Probing neutron star structure via f -mode oscillations and damping in dynamical spacetime models

Gravitational wave and electromagnetic observations can provide new insights into the nature of matter at supranuclear densities inside neutron stars. Improvements in electromagnetic and gravitational wave sensing instruments continue to enhance the accuracy with which they can measure the masses, r...

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Veröffentlicht in:	Physical review. D 2019-04, Vol.99 (8), p.1, Article 084024
Hauptverfasser:	Rosofsky, Shawn G., Gold, Roman, Chirenti, Cecilia, Huerta, E. A., Miller, M. Coleman
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Binary stars Computer simulation Damping Deformation Eccentric orbits Equations of state Formability Gravitation theory Gravitational waves Mathematical models Neutron stars Neutrons Numerical relativity Oscillations Perturbation theory Relativity Stars Theory of relativity Time dependence
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