In 1915, Einstein put the finishing touches on his radical reinvention of space, time, gravity and the Universe itself. The first experimental success of his beautiful theory, general relativity, dates back to 1919 when, during a solar eclipse, two British expeditions detected the predicted deflection of light rays travelling past the Sun. In the 1960s, systematic experiments in the Solar System started, while tests using the observation of binary pulsars began in the 1970s. General relativity has passed all these tests, in the so-called weak-field regime, with flying colors. However, thanks to a new generation of observational facilities, the past 20 years have seen remarkable changes in this research field and there are now various possibilities for testing general relativity and alternatives on much larger scales (i.e., cosmological tests), as well as in the strong-field regime with black holes and neutron stars.
On the cosmological side, while the dark matter problem is more likely due to some weakly interacting massive particles beyond the Standard Model rather than a breakdown of the laws of gravitation, the problem of dark energy is open. At the state of the facts, the accelerating expansion rate of the Universe may be explained by a small positive cosmological constant. Yet, it is possible that the actual explanation is either a breakdown of general relativity at large scales or the existence of some new field with peculiar properties.
From the astrophysical point of view, we can probe general relativity and various alternative theories of gravity by using electromagnetic waves from a black hole with an accretion disk, and gravitational waves from black-hole binaries. A direct observational confirmation of the nature of these exotic objects could be seen as an important test of the theory in the strong-gravity regime. Deviations from the Kerr metric may be indeed expected from classical extensions of general relativity as well as from macroscopic quantum gravity effects.
The purpose of this Research Topic is to collect contributions on current and proposed tests of general relativity, focusing on cosmological scales as well as on the strong-field regime. We welcome the submission of both original research articles and topical reviews (Brief Research Report, Data Report, General Commentary, Hypothesis and Theory, Methods, Mini Review and Review, Opinion, Original Research, and Perspective).
Topics of interest to this Research Topic include but are most certainly not limited to:
• Dark-energy tests of general relativity at cosmological scales
• Tests of general relativity with gravitational waves from black-hole mergers
• Testing general relativity and alternative theories of gravity using the black-hole shadow
• Revealing the properties of rotating black holes with the vorticity of light
• Testing general relativity using X-ray data.
In 1915, Einstein put the finishing touches on his radical reinvention of space, time, gravity and the Universe itself. The first experimental success of his beautiful theory, general relativity, dates back to 1919 when, during a solar eclipse, two British expeditions detected the predicted deflection of light rays travelling past the Sun. In the 1960s, systematic experiments in the Solar System started, while tests using the observation of binary pulsars began in the 1970s. General relativity has passed all these tests, in the so-called weak-field regime, with flying colors. However, thanks to a new generation of observational facilities, the past 20 years have seen remarkable changes in this research field and there are now various possibilities for testing general relativity and alternatives on much larger scales (i.e., cosmological tests), as well as in the strong-field regime with black holes and neutron stars.
On the cosmological side, while the dark matter problem is more likely due to some weakly interacting massive particles beyond the Standard Model rather than a breakdown of the laws of gravitation, the problem of dark energy is open. At the state of the facts, the accelerating expansion rate of the Universe may be explained by a small positive cosmological constant. Yet, it is possible that the actual explanation is either a breakdown of general relativity at large scales or the existence of some new field with peculiar properties.
From the astrophysical point of view, we can probe general relativity and various alternative theories of gravity by using electromagnetic waves from a black hole with an accretion disk, and gravitational waves from black-hole binaries. A direct observational confirmation of the nature of these exotic objects could be seen as an important test of the theory in the strong-gravity regime. Deviations from the Kerr metric may be indeed expected from classical extensions of general relativity as well as from macroscopic quantum gravity effects.
The purpose of this Research Topic is to collect contributions on current and proposed tests of general relativity, focusing on cosmological scales as well as on the strong-field regime. We welcome the submission of both original research articles and topical reviews (Brief Research Report, Data Report, General Commentary, Hypothesis and Theory, Methods, Mini Review and Review, Opinion, Original Research, and Perspective).
Topics of interest to this Research Topic include but are most certainly not limited to:
• Dark-energy tests of general relativity at cosmological scales
• Tests of general relativity with gravitational waves from black-hole mergers
• Testing general relativity and alternative theories of gravity using the black-hole shadow
• Revealing the properties of rotating black holes with the vorticity of light
• Testing general relativity using X-ray data.
