Results 21 to 30 of about 677 (118)
The cosmic distance duality relation (CDDR), expressed as d _L ( z ) = (1 + z ) ^2 D _A ( z ), is a fundamental relation in modern cosmology. In this work, we apply a method to test the CDDR using simulated strongly lensed gravitational-wave (SLGW ...
Yong Yuan +6 more
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Quasar Milli-lensing and Cold Dark Matter (TNG50) Subhaloes. I. Image Splitting
We use numerical mass density profiles from the TNG50 simulation to study the impact of gravitational milli-lensing by dark matter subhaloes on the images of lensed quasars.
E. Mediavilla +3 more
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Microlensing timescales and flux magnification probabilities of a sample of 204 lensed quasars
Context. Quasar microlensing is a very useful tool in cosmology and astrophysics, as well as a source of uncertainty in certain investigations, such as the determination of the Hubble constant from lensed quasars.
Ávila-Vera F., Motta V., Mediavilla E.
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Dynamical Systematics for Time-delay Lenses and the Impact on the Hubble Constant
While time-delay lenses can independently probe H _0 , the estimates are degenerate with the convergence of the lens near the Einstein radius. Velocity dispersions, σ , can be used to break the degeneracy, with uncertainties Δ H / H _0 ∝ Δ σ ^2 / σ ^2 ...
R. Forés-Toribio +2 more
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Strong Gravitational-wave Lensing Posterior Odds
Like light, gravitational waves are gravitationally lensed by intervening massive astrophysical objects—such as galaxies, clusters, black holes, and stars—resulting in a variety of potentially observable gravitational-wave lensing signatures.
Otto A. Hannuksela +6 more
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With the advancement of third-generation gravitational-wave (GW) detectors, the identification of strongly lensed GW events is expected to play an increasingly vital role in cosmology and fundamental physics.
Dejiang Li +6 more
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Hierarchical Cosmological Constraints through a Strong-lensing Distance Ratio
Strong gravitational lensing provides an independent and powerful probe of cosmic expansion by directly linking observables to cosmological distances.
Shuaibo Geng +5 more
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When a rectangular hyperbola is constructed from the image positions of a quadruply lensed quasar, as proposed by Witt, it passes very close to the lensing galaxy. The median measured perpendicular offset between the observed light center of the lens and
Paul L. Schechter, Richard Luhtaru
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As plans for the construction of third-generation gravitational-wave (GW) detectors advance, research into strongly lensed GWs has become increasingly critical. It is anticipated that hundreds of multi-image lensed GWs will be detected annually.
Youkai Li +6 more
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A Targeted Search for Variable Gravitationally Lensed Quasars
We present a pipeline to identify photometric variability within strong gravitationally lensing candidates, in the Dark Energy Spectroscopic Instrument Legacy Imaging Surveys.
William Sheu +6 more
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