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相关论文: Rethinking Lensing and Lambda

200 篇论文

By directly probing mass distributions, gravitational lensing offers several new tests of the CDM paradigm. Lens statistics place upper limits on the dark matter content of elliptical galaxies. Galaxies built from CDM mass distributions are…

天体物理学 · 物理学 2007-05-23 Charles R. Keeton

Upcoming ground and space based observatories such as the DES, the LSST, the JDEM concepts and the SKA, promise to dramatically increase the size of strong gravitational lens samples. A significant fraction of the systems are expected to be…

宇宙学与河外天体物理 · 物理学 2015-05-13 Benjamin M. Dobke , Lindsay J. King , Christopher D. Fassnacht , Matthew W. Auger

Over the past decade advancements in the understanding of several astrophysical phenomena have allowed us to infer a concordance cosmological model that successfully accounts for most of the observations of our universe. This has opened up…

宇宙学与河外天体物理 · 物理学 2011-12-13 Irène Balmès , Pier-Stefano Corasaniti

Propagation of light in the universe with structure which amplify and modify the shape of distant galaxies, producing a correlation between nearby and distant density of galaxies, is a phenomena very important in cosmology for determining…

星系天体物理 · 物理学 2014-09-05 Leonardo Castañeda

In this paper, we assemble a well-defined sample of early-type gravitational lenses extracted from a large collection of 158 systems, and use the redshift distribution of galactic-scale lenses to test the standard cosmological model…

宇宙学与河外天体物理 · 物理学 2019-02-20 Yu-Bo Ma , Shuo Cao , Jia Zhang , Shuaibo Geng , Yuting Liu , Tonghua Liu , Yu Pan

We investigate how observations of strong lensing can be used to infer cosmological parameters, in particular the equation of state of dark energy. We focus on the growth of the critical lines of lensing clusters with the source redshift as…

宇宙学与河外天体物理 · 物理学 2012-04-03 Britta Zieser , Matthias Bartelmann

We study moderate gravitational lensing where a background galaxy is magnified substantially, but not multiply imaged, by an intervening galaxy. We focus on the case where both the lens and source are elliptical galaxies. The signatures of…

宇宙学与河外天体物理 · 物理学 2015-06-03 S. Mao , J. Wang , M. C. Smith

We study the effects of strong lensing on the observed number counts of mm sources using a ray tracing simulation and two number count models of unlensed sources. We employ a quantitative treatment of maximum attainable magnification factor…

宇宙学与河外天体物理 · 物理学 2015-03-17 Yashar D. Hezaveh , Gilbert P. Holder

We study the impact of the often neglected lensing contribution to galaxy number counts on the $E_g$ statistics which is used to constrain deviations from GR. This contribution affects both the galaxy-galaxy and the convergence-galaxy…

宇宙学与河外天体物理 · 物理学 2016-10-10 Azadeh Moradinezhad Dizgah , Ruth Durrer

We use the statistics of strong gravitational lensing from the CLASS survey to impose constraints on the velocity dispersion and density profile of elliptical galaxies. This approach differs from much recent work, where the luminosity…

天体物理学 · 物理学 2009-11-07 Adam N. Davis , Dragan Huterer , Lawrence M. Krauss

A large number of cosmological studies now suggest that roughly two-thirds of the critical energy density of the Universe exists in a component with negative pressure. If the equation of state of such an energy component varies with time,…

天体物理学 · 物理学 2010-04-06 Asantha R. Cooray , Dragan Huterer

Strong gravitational lensing provides an independent measurement of the Hubble parameter ($H_0$). One remaining systematic is a bias from the additional mass due to a galaxy group at the lens redshift or along the sightline. We quantify…

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

The light we observe from distant astrophysical objects including supernovae and quasars allows us to determine large distances in terms of a cosmological model. Despite the success of the standard cosmological model in fitting the data,…

宇宙学与河外天体物理 · 物理学 2024-05-07 Angela L. H. Ng

We investigate observational constraints from lensing statistics and high-z type Ia supernovae on flat cosmological models with nonrelativistic matter and an exotic fluid with equation of state, $p_x=(m/3 -1)\rho_x$. We show that agreement…

天体物理学 · 物理学 2008-11-26 Ioav Waga , Ana Paula M. R. Miceli

Foreground galaxies that amplify the light from background quasars may also dim that light if the galaxies contain enough dust. Extinction by dust in lenses could hide the large number of lensed systems predicted for a flat universe with a…

天体物理学 · 物理学 2015-06-24 Sangeeta Malhotra , James E. Rhoads , Edwin L. Turner

An analysis of null geodesics in Schwarzschild de Sitter space is presented with special attention to their global `bending angles', local measurable angles, and the involvement of the cosmological constant. We make use of a general…

广义相对论与量子宇宙学 · 物理学 2016-09-19 Dmitri Lebedev , Kayll Lake

Several recent studies show that bright, intermediate and high redshift optically and radio selected QSOs are positively correlated with nearby galaxies on a range of angular scales up to a degree. Obscuration by unevenly distributed…

天体物理学 · 物理学 2009-10-31 Liliya L. R. Williams

The cosmological constant Lambda affects gravitational lensing phenomena. The contribution of Lambda to the observable angular positions of multiple images and to their amplification and time delay is here computed through a study in the…

天体物理学 · 物理学 2008-11-26 M. Sereno

Recent observations suggest appreciable star formation activity in early-type galaxies down to redshift $z\sim 0.5$. If so, there is likely to be dust in these galaxies. We consider the possibility that obscuration by dust can reconcile the…

天体物理学 · 物理学 2007-05-23 M. Fukugita , P. J. E. Peebles