96
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2018
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2018
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2018
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Jérémie Gagnon-Bischoff, Stephen R. Green, Philippe Landry, and Néstor Ortiz, “Extended I-Love relations for slowly rotating neutron stars,” Phys. Rev. D 97
2018
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2018
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David Radice, Albino Perego, Francesco Zappa, and Sebastiano Bernuzzi, “GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations,” Astrophys. J. 852
2041
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Carolyn A. Raithel, Feryal Özel, and Dimitrios Psaltis, “Tidal Deformability from GW170817 as a Direct Probe of the Neutron Star Radius,” Astrophys. J. 857
2041
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