Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-28T08:39:04.292Z Has data issue: false hasContentIssue false

The Statistics Of Nearly On-Axis Gravitational Lensing Events

Published online by Cambridge University Press:  25 May 2016

Yun Wang*
Affiliation:
NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510-0500

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Chapter 10: Emerging Applications
Copyright
Copyright © Kluwer 1996 

References

Turner, E.L., 1980, ApJ, 242, L135 Google Scholar
Turner, E.L., Ostriker, J.P. & Gott, J.R., 1984, ApJ, 284, 1 Google Scholar
Wang, Y. & Turner, E.L., 1995, in preparation Google Scholar