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相关论文: Gravitational lensing effects on sub-millimetre ga…

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The magnification effect of gravitational lensing is a powerful probe of the distribution of matter in the universe, yet it is frequently overlooked due to the fact that its signal to noise is smaller than that of lensing shear. Because its…

宇宙学与河外天体物理 · 物理学 2014-04-23 Anne H. Bauer , Enrique Gaztañaga , Pol Martí , Ramon Miquel

In cosmological N-body simulations, the baryon effects on the cold dark matter (CDM) halos can be used to solve the small scale problems in $\Lambda$CDM cosmology, such as cusp-core problem and missing satellites problem. It turns out that…

星系天体物理 · 物理学 2017-08-02 Lin Wang , Da-Ming Chen

We reanalyse optical gravitational lens surveys from the literature in order to determine relative probabilities in the $\lambda_{0}$-$\Omega_{0}$ plane, using a softened singular isothermal sphere lens model. In addition, we examine a…

天体物理学 · 物理学 2007-05-23 Ralf Quast , Phillip Helbig

We investigate the influence of the matter along the line of sight and in the lens environment on the image configurations, relative time delays, and the resulting models of strong gravitational lensing. The distribution of matter in space…

宇宙学与河外天体物理 · 物理学 2015-06-18 M. Jaroszynski , Z. Kostrzewa-Rutkowska

We quantify the accuracy with which the cosmological parameters characterizing the energy density of matter (\Omega_m), the amplitude of the power spectrum of matter fluctuations (\sigma_8), the energy density of neutrinos (\Omega_{\nu})…

宇宙学与河外天体物理 · 物理学 2015-06-05 Surhud More , Frank van den Bosch , Marcello Cacciato , Anupreeta More , Houjun Mo , Xiaohu Yang

Gravitational lensing effects arise from the light ray deflection by all of the mass distribution along the line of sight. It is then expected that weak lensing cluster surveys can provide us true mass-selected cluster samples. With…

天体物理学 · 物理学 2009-11-13 J. Y. Tang , Z. H. Fan

This paper argues that there is a large population of dark galaxies which reveals its presence by the gravitational lensing of quasars, and outnumbers normal galaxies by around 3:1. There are 8 double quasars with a separation greater than…

天体物理学 · 物理学 2007-05-23 M. R. S. Hawkins

The angular correlation function \wth of faint galaxies is affected both by nonlinear gravitational evolution and by magnification bias due to gravitational lensing. We compute the resulting \wth for different cosmological models and show…

天体物理学 · 物理学 2020-11-25 R. Moessner , B. Jain , J. V. Villumsen

We combine photometry and lens modeling to study the properties of 17 gravitational lens galaxies between z=0.1 and 1. Most of the lens galaxies are passively evolving early-type galaxies, with a few spirals. The colors, scale lengths, and…

天体物理学 · 物理学 2010-03-01 C. R. Keeton , C. S. Kochanek , E. E. Falco

Some aspects of gravitational lensing by large scale structure (LSS) are investigated. We show that lensing causes the damping tail of the cosmic microwave background (CMB) power spectrum to fall less rapidly with decreasing angular scale…

天体物理学 · 物理学 2015-06-24 R. Benton Metcalf , Joseph Silk

Gravitational lensing can amplify the apparent brightness of distant sources. Images that are highly magnified are often part of multiply-imaged systems, but we consider the possibility of having large magnifications without additional…

天体物理学 · 物理学 2009-11-10 Charles R. Keeton , Michael Kuhlen , Zoltan Haiman

We gain insight into the effects of gravitational lensing on the estimated distribution of merging binaries observed through gravitational waves. We quantify the efficiency of magnification for gravitational wave events in the geometric…

宇宙学与河外天体物理 · 物理学 2020-01-15 O. Contigiani

We present the results of a study of weak lensing by galaxies based on 45.5 deg$^2$ of $R_C$ band imaging data from the Red-Sequence Cluster Survey (RCS). We present the first weak lensing detection of the flattening of galaxy dark matter…

天体物理学 · 物理学 2008-11-26 Henk Hoekstra , Howard K. C. Yee , Michael D. Gladders

We present the effects of ellipticity of matter distribution in massive halos on the observation of supernovae. A pseudo elliptical Navarro-Frenk-White (NFW) mass model is used to calculate the introduced gain factors and observation rates…

天体物理学 · 物理学 2007-05-23 Hamed Bagherpour

It has been proposed that the MACHOs in our galaxy could be clumped in globular cluster--like associations or RAMBOs (robust associations of massive baryonic objects) (Moore \& Silk 1995). Here we investigate the effect such clustering has…

天体物理学 · 物理学 2015-06-24 R Benton Metcalf , Joseph Silk

With the increase in the number of observed gravitational wave (GW) signals, detecting strongly lensed GWs by galaxies has become a real possibility. Lens galaxies also contain microlenses (e.g., stars and black holes), introducing further…

星系天体物理 · 物理学 2022-10-05 Ashish Kumar Meena , Anuj Mishra , Anupreeta More , Sukanta Bose , Jasjeet Singh Bagla

The dark matter halo has non-negligible effects on the gravitational lensing of supermassive black hole in the galaxy center. Our work presents a study on the time-delay of light in gravitational lensing of black holes enclosed by dark…

广义相对论与量子宇宙学 · 物理学 2024-10-14 Chen-Kai Qiao , Ping Su

We study lensing by voids in Cubic Galileon and Nonlocal gravity cosmologies, which are examples of theories of gravity that modify the lensing potential. We find voids in the dark matter and halo density fields of N-body simulations and…

宇宙学与河外天体物理 · 物理学 2015-09-15 Alexandre Barreira , Marius Cautun , Baojiu Li , Carlton Baugh , Silvia Pascoli

Differential magnification is now well-known to distort the spectral energy distributions of strongly gravitationally lensed galaxies. However, that does not mean that any distortions are possible. Here I prove an analytic upper bound to…

星系天体物理 · 物理学 2024-03-05 Stephen Serjeant

A possible wave effect in the gravitational lensing phenomenon is discussed. We consider the interference of two coherent gravitational waves of slightly different frequencies from a compact binary, due to the gravitational lensing by a…

天体物理学 · 物理学 2009-11-11 Kazuhiro Yamamoto