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Zeitschriftenartikel

Gravitational waves from neutron stars: Promises and challenges

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20661

Krishnan,  B.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4291

Read,  J.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons20670

Rezzolla,  L.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Externe Ressourcen
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Volltexte (frei zugänglich)

0912.0384
(Preprint), 2MB

GRG43_409.pdf
(beliebiger Volltext), 796KB

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Zitation

Andersson, N., Ferrari, V., Jones, D. I., Kokkotas, K. D., Krishnan, B., Read, J., et al. (2011). Gravitational waves from neutron stars: Promises and challenges. General Relativity and Gravitation, 43(2), 409-436. doi:10.1007/s10714-010-1059-4.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0012-9E08-0
Zusammenfassung
We discuss different ways that neutron stars can generate gravitational waves, describe recent improvements in modelling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to test our understanding of fundamental physics. The main purpose of the discussion is to establish promising science goals for third-generation ground-based detectors, like the Einstein Telescope, and identify the various challenges that need to be met if we want to use gravitational-wave data to probe neutron star physics.