Time delay of the photons coupled to the Weyl tensor in a regular phantom black hole is investigated in both weak and strong deflection gravitational lensing. We find that the time delay in the weak deflection lensing strongly depends on the phantom hair while the delay in the strong deflection lensing is significantly affected by the hair and the strength of the coupling. We suggest that it is necessary to measure these two kind of time signals for fully understanding and distinguishing such an interaction beyond the standard Einstein–Maxwell theory
Current constraints on Einstein’s weak equivalence principle (WEP) utilize the observed time delay b...
We investigate the potential of high-energy astrophysical events, from which both massless and massi...
In this article, we have investigated the equations of motion of the photons coupled to Weyl tensor ...
We study strong gravitational lensing for photons coupled to Weyl tensor in a regular phantom black ...
Beyond the Einstein–Maxwell model, electromagnetic field might couple with gravitational field throu...
We calculate the time delay between different relativistic images formed by black hole gravitational...
We calculate the time delay between different relativistic images formed by black hole gravitational...
We calculate the time delay between different relativistic images formed by black hole gravitational...
International audienceThis paper investigates the use of gravitational time delays of macro-lenses t...
Gravitational lensing can happen not only for null signals but also timelike signals such as neutrin...
The current standard time delay formula (CSTD) in gravitational lensing and its claimed relation to ...
International audienceThe gravitational deflection of massless and massive particles, both with and ...
Gravitational lens time delays depend on the Hubble constant, the observed image positions, and the ...
Strong gravitational lenses with measured time delays between the multiple images and models of the ...
Time delays between lensed multiple images have been known to provide an interesting probe of the Hu...
Current constraints on Einstein’s weak equivalence principle (WEP) utilize the observed time delay b...
We investigate the potential of high-energy astrophysical events, from which both massless and massi...
In this article, we have investigated the equations of motion of the photons coupled to Weyl tensor ...
We study strong gravitational lensing for photons coupled to Weyl tensor in a regular phantom black ...
Beyond the Einstein–Maxwell model, electromagnetic field might couple with gravitational field throu...
We calculate the time delay between different relativistic images formed by black hole gravitational...
We calculate the time delay between different relativistic images formed by black hole gravitational...
We calculate the time delay between different relativistic images formed by black hole gravitational...
International audienceThis paper investigates the use of gravitational time delays of macro-lenses t...
Gravitational lensing can happen not only for null signals but also timelike signals such as neutrin...
The current standard time delay formula (CSTD) in gravitational lensing and its claimed relation to ...
International audienceThe gravitational deflection of massless and massive particles, both with and ...
Gravitational lens time delays depend on the Hubble constant, the observed image positions, and the ...
Strong gravitational lenses with measured time delays between the multiple images and models of the ...
Time delays between lensed multiple images have been known to provide an interesting probe of the Hu...
Current constraints on Einstein’s weak equivalence principle (WEP) utilize the observed time delay b...
We investigate the potential of high-energy astrophysical events, from which both massless and massi...
In this article, we have investigated the equations of motion of the photons coupled to Weyl tensor ...