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Most of the matter in the universe is not luminous and can be observed directly only through its gravitational effect. An emerging technique called weak gravitational lensing uses background galaxies to reveal the foreground dark matter…

天体物理学 · 物理学 2017-05-10 David M. Wittman , J. Anthony Tyson , David Kirkman , Ian Dell'Antonio , Gary Bernstein

In light of the surge in popularity of electromagnetic cloaking devices, we consider whether it is possible to use gravitational lensing to cloak a volume of spacetime. A metric for such a spacetime geometry is presented, and its geometric…

广义相对论与量子宇宙学 · 物理学 2012-10-30 Benjamin K. Tippett

Despite much interest and progress in optical spatial cloaking, a three-dimensional (3D), transmitting, continuously multidirectional cloak in the visible regime has not yet been demonstrated. Here we experimentally demonstrate such a cloak…

光学 · 物理学 2015-03-10 Joseph S. Choi , John C. Howell

In the cold dark matter scenario, dark matter halos are assembled hierarchically from smaller subunits. Some of these subunits are disrupted during the merging process, whereas others survive temporarily in the form of subhalos. A…

宇宙学与河外天体物理 · 物理学 2015-05-13 E. Zackrisson , T. Riehm

Invisibility cloaks, a subject that usually occurs in science fiction and myths, have attracted wide interest recently because of their possible realization. The biggest challenge to true invisibility is known to be the cloaking of a…

光学 · 物理学 2013-05-29 Baile Zhang , Yuan Luo , Xiaogang Liu , George Barbastathis

Gravitational lensing is a powerful tool to detect compact matter on very different mass scales. Of particular importance is the fact that lensing is sensitive to both luminous and dark matter alike. Depending on the mass scale, all lensing…

天体物理学 · 物理学 2007-05-23 Joachim Wambsganss

Gravitational lensing allows us to probe the structure of matter on a broad range of astronomical scales, and as light from a distant source traverses an intervening galaxy, compact matter such as planets, stars, and black holes act as…

宇宙学与河外天体物理 · 物理学 2009-11-09 Hugh Garsden , Geraint F. Lewis

Deflection of light by gravity was predicted by General Relativity and observationaly confirmed in 1919. In the following decades various aspects of the gravitational lens effect were explored theoretically, among them the possibility of…

天体物理学 · 物理学 2015-06-24 Joachim Wambsganss

Gravitational lensing by a spiral galaxy occurs when the line-of-sight to a background quasar passes within a few kpc from the center of the galactic disk. Since galactic disks are rich in neutral hydrogen, the quasar spectrum will likely…

天体物理学 · 物理学 2016-08-30 Abraham Loeb

Gravitational lensing has become one of the most interesting tools to study the mass distribution in the Universe. Since gravitational light deflection is independent of the nature and state of the matter, it is ideally suited to…

天体物理学 · 物理学 2007-05-23 Peter Schneider

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

We consider small-scale spheroidal clusters of weakly interacting massive particles in our Galaxy as non-compact gravitational microlenses and predict the appearance of caustics in the plane of a lensed source. The crossing of these…

天体物理学 · 物理学 2010-04-30 M. B. Bogdanov , A. M. Cherepashchuk

We review progress in understanding dark matter by astrophysics, and particularly via the effect of gravitational lensing. Evidence from many different directions now all imply that five sixths of the material content of the universe is in…

宇宙学与河外天体物理 · 物理学 2015-05-14 Richard Massey , Thomas Kitching , Johan Richard

Gravitational lensing is most often used as a tool to investigate the distribution of (dark) matter in the universe, but, if the mass distribution is known a priori, it becomes, at least in principle, a powerful probe of gravity itself.…

天体物理学 · 物理学 2009-11-06 Daniel J. Mortlock , Edwin L. Turner

According to the theory of general relativity, masses deflect light in a way similar to convex glass lenses. This gravitational lensing effect is astigmatic, giving rise to image distortions. These distortions allow to quantify cosmic…

宇宙学与河外天体物理 · 物理学 2016-12-21 Matthias Bartelmann , Matteo Maturi

Dark matter is an important ingredient of galaxies, as was recognised early on by Ken Freeman himself! Evidence for dark matter halos is still indirect, based on analysing motions of tracers such as gas and stars. In a sense the visible…

宇宙学与河外天体物理 · 物理学 2015-05-20 Konrad Kuijken

Gravitational lensing directly measures mass density fluctuations along the lines of sight to very distant objects. No assumptions need to be made concerning bias, the ratio of fluctuations in galaxy density to mass density. Hence, lensing…

天体物理学 · 物理学 2007-05-23 Joachim Wambsganss , Renyue Cen , Jeremiah P. Ostriker

The concept of an invisibility cloak is a fixture of science fiction, fantasy, and the collective imagination. However, a real device that could hide an object from sight in visible light from absolutely any viewpoint would be extremely…

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

After exactly a century since the formulation of the general theory of relativity, the phenomenon of gravitational lensing is still an extremely powerful method for investigating in astrophysics and cosmology. Indeed, it is adopted to study…

宇宙学与河外天体物理 · 物理学 2016-04-25 Francesco De Paolis , Mosè Giordano , Gabriele Ingrosso , Luigi Manni , Achille Nucita , Francesco Strafella
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