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Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A ∗ [PDF]

open access: yesClassical and quantum gravity, 2022
Horizon-scale images of black holes (BHs) and their shadows have opened an unprecedented window onto tests of gravity and fundamental physics in the strong-field regime.
S. Vagnozzi   +3 more
semanticscholar   +1 more source

The non-relativistic geometric trinity of gravity [PDF]

open access: yesGeneral Relativity and Gravitation, 2023
The geometric trinity of gravity comprises three distinct formulations of general relativity: (i) the standard formulation describing gravity in terms of spacetime curvature, (ii) the teleparallel equivalent of general relativity describing gravity in ...
William J. Wolf, James Read
semanticscholar   +1 more source

Classical and quantum gravity with fractional operators [PDF]

open access: yesClassical and quantum gravity, 2021
Following the same steps made for a scalar field in a parallel publication, we propose a class of perturbative theories of quantum gravity based on fractional operators, where the kinetic operator of the graviton is made of either fractional derivatives ...
G. Calcagni
semanticscholar   +1 more source

The off-shell recursion for gravity and the classical double copy for currents [PDF]

open access: yesJournal of High Energy Physics, 2021
We construct the off-shell recursion for gravity and the graviton current for the perturbative double field theory (DFT). We first formulate the perturbative DFT, which is equivalent but simpler to perturbative general relativity, to all-orders in ...
Kyoungho Cho, Kwangeon Kim, Kanghoon Lee
semanticscholar   +1 more source

Eikonal phase matrix, deflection angle, and time delay in effective field theories of gravity [PDF]

open access: yesPhysical Review D, 2020
The eikonal approximation is an ideal tool to extract classical observables in gauge theory and gravity directly from scattering amplitudes. Here we consider effective theories of gravity where in addition to the Einstein-Hilbert term we include non ...
Manuel Accettulli Huber   +3 more
semanticscholar   +1 more source

Decoherence of cosmological perturbations from boundary terms and the non-classicality of gravity [PDF]

open access: yesJournal of High Energy Physics, 2022
We note that the decoherence of inflationary curvature perturbation ζ is dominated by a boundary term of the gravity action. Although this boundary term cannot affect cosmological correlators 〈 ζ ^ n 〉, it induces much faster decoherence for ζ than that ...
C. Sou, Duc-Huy Tran, Yi Wang
semanticscholar   +1 more source

Supersymmetric backgrounds in (1 + 1) dimensions and inhomogeneous field theory

open access: yesJournal of High Energy Physics, 2023
We find a (1 + 1)-dimensional metric solution for a background hosting various supersymmetric field theories with a single non-chiral real supercharge. This supersymmetric background is globally hyperbolic even though it contains a naked null singularity.
Jeongwon Ho   +3 more
doaj   +1 more source

Isolated surfaces and symmetries of gravity [PDF]

open access: yesPhysical Review D, 2021
Conserved charges in theories with gauge symmetries are supported on codimension-2 surfaces in the bulk. It has recently been suggested that various classical formulations of gravity dynamics display different symmetries, and paying attention to the ...
Luca Ciambelli, R. Leigh
semanticscholar   +1 more source

Generating cosmological perturbations in non-singular Horndeski cosmologies

open access: yesJournal of High Energy Physics, 2023
We construct a concrete model of Horndeski bounce with strong gravity in the past. Within this model we show that the correct spectra of cosmological perturbations may be generated at early contracting epoch, with mild fine-tuning ensuring that the ...
Yulia Ageeva   +2 more
doaj   +1 more source

Distinguishable consequence of classical gravity on quantum matter [PDF]

open access: yesPhys. Rev. Lett. 134, 061501 (2025), 2023
What if gravity is classical? If true, a consistent co-existence of classical gravity and quantum matter requires that gravity exhibit irreducible fluctuations. These fluctuations can mediate classical correlations, but not quantum entanglement, between the quantized motion of the gravitationally interacting matter.
arxiv   +1 more source

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