The Double Pulsar PSR J0737-3039
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The Double Pulsar (PSR J0737-3039) consists of two active radio pulsars (labeled as A and B) that are bound in a slightly eccentric, tight orbit. This is one of the best astrophysical laboratories to test Einstein’s theory of general relativity. All five post-Keplerian parameters are measured independently for the A and the B pulsars, and they are consistent with predictions from general relativity. The Double Pulsar is also useful for understanding the formation and the coalescence of double-neutron-star systems. We summarize the properties of the Double Pulsar and discuss their implications for testing general relativity and for detecting gravitational waves.
KeywordsPulsars Binary Gravitational Waves Ratio Observations
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- L. Blanchet, Living Rev. Relativity 17, no. 2 (2014) http://www.livingreviews.org/lrr-2014-2.Google Scholar
- J. Degallaix, et al. (Virgo Collaboration) in G. Auger, P. Binetruy and E. Plagnol, eds, 9th LISA Symposium Vol. 467 of Astronomical Society of the Pacific Conference Series, Advanced Virgo Status, 151 (2013).Google Scholar
- ATNF pulsar catalogue: www.atnf.csiro.au/people/pulsar/psrcat/.Google Scholar
- D. R. Lorimer, Living Rev. Relativity 11, no. 8 (2008) www.livingreviews.org/lrr-2008-8.Google Scholar
- I. H. Stairs, Living Rev. Relativity 6, no. 5 (2003) www.livingreviews.org/lrr-2003-5.Google Scholar
- N. Wex, to appear in the Brumberg Festschrift, edited by S. M. Kopeikein and to be published by de Gruyter, Berlin (2014) [arxiv.org/abs/1402.5594].Google Scholar
- M. A. McLaughlin, Private communication (2012).Google Scholar
- J. G. Williams, S. G. Turyshev and D. H. Boggs, Class. & Quantum Grav. 29, 18400 (2012).Google Scholar
- C. Kim, B. B. P. Perera and M. A. McLaughlin, submitted to Mon. Noc. Roy. Astron. Soc. http://jp.arxiv.org/abs/1308.4676.Google Scholar