PIRSA:11020087 Scientific Series Strong Gravity

DOI10.48660/11020087

Series: Strong Gravity

Lyutikov, M. (2011). The Double Pulsar: testing GR in strong regime. Perimeter Institute. https://pirsa.org/11020087

Lyutikov, Maxim. The Double Pulsar: testing GR in strong regime. Perimeter Institute, Feb. 04, 2011, https://pirsa.org/11020087 

@misc{ pirsa_PIRSA:11020087,
  doi = {10.48660/11020087},
  url = {https://pirsa.org/11020087},
  author = {Lyutikov, Maxim},
  keywords = {Strong Gravity},
  language = {en},
  title = {The Double Pulsar: testing GR in strong regime},
  publisher = {Perimeter Institute},
  year = {2011},
  month = {feb},
  note = {PIRSA:11020087 see, \url{https://pirsa.org}}
}

Abstract

The long awaited discovery of the double radio pulsar system, PSR J0737-3039A/B, surpassed most expectations, both theoretical and observational, as a tool to probe general relativity, stellar evolution and pulsar theories. The Double Pulsar provides a unique and the most complete and clean test of theories of gravity in a regime sensitive to possible strong-gravitational self-field effects. All six post-Keplerian parameters have been measured (including the measurement of the relativistic spin precession), some parameters to a precision of 10^{-4}.

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