A comparison of methods for the detection of gravitational waves from unknown neutron stars

Rapidly rotating neutron stars are promising sources of continuous gravitational wave radiation for the LIGO and Virgo interferometers. The majority of neutron stars in our galaxy have not been identified with electromagnetic observations. All-sky searches for isolated neutron stars offer the potent...

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Veröffentlicht in:	arXiv.org 2016-06
Hauptverfasser:	Walsh, Sinead, Pitkin, Matthew, Oliver, Miquel, D'Antonio, Sabrina, Dergachev, Vladimir, Krolak, Andrzej, Astone, Pia, Bejger, Michal, Matteo Di Giovanni, Dorosh, Orest, Frasca, Sergio, Leaci, Paola, Mastrogiovanni, Simone, Miller, Andrew, Palomba, Cristiano, Papa, Maria Alessandra, Piccinni, Ornella J, Riles, Keith, Sauter, Orion, Sintes, Alicia M
Format:	Artikel
Sprache:	eng
Schlagworte:	Computation Computer simulation Gravitation Gravitational waves Interferometers Methods Milky Way Neutron stars Neutrons Parameter estimation Physics - General Relativity and Quantum Cosmology Physics - Instrumentation and Methods for Astrophysics Search methods Sensitivity Stars Stellar rotation
Online-Zugang:	Volltext
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