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Phys. Rev. D 74, 024020 (2006) [13 pages]

Gravitational lensing by wormholes

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Kamal K. Nandi1,3,4,*, Yuan-Zhong Zhang2,3,†, and Alexander V. Zakharov4,‡
1Department of Mathematics, University of North Bengal, Darjeeling (West Bengal) 743 430, India
2CCAST (World Laboratory), P.O. Box 8730, Beijing 100080, Beijing, China
3Institute of Theoretical Physics, Chinese Academy of Sciences, P.O. Box 2735, Beijing 100080, Beijing, China
4Joint Research Center for Mathematics and Physics (JRCMP), Bashkir State Pedagogical University, 3-A, October Revolution Street, Ufa 450000, Russia

Received 17 February 2006; published 20 July 2006

Gravitational lensing by traversable Lorentzian wormholes is a new possibility which is analyzed here in the strong field limit. Wormhole solutions are considered in the Einstein minimally coupled theory and in the brane world model. The observables in both the theories show significant differences from those arising in the Schwarzschild black hole lensing. As a corollary, it follows that wormholes with zero Keplerian mass exhibit lensing properties which are qualitatively (though not quantitatively) the same as those of a Schwarzschild black hole. Some special features of the considered solutions are pointed out.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.74.024020
DOI:
10.1103/PhysRevD.74.024020
PACS:
04.50.+h, 04.70.Bw, 95.30.Sf, 98.62.Sb

*Email: kamalnandi1952@yahoo.co.in

Email: yzhang@itp.ac.cn

Email: zakharov@bspu.ru