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The Statistics of Nearly On-Axis Gravitational Lensing Events

  • Yun Wang
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 173)

Abstract

A small volume of space, nearly on-axis behind a gravitational lens with respect to a given source, will receive a greatly increased radiation flux. In the idealized case of a point mass lens acting on a point source in complete isolation, the volume will approach zero only as the flux tends to infinity; in fact, the volume weighted rms flux is divergent. In realistic cases, finite source size and the effects of other gravitational deflections (i.e., non-zero shear) limit the maximum flux and considerably complicate the physics, but very large fluxes are still produced in small volumes. We consider the physics and statistics of these Extreme Gravitational Lensing Events (EGLE) and present an initial examination of their possible astrophysical effects for various known and putative populations of lensing objects and sources, with particular attention to the case in which finite source size is important but shear is not.

Keywords

Gravitational Lens Tube Volume Angular Diameter Distance Finite Source Minimum Flux 
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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References

  1. Turner, E.L., 1980, ApJ, 242, L135ADSCrossRefGoogle Scholar
  2. Turner, E.L., Ostriker, J.P. & Gott, J.R., 1984, ApJ, 284, 1ADSCrossRefGoogle Scholar
  3. Wang, Y. & Turner, E.L., 1995, in preparationGoogle Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • Yun Wang
    • 1
  1. 1.NASA/Fermilab Astrophysics CenterFermi National Accelerator LaboratoryBataviaUSA

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