Analysis of the Angular Dependence of Time Delay in Gravitational Lensing
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 same degrees of freedom as the standard one. In addition to...
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doaj-6358b10df20949ef935113467a3970d32020-11-24T20:43:25ZengMDPI AGSymmetry2073-89942018-07-0110724610.3390/sym10070246sym10070246Analysis of the Angular Dependence of Time Delay in Gravitational LensingNicola Alchera0Marco Bonici1Roberta Cardinale2Alba Domi3Nicola Maggiore4Chiara Righi5Silvano Tosi6Dipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyI.N.F.N.—Sezione di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, I-16146 Genova, ItalyWe 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 same degrees of freedom as the standard one. In addition to this, it is shown that the standard expression for time delay is recovered when small angles are involved. These two features strongly support the claim that the formula for time delay studied in this paper is the generalization to the arbitrary angles of the standard one, which is valid at small angles. This could therefore result in a useful tool in Astrophysics and Cosmology which may be applied to investigate the discrepancy between the various estimates of the Hubble constant. As an aside, two interesting consequences of our proposal for time delay are discussed: the existence of a constraint on the gravitational potential generated by the lens and a formula for the mass of the lens in the case of central potential.http://www.mdpi.com/2073-8994/10/7/246classical general relativitygravitational lensestime delay |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Nicola Alchera Marco Bonici Roberta Cardinale Alba Domi Nicola Maggiore Chiara Righi Silvano Tosi |
spellingShingle |
Nicola Alchera Marco Bonici Roberta Cardinale Alba Domi Nicola Maggiore Chiara Righi Silvano Tosi Analysis of the Angular Dependence of Time Delay in Gravitational Lensing Symmetry classical general relativity gravitational lenses time delay |
author_facet |
Nicola Alchera Marco Bonici Roberta Cardinale Alba Domi Nicola Maggiore Chiara Righi Silvano Tosi |
author_sort |
Nicola Alchera |
title |
Analysis of the Angular Dependence of Time Delay in Gravitational Lensing |
title_short |
Analysis of the Angular Dependence of Time Delay in Gravitational Lensing |
title_full |
Analysis of the Angular Dependence of Time Delay in Gravitational Lensing |
title_fullStr |
Analysis of the Angular Dependence of Time Delay in Gravitational Lensing |
title_full_unstemmed |
Analysis of the Angular Dependence of Time Delay in Gravitational Lensing |
title_sort |
analysis of the angular dependence of time delay in gravitational lensing |
publisher |
MDPI AG |
series |
Symmetry |
issn |
2073-8994 |
publishDate |
2018-07-01 |
description |
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 same degrees of freedom as the standard one. In addition to this, it is shown that the standard expression for time delay is recovered when small angles are involved. These two features strongly support the claim that the formula for time delay studied in this paper is the generalization to the arbitrary angles of the standard one, which is valid at small angles. This could therefore result in a useful tool in Astrophysics and Cosmology which may be applied to investigate the discrepancy between the various estimates of the Hubble constant. As an aside, two interesting consequences of our proposal for time delay are discussed: the existence of a constraint on the gravitational potential generated by the lens and a formula for the mass of the lens in the case of central potential. |
topic |
classical general relativity gravitational lenses time delay |
url |
http://www.mdpi.com/2073-8994/10/7/246 |
work_keys_str_mv |
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1716820045066141696 |