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相关论文: Effects of Dark Matter Substructures on Gravitatio…

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Lensing flux-ratio anomalies have been frequently observed and taken as evidence for the presence of abundant dark matter substructures in lensing galaxies, as predicted by the cold dark matter (CDM) model of cosmogony. In previous work, we…

宇宙学与河外天体物理 · 物理学 2015-05-18 D. D. Xu , S. Mao , A. Cooper , J. Wang , L. Gao , C. S. Frenk , V. Springel

It has been argued that the flux anomalies detected in gravitationally lensed QSOs are evidence for substructures in the foreground lensing haloes. In this paper we investigate this issue in greater detail focusing on the Cusp relation…

天体物理学 · 物理学 2009-11-11 Andrea V. Maccio' , Marco Miranda

Lensing flux-ratio anomalies are most likely caused by gravitational lensing by small-scale dark matter structures. These anomalies offer the prospect of testing a fundamental prediction of the cold dark matter (CDM) cosmological model: the…

宇宙学与河外天体物理 · 物理学 2014-10-20 D. D. Xu , Dominique Sluse , Liang Gao , Jie Wang , Carlos Frenk , Shude Mao , Peter Schneider

The flux-ratio anomalies observed in multiply-lensed quasar images are most plausibly explained as the result of perturbing structures superposed on the underlying smooth matter distribution of the primary lens. The cold dark matter…

宇宙学与河外天体物理 · 物理学 2015-05-30 D. D. Xu , Shude Mao , Andrew Cooper , Liang Gao , Carlos Frenk , Raul Angulo , John Helly

We investigate the statistics of flux anomalies in gravitationally lensed QSOs as a function of dark matter halo properties such as substructure content and halo ellipticity. We do this by creating a very large number of simulated lenses…

宇宙学与河外天体物理 · 物理学 2015-05-19 R. Benton Metcalf , Adam Amara

We explore the halo-to-halo variation of dark matter substructure in galaxy-sized dark matter halos, focusing on its implications for strongly gravitational lensed systems. We find that the median value for projected substructure mass…

宇宙学与河外天体物理 · 物理学 2015-05-27 Jacqueline Chen , Savvas M. Koushiappas , Andrew R. Zentner

We review the evidence for substructures from the anomalous flux ratios in gravitational lenses. Using high-resolution numerical simulations, we show that at typical image positions, the fraction of surface mass density in substructures is…

天体物理学 · 物理学 2009-11-10 S. Mao , Y. P. Jing , J. P. Ostriker , J. Weller

We have performed the largest ever particle simulation of a Milky Way-sized dark matter halo, and present the most comprehensive convergence study for an individual dark matter halo carried out thus far. We have also simulated a sample of 6…

We show how observations of multiply-imaged quasars at high redshift can be used as a probe of dark matter clumps (subhalos with masses ~ 10^9 solar masses) within the virialized extent of more massive lensing halos. A large abundance of…

天体物理学 · 物理学 2015-06-24 R. Benton Metcalf , Piero Madau

We present a study of the lens properties of quadruply imaged systems, lensed by numerically simulated galaxies. We investigate a simulated elliptical and disc galaxy drawn from high resolution simulations of galaxy formation in a…

天体物理学 · 物理学 2009-11-07 M. Bradac , P. Schneider , M. Lombardi , M. Steinmetz , L. V. E. Koopmans , Julio F. Navarro

Gravitational lens flux ratio anomalies are a powerful probe of small-scale mass structures, often attributed to dark matter subhalos. However, baryonic components can also play a significant role. This study investigates, for the first…

宇宙学与河外天体物理 · 物理学 2026-05-29 Xikai Shan , Yunpeng Jin , Shude Mao

We investigate the effects of numerous dark matter subhalos in a galaxy-sized halo on the events of strong lensing, to assess their presence as expected from the cold dark matter scenario. Lens galaxies are represented by a smooth ellipsoid…

天体物理学 · 物理学 2009-11-07 Masashi Chiba

The gravitational lensing constraints on the small mass end of the LCDM mass function are discussed. Here a conservative approach is taken where only the most difficult to explain image flux anomalies in strong QSO lenses are emphasized.…

天体物理学 · 物理学 2009-11-10 R. Benton Metcalf

Discrepancies between the observed and model-predicted radio flux ratios are seen in a number of quadruply-lensed quasars. The most favored interpretation of these anomalies is that CDM substructures present in lensing galaxies perturb the…

宇宙学与河外天体物理 · 物理学 2015-06-23 Dandan Xu , Dominique Sluse , Liang Gao , Jie Wang , Carlos Frenk , Shude Mao , Peter Schneider , Volker Springel

We explore the weak lensing effect by line-of-sight halos and sub-halos with a mass of M < 10^7 solar mass in QSO-galaxy strong lens systems with quadruple images in a concordant LCDM universe. Using a polynomially fitted non-linear power…

宇宙学与河外天体物理 · 物理学 2015-03-20 Kaiki Taro Inoue , Ryuichi Takahashi

Multiply-imaged quasar lenses can be used to constrain the substructure mass fraction in galaxy-sized dark matter halos via anomalous flux ratios in lensed images. The flux ratios, however, can be affected by both the substructure in the…

天体物理学 · 物理学 2008-11-26 Jacqueline Chen , Andrey V. Kravtsov , Charles R. Keeton

The flux anomalies in four-image gravitational lenses can be interpreted as evidence for the dark matter substructure predicted by cold dark matter (CDM) halo models. In principle, these flux anomalies could arise from alternate sources…

天体物理学 · 物理学 2008-11-26 C. S. Kochanek , N. Dalal

Gravitational lenses with anomalous flux ratios are often cited as possible evidence for dark matter satellites predicted by simulations of hierarchical merging in cold dark matter cosmogonies. We show that the fraction of quads with…

天体物理学 · 物理学 2009-11-13 E. M. Shin , N. W. Evans

To set useful limits on the abundance of small-scale dark matter halos (subhalos) in a galaxy scale, we have carried out mid-infrared imaging and integral-field spectroscopy for a sample of quadruple lens systems showing anomalous flux…

We investigate the impact of baryonic physics on the subhalo population by analyzing the results of two recent hydrodynamical simulations (EAGLE and Illustris), which have very similar configuration, but a different model of baryonic…

星系天体物理 · 物理学 2017-06-21 Giulia Despali , Simona Vegetti
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