We review the tests of general relativity that will become possible with space-based gravitational-wave detectors operating in the ∼ 10^{-5} – 1 Hz low-frequency band. The fundamental aspects of gravitation that can be tested include the presence of additional gravitational fields other than the metric; the number and tensorial nature of gravitational-wave polarization states; the velocity of propagation of gravitational waves; the binding energy and gravitational-wave radiation of binaries, and therefore the time evolution of binary inspirals; the strength and shape of the waves emitted from binary mergers and ringdowns; the true nature of astrophysical black holes; and much more. The strength of this science alone calls for the swift implementation of a space-based detector; the remarkable richness of astrophysics, astronomy, and cosmology in the low-frequency gravitational-wave band make the case even stronger.
Keywords: gravitation, black holes, LISA, gravitational waves, eLISA, general relativity, data analysis
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Since a Living Reviews in Relativity article may evolve over time, please cite the access <date>, which uniquely identifies the version of the article you are referring to:
Jonathan R. Gair and Michele Vallisneri and Shane L. Larson and John G. Baker,
"Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors",
Living Rev. Relativity 16, (2013), 7. URL (cited on <date>):
http://www.livingreviews.org/lrr-2013-7
ORIGINAL | http://www.livingreviews.org/lrr-2013-7 |
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Title | Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors |
Author | Jonathan R. Gair / Michele Vallisneri / Shane L. Larson / John G. Baker |
Date | accepted 19 August 2013, published 12 September 2013 |