Neutron stars and black holes are the astrophysical systems with the strongest gravitational fields in the universe. In this article, I review the prospect of using observations of such compact objects to probe some of the most intriguing general relativistic predictions in the strong-field regime: the absence of stable circular orbits near a compact object and the presence of event horizons around black-hole singularities. I discuss the need for a theoretical framework, within which future experiments will provide detailed, quantitative tests of gravity theories. Finally, I summarize the constraints imposed by current observations of neutron stars on potential deviations from general relativity.
Keywords: Neutron stars, Black holes, Tests of relativistic gravity
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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:
Dimitrios Psaltis,
"Probes and Tests of Strong-Field Gravity with Observations in the Electromagnetic Spectrum",
Living Rev. Relativity 11, (2008), 9. URL (cited on <date>):
http://www.livingreviews.org/lrr-2008-9
ORIGINAL | http://www.livingreviews.org/lrr-2008-9 |
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Title | Probes and Tests of Strong-Field Gravity with Observations in the Electromagnetic Spectrum |
Author | Dimitrios Psaltis |
Date | accepted 1 July 2008, published 18 November 2008 |