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相关论文: Hubble Constant, Lensing, and Time Delay in Relati…

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In a series of articles, we have shown that the newly discovered plasma-redshift cosmology gives a simpler, more accurate and consistent explanation of many cosmological phenomena than the big-bang cosmology. The SNe Ia observations are in…

天体物理学 · 物理学 2007-05-23 Ari Brynjolfsson

We discuss how inhomogeneities of the universe affect observations of the gravitational lensing; (1) the bending angle, (2) the lensing statistics and (3) the time delay. In order to take account of the inhomogeneities, the Dyer-Roeder…

天体物理学 · 物理学 2009-10-30 Hideki Asada

We derive the delay in travel time of photons due to the spin of a body both inside a rotating shell and outside a rotating body. We then show that this time delay by the spin of an astrophysical object might be detected in different images…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Ignazio Ciufolini , Franco Ricci

In light of the newly opened and rapidly growing gravitational waves window in multi-messenger astronomy, in order to fully take advantage of the new opportunities we are provided with, new ideas are required for a better and deeper employ…

宇宙学与河外天体物理 · 物理学 2020-11-06 Paolo Cremonese , Vincenzo Salzano

Under the assumption of a flat Lambda-CDM cosmology, recent data from the Planck satellite point toward a Hubble constant that is in tension with that measured by gravitational lens time delays and by the local distance ladder. Prosaically,…

Using strong lensing data Milgrom's MOdified Newtonian Dynamics (MOND) or its covariant TeVeS (Tensor-Vector-Scalar Theory) is being examined here as an alternative to the conventional $\Lambda$CDM paradigm. We examine 10 double-image…

星系天体物理 · 物理学 2011-05-10 Mu-Chen Chiu , Chung-Ming Ko , Yong Tian , HongSheng Zhao

We present a simultaneous analysis of 18 galaxy lenses with time delay measurements. For each lens we derive mass maps using pixelated simultaneous modeling with shared Hubble constant. We estimate the Hubble constant to be 66_{-4}^{+6}…

宇宙学与河外天体物理 · 物理学 2010-10-05 Danuta Paraficz , Jens Hjorth

(abridged) Gravitationally lensed quasars can be used as powerful cosmological and astrophysical probes. We can (i) infer the Hubble constant based on the time-delay technique, (ii) unveil substructures along the l.o.s. toward distant…

宇宙学与河外天体物理 · 物理学 2012-06-05 D. Sluse , V. Chantry , P. Magain , F. Courbin , G. Meylan

The Hubble constant is of paramount importance in astrophysics and cosmology. A large number of methods have been developed with different electromagnetic probes to estimate its value. The most recent results show a tension between values…

广义相对论与量子宇宙学 · 物理学 2025-06-19 Rosa Poggiani

We study gravitational lens time delays for a general family of lensing potentials, which includes the popular singular isothermal elliptical potential and singular isothermal elliptical density distribution but allows general angular…

天体物理学 · 物理学 2016-08-30 H. J. Witt , S. Mao , C. R. Keeton

Strongly lensed quasar systems with time delay measurements provide "time delay distances", which are a combination of three angular diameter distances and serve as powerful tools to determine the Hubble constant $H_0$. However, current…

宇宙学与河外天体物理 · 物理学 2019-12-18 Kai Liao , Arman Shafieloo , Ryan E. Keeley , Eric V. Linder

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

The 0th, 1st and 2nd derivatives of a ``Fermat potential'' give the three D's of gravitational lensing: delay, deflection and distortion. Observations of these delays, deflections and distortions for doubly and quadruply imaged quasars give…

天体物理学 · 物理学 2007-05-23 Paul L. Schechter

The light travel time differences in strong gravitational lensing systems allows an independent determination of the Hubble constant. This method has been successfully applied to several lens systems. The formally most precise measurements…

宇宙学与河外天体物理 · 物理学 2015-06-16 Peter Schneider , Dominique Sluse

Double-plane gravitational lensing is a rare but increasingly observed phenomenon in which the light from a distant source is lensed by two foreground objects at different redshifts. Such systems can be used to provide simultaneous…

宇宙学与河外天体物理 · 物理学 2026-02-04 Daniel Johnson , Pierre Fleury , Martin Millon

The best studied gravitational lens is the Twin QSO Q0957+561, and as a result of recent advances in observations and modelling, a ten percent measurement of the Hubble constant is attainable. We discuss in detail this system and review the…

天体物理学 · 物理学 2009-10-30 L. J. Goicoechea , E. Mediavilla , A. Oscoz , M. Serra-Ricart , J. Buitrago

We present a refined gravitational lens model of the four-image lens system B1608+656 based on new and improved observational constraints: (i) the three independent time-delays and flux-ratios from VLA observations, (ii) the radio-image…

天体物理学 · 物理学 2009-11-07 L. V. E. Koopmans , T. Treu , C. D. Fassnacht , R. D. Blandford , G. Surpi

We present a blind time-delay cosmography measurement of the Hubble constant $H_0$ based on the quadruply imaged quasar SDSSJ1433+6007. Our analysis combines deep Hubble Space Telescope imaging, extended time-delay monitoring from the…

There is growing evidence that the majority of the energy density of the universe is not baryonic or dark matter, rather it resides in an exotic component with negative pressure. The nature of this `quintessence' influences our view of the…

天体物理学 · 物理学 2011-03-10 Geraint F. Lewis , Rodrigo A. Ibata

We consider an alternative formula for time delay in gravitational lensing. Imposing a smoothness condition on the gravitationally deformed paths followed by the photons from the source to the observer, we show that our formula displays the…

宇宙学与河外天体物理 · 物理学 2018-07-04 Nicola Alchera , Marco Bonici , Roberta Cardinale , Alba Domi , Nicola Maggiore , Chiara Righi , Silvano Tosi