A Possible Manifestation of Microlensing in Pulsar Timing

  • T. I. Larchenkova
  • O. V. Doroshenko
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 173)

Abstract

Gravitational lensing and the time delay of a pulsar signal in the gravitational field of a mass are General Relativistic effects that may be used as a tool to detect the observational parameters of dark matter in our Galaxy. We propose to use observations of the time delay of pulses from pulsars to detect lensing objects located close to the line of the sight, to study the distribution of dark matter in our Galaxy. We discuss the possibility of finding such an event by measuring the delay of pulses from a pulsar, and apply it to data for PSR B0525+21.

Keywords

Dark Matter Gravitational Field Pulsar Signal Pulsar Velocity Observational Parameter 
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.

References

  1. Doroshenko, O.V. & Kopeikin, S.M., 1990, SvA, 34(5), 496ADSGoogle Scholar
  2. Downs, G.S. & Reichley, P.E., 1983, ApJS, 53, 169ADSCrossRefGoogle Scholar
  3. Downs, G.S. & Krause-PolstrofF, J., 1986, ApJS, 62, 81ADSCrossRefGoogle Scholar
  4. Moore, B. & Silk, J., 1995, ApJL, 442, L5ADSGoogle Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • T. I. Larchenkova
    • 1
  • O. V. Doroshenko
    • 1
  1. 1.Astro Space Center of P.N. Lebedev Physical InstituteMoscowRussia

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