Deflection of light and particles by moving gravitational lenses

Phys. Rev. D 69 (2004) 063001

DOI: 10.1103/PhysRevD.69.063001 (http) or 10.1103/PhysRevD.69.063001 (doi)
ADS bibcode 2004PhRvD..69f3001W
astro-ph/0401362

Olaf Wucknitz [1], Ulrich Sperhake [2]

  1. Universität Potsdam, Institut für Physik, Am Neuen Palais 10, D-14469 Potsdam, Germany
  2. Penn State University, Centers for Gravitational Physics & Geometry and for Gravitational Wave Physics, University Park, PA 16802, USA

Abstract

Various authors have investigated the problem of light deflection by radially moving gravitational lenses, but the results presented so far do not appear to agree on the expected deflection angles. Some publications claim a scaling of deflection angles with 1-v to first order in the radial lens velocity v, while others obtained a scaling with 1-2v. In this paper we generalize the calculations for arbitrary lens velocities and show that the first result is the correct one.

We discuss a seeming inconsistency of relativistic light deflection with the classical picture of moving test particles by generalizing the lens effect to test particles of arbitrary velocity, including light as a limiting case. We show that the effect of radial motion of the lens is very different for slowly moving test particles and light and that a critical test particle velocity exists for which motion of the lens has no effect on the deflection angle to first order. An interesting and not immediately intuitive result is obtained in the limit of a highly relativistic motion of the lens towards the observer, where the deflection angle of light reduces to zero. This phenomenon is elucidated in terms of moving refractive media. Furthermore we discuss the dragging of inertial frames in the field of a moving lens and the corresponding Lense-Thirring precession, in order to shed more light on the geometrical effects in the surroundings of a moving mass.

In a second part we discuss the effect of transversal motion on the observed redshift of lensed sources. We demonstrate how a simple kinematic calculation explains the effects for arbitrary velocities of the lens and the test particles. Additionally we include transversal motion of the source and observer to show that all three velocities can be combined into an effective relative transversal velocity similar to the approach used in microlensing studies.

Key words: PACS 95.30.Sf, 04.20.Cv, 04.25.Nx, 98.62.Sb

The first and second version are still available.
A summary of this paper was presented in a conference talk and (slightly more condensed) in a workshop talk.
Another paper on the subject was submitted later.



Phys. Rev. D 69 (2004) 063001 (link to online journal)
DOI (Digital Object Identifier): 10.1103/PhysRevD.69.063001 (http) or 10.1103/PhysRevD.69.063001 (doi)
ADS bibcode 2004PhRvD..69f3001W (link to ADS entry)
astro-ph/0401362 (link to e-print archive)



download full article, PRD version
PDF file (126.3 kB, last change 15 Mar 2004)
Letter paper, 13 pages. Published version.

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gzipped postscript file (163.3 kB, last change 19 Jan 2004)
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PDF file (335.9 kB, last change 19 Jan 2004)
Letter paper, 13 pages. PDF version with crosslinks.



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