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Gravitational Lensing in Compact Binary Systems

  • David W. Hobill
  • John Kollar
  • Julia Pulwicki
Part of the Astrophysics and Space Science Library book series (ASSL, volume 352)

The theory of microlensing is modified for sources producing pulsed, directional light beams in order to analyze the changes in pulse profiles that arise due to time delays and magnification factors occurring as a result of gravitational lensing by other compact objects. The results are applied to the double pulsar PSR J0737-3039 to determine whether or not anomalous enhancements observed during the eclipse of pulsar A by pulsar B have the signature of gravitational lensing. Predictions regarding the eclipse of pulsar B by pulsar A are also provided.

Keywords

Black Hole Neutron Star Inclination Angle Light Curve Pulsar Source 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media B.V 2008

Authors and Affiliations

  • David W. Hobill
    • 1
  • John Kollar
    • 1
  • Julia Pulwicki
    • 1
  1. 1.Department of Physics and AstronomyUniversity of CalgaryCalgaryCanada

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