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We discuss strong gravitational lensing by multiple objects along any line of sight. The probability for strong gravitational lensing by more than one lens is small, but a number of strong lens systems in which more than one separate lens…

天体物理学 · 物理学 2009-11-06 Ole Moeller , A. W. Blain

The strange morphology of the six-component gravitational lens PMN J0134-0931 has resisted explanation. We present the first successful quantitative models for the system, based on the idea that there are two lens galaxies and two…

天体物理学 · 物理学 2008-11-26 Charles R. Keeton , Joshua N. Winn

We demonstrate that for several of the gravitational lens models used to describe galaxies, there exists a quantity we dub the magnification invariant, equaling the sum of the signed magnifications of the images, that is a constant when the…

天体物理学 · 物理学 2009-10-30 N. Dalal

Among known strongly lensed quasar systems, ~25% have gravitational potentials sufficiently flat (and sources sufficiently well aligned) to produce four images rather than two. The projected flattening of the lensing galaxy and tides from…

星系天体物理 · 物理学 2021-06-30 Richard Luhtaru , Paul L. Schechter , Kaylee M. de Soto

We simulate the effects of gravitational lensing on the source count of high redshift galaxies as projected to be observed by the Hubble Frontier Fields program and the James Webb Space Telescope (JWST) in the near future. Taking the mass…

宇宙学与河外天体物理 · 物理学 2015-06-16 Natalie Mashian , Abraham Loeb

A number of recent surveys for gravitational lenses have found examples of double Einstein rings. Here, we investigate analytically the occurrence of multiple Einstein rings. We prove, under very general assumptions, that at most one…

天体物理学 · 物理学 2009-11-13 M. C. Werner , J. An , N. W. Evans

Of order one in 10^3 quasars and high-redshift galaxies appears in the sky as multiple images as a result of gravitational lensing by unrelated galaxies and clusters that happen to be in the foreground. While the basic phenomenon is a…

宇宙学与河外天体物理 · 物理学 2024-01-10 Prasenjit Saha , Dominique Sluse , Jenny Wagner , Liliya L. R. Williams

Dark matter caustics have specific density profiles and, therefore, precisely calculable gravitational lensing properties. We present a formalism which simplifies the relevant calculations, and apply it to four specific cases. In the first…

天体物理学 · 物理学 2009-11-07 C. Charmousis , V. Onemli , Z. Qiu , P. Sikivie

A galaxy can act as a gravitational lens, producing multiple images of a background object. Theory predicts there should be an odd number of images but, paradoxically, almost all observed lenses have 2 or 4 images. The missing image should…

天体物理学 · 物理学 2015-06-24 Joshua N. Winn , David Rusin , Christopher S. Kochanek

A complete manual search has been carried out of the list of 285423 objects, nearly all of them galaxies, identified in the COSMOS field that are brighter than I=25. Two certain and one highly probable new gravitational lenses are found, in…

天体物理学 · 物理学 2009-11-13 Neal Jackson

When a gravitationally lensed source crosses a caustic, a pair of images is created or destroyed. We calculate the mean number of such pairs of micro-images $<n>$ for a given macro-image of a gravitationally lensed point source, due to…

天体物理学 · 物理学 2016-08-30 Jonathan Granot , Paul L. Schechter , Joachim Wambsganss

The transparent Sun is modeled as a spherically symmetric and centrally condensed gravitational lens using recent Standard Solar Model (SSM) data. The Sun's minimum focal length is computed to a refined accuracy of 23.5 +/- 0.1 AU, just…

天体物理学 · 物理学 2011-12-13 Bijunath Patla , Robert J. Nemiroff

In this work are reviewed several aspects of gravitational lensing produced by astrophysical bodies that strongly curve the spacetime in their vicinity. When an object with a photon sphere (e.g. a black hole) is interposed between a source…

广义相对论与量子宇宙学 · 物理学 2014-09-15 Ernesto F. Eiroa

The mathematical theory of gravitational lensing has revealed many generic and global properties. Beginning with multiple imaging, we review Morse-theoretic image counting formulas and lower bound results, and complex-algebraic upper bounds…

星系天体物理 · 物理学 2014-11-20 A. O. Petters , M. C. Werner

Gravitational lensing is the phenomenon arising when light rays are deflected by the mass between the source and the observer. Largely magnified and highly distorted images of background galaxies are formed by these angular deflections if…

宇宙学与河外天体物理 · 物理学 2025-07-02 Atınç Çağan Şengül

Gravitational waves act like lenses for the light propagating through them. This phenomenon is described using the vector formalism employed for ordinary gravitational lenses, which was proved to be applicable also to a non-stationary…

天体物理学 · 物理学 2014-10-13 Valerio Faraoni

We investigate imaging point sources with a monopole gravitational lens, such as the Solar Gravitational Lens in the geometric optics limit. We compute the light amplification of the lens used in conjunction with a telescope featuring a…

天体物理仪器与方法 · 物理学 2023-11-08 Viktor T. Toth

The total magnification due to a point lens has been of particular interest as the theorem that gravitational lensing results in light amplification for all observers appears to contradict the conservation of photon number. This has been…

天体物理仪器与方法 · 物理学 2015-10-20 S. J. Walters , L. K. Forbes

We discuss boson stars as possible gravitational lenses and study the lensing effect by these objects made of scalar particles. The mass and the size of a boson star may vary from an individual Newtonian object similar to the Sun to the…

天体物理学 · 物理学 2009-10-30 Mariusz P. Dabrowski , Franz E. Schunck

If an extended source, such as a galaxy, is gravitationally lensed by a massive object in the foreground, the lensing distorts the observed image. It is straightforward to simulate what the observed image would be for a particular lens and…

天体物理学 · 物理学 2009-11-13 Brendon J. Brewer , Geraint F. Lewis