Constraints on the neutron star’s maximum densities from postmerger gravitational-waves with third-generation observations
@inproceedings{Breschi2021ConstraintsOT, title={Constraints on the neutron star’s maximum densities from postmerger gravitational-waves with third-generation observations}, author={Matteo Breschi and Sebastiano Bernuzzi and Daniel A. Godzieba and Albino Perego and Davide Radice}, year={2021} }
Matteo Breschi, Sebastiano Bernuzzi, Daniel Godzieba, Albino Perego, and David Radice Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, 07743, Jena, Germany Department of Physics, The Pennsylvania State University, University Park, PA 16802, USA Dipartimento di Fisica, Università di Trento, Via Sommarive 14, 38123 Trento, Italy INFN-TIFPA, Trento Institute for Fundamental Physics and Applications, via Sommarive 14, I-38123 Trento, Italy Institute for Gravitation & the…
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3 Citations
Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
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Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
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The merger of two compact objects of which at least one is a neutron star is signalled by transient electromagnetic emission in a kilonova. This event is accompanied by gravitational waves and…
Snowmass2021 Cosmic Frontier White Paper: Numerical relativity for next-generation gravitational-wave probes of fundamental physics
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The next generation of gravitational-wave detectors, conceived to begin operations in the 2030s, will probe fundamental physics with exquisite sensitivity. These observations will measure the…
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