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Extensive analyses of statistical strong gravitational lensing are performed based on the final Cosmic Lens All Sky Survey (CLASS) well-defined statistical sample of flat spectrum radio sources and current estimates of galaxy luminosity…

天体物理学 · 物理学 2009-11-07 Kyu-Hyun Chae

Light rays from a multiply imaged quasar usually sample different path lengths across the deflector. Extinction in the lensing galaxy may thus lead to a differential obscuration and reddening between the observed macro-lensed QSO images.…

天体物理学 · 物理学 2007-05-23 C. Jean , J. Surdej

The mass derived from gravitational lensing reflects the total mass contained in the lensing system, independent of the specific matter contents and states. A comparison of the dynamical masses from hydrostatic equilibrium with the…

天体物理学 · 物理学 2009-10-22 Xiang-Ping Wu

The combination of deep exposures and high resolution offered by telescopes in space allows the detection of lensing over a wide range of source redshifts and lens masses. As an example, we model a lens candidate found in the southern…

天体物理学 · 物理学 2007-05-23 Rennan Barkana , David Hogg , Abraham Loeb , Roger Blandford

We present new results on the gravitational lensing shear and magnification power spectra obtained from numerical simulations of a flat cosmology with a cosmological constant. These results are of considerable interest since both the shear…

天体物理学 · 物理学 2009-11-07 Andrew J. Barber , A. N. Taylor

We consider the nonunitary quantum dynamics of neutral massless scalar particles used to model photons around a massive gravitational lens. The gravitational interaction between the lensing mass and asymptotically free particles is…

广义相对论与量子宇宙学 · 物理学 2018-10-09 Charles H. -T. Wang , Elliott Mansfield , Teodora Oniga

I describe a new approach (developed in collaboration with D.E. Holz) to calculating the statistical distributions for magnification, shear, and rotation of images of cosmological sources due to gravitational lensing by mass inhomogeneities…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Robert M. Wald

We describe the feasibility of detecting the gravitational deflection of light emitted by stars moving under the influence of the massive object at the Galactic center. Light emitted by a star orbiting behind the central mass has a smaller…

天体物理学 · 物理学 2009-11-10 Adi Nusser , Tom Broadhurst

This paper reviews the measurements of galaxy correlations at high redshifts, and discusses how these may be understood in models of hierarchical gravitational collapse. The clustering of galaxies at redshift one is much weaker than at…

天体物理学 · 物理学 2009-10-30 J. A. Peacock

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

We present near infrared observations of the red gravitational lens system MG0414+0534. Our images are of sufficient quality to allow photometry of all four QSO images and the lens galaxy. The observations show that the K-band brightnesses…

天体物理学 · 物理学 2009-10-30 B. A. McLeod , G. M. Bernstein , M. J. Rieke , D. W. Weedman

We study gravitational lensing by clusters of galaxies in the context of the generic class of unconventional gravity theories of the scalar--tensor type. For positive energy scalar fields with any dynamics, the bending of light by a weakly…

天体物理学 · 物理学 2010-11-01 Jacob D. Bekenstein , Robert H. Sanders

LISA might detect gravitational waves from mergers of massive black hole binaries strongly lensed by intervening galaxies (Sereno et al. 2010). The detection of multiple gravitational lensing events would provide a new tool for cosmography.…

宇宙学与河外天体物理 · 物理学 2015-05-27 M. Sereno , Ph. Jetzer , A. Sesana , M. Volonteri

We calculate the expected number of multiply-imaged galaxies in the Hubble Deep Field (HDF), using photometric redshift information for galaxies with m_I < 27 that were detected in all four HDF passbands. A comparison of these expectations…

天体物理学 · 物理学 2009-10-31 Asantha R. Cooray , Jean M. Quashnock , M. Coleman Miller

Hydrodynamic cosmological simulations predict that the average opacity of the Ly-alpha forest should increase in the neighborhood of galaxies because galaxies form in dense environments. Recent observations (Adelberger et al. 2002) confirm…

天体物理学 · 物理学 2009-11-07 Juna A. Kollmeier , David H. Weinberg , Romeel Dave' , Neal Katz

The probability that high-redshift sources are gravitationally-lensed with large image separations (i.e., greater than can be produced by galactic deflectors) is determined by the cosmological population of group- and cluster-sized halos.…

天体物理学 · 物理学 2007-05-23 Daniel J. Mortlock

The deflection and gravitational lensing of light and massive particles in arbitrary static, spherically symmetric and asymptotically (anti-)de Sitter spacetimes are considered in this work. We first proved that for spacetimes whose metric…

广义相对论与量子宇宙学 · 物理学 2021-10-13 Zixiao Li , Haotian Liu , Junji Jia

We explore the possibility that the entire departure of galactic rotational velocities from their luminous Newtonian expectation be cosmological in origin, and show that within the framework of conformal gravity (but not Einstein gravity…

天体物理学 · 物理学 2016-08-30 Philip D. Mannheim

We report the possible discovery of multiple gravitationally-lensed images of QSOs with angular separations on arcminute scales. The QSOs were selected from the completed 2dF QSO survey as having redshifts and optical colours which are…

天体物理学 · 物理学 2011-03-10 L. Miller , A. M. Lopes , R. J. Smith , S. M. Croom , B. J. Boyle , T. Shanks , P. Outram

Strong gravitational lenses come in many forms, but are typically divided into two populations: galaxies, and groups and clusters of galaxies. The largest objects in the Universe (i.e. galaxy clusters) are highly irregular and composed of…

宇宙学与河外天体物理 · 物理学 2025-10-17 Luka Vujeva , Jose María Ezquiaga , Rico K. L. Lo , Juno C. L. Chan