Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects

The combined observation of gravitational and electromagnetic waves from the coalescence of two neutron stars marks the beginning of multimessenger astronomy with gravitational waves (GWs). The development of accurate gravitational waveform models is a crucial prerequisite to extract information abo...

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Veröffentlicht in:	Physical review. D 2019-01, Vol.99 (2), p.024029, Article 024029
Hauptverfasser:	Dietrich, Tim, Khan, Sebastian, Dudi, Reetika, Kapadia, Shasvath J., Kumar, Prayush, Nagar, Alessandro, Ohme, Frank, Pannarale, Francesco, Samajdar, Anuradha, Bernuzzi, Sebastiano, Carullo, Gregorio, Del Pozzo, Walter, Haney, Maria, Markakis, Charalampos, Pürrer, Michael, Riemenschneider, Gunnar, Setyawati, Yoshinta Eka, Tsang, Ka Wa, Van Den Broeck, Chris
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Astronomical models Astronomy Astrophysics Binary stars Black holes Coalescing Electromagnetic radiation Frequency ranges General Relativity and Quantum Cosmology Gravitation Gravitational waves Neutron stars Neutrons Numerical relativity Physics Relativity Stellar systems Tidal effects Waveforms
Online-Zugang:	Volltext
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