Kerr-Sen dilaton-axion black hole lensing in the strong deflection limit

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dc.creatorGyulchev, Galin N.
dc.creatorYazadjiev, Stoytcho S.
dc.date2006-11-21
dc.date2007-03-29
dc.date.accessioned2026-07-07T11:21:32Z
dc.date.available2026-07-07T11:21:32Z
dc.descriptionIn the present work we study numerically quasi-equatorial lensing by the charged, stationary, axially-symmetric Kerr-Sen dilaton-axion black hole in the strong deflection limit. In this approximation we compute the magnification and the positions of the relativistic images. The most outstanding effect is that the Kerr-Sen black hole caustics drift away from the optical axis and shift in clockwise direction with respect to the Kerr caustics. The intersections of the critical curves on the equatorial plane as a function of the black hole angular momentum are found, and it is shown that they decrease with the increase of the parameter $Q^{2}/M$. All of the lensing quantities are compared to particular cases as Schwarzschild, Kerr and Gibbons-Maeda black holes.
dc.description31 pages, 17 figures; V2 references added, some typos corrected, V3 references added, language corrections, V4 table added, minor technical corrections
dc.identifierhttps://arxiv.org/abs/gr-qc/0611110
dc.identifierhttp://arxiv.org/abs/gr-qc/0611110
dc.identifierPhys.Rev.D75:023006,2007
dc.identifierdoi:10.1103/PhysRevD.75.023006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194291
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleKerr-Sen dilaton-axion black hole lensing in the strong deflection limit
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