Results 71 to 80 of about 2,908,412 (339)

Tree-level scattering amplitudes in nonlocal field theories

open access: yesJournal of High Energy Physics, 2021
We prove in two ways that, for a special class of nonlocal field theories consistent with linear and non-linear stability at the classical level, and with unitarity and super-renormalizability or finiteness at the quantum level, the n-point tree-level ...
Leonardo Modesto, Gianluca Calcagni
doaj   +1 more source

On scalar and vector fields coupled to the energy-momentum tensor

open access: yesJournal of High Energy Physics, 2018
We consider theories for scalar and vector fields coupled to the energy-momentum tensor. Since these fields also carry a non-trivial energy-momentum tensor, the coupling prescription generates self-interactions. In analogy with gravity theories, we build
Jose Beltrán Jiménez   +2 more
doaj   +1 more source

Field theory for gravity at all scales [PDF]

open access: yesProceedings of the MG15 Meeting on General Relativity 2018 (2022) 1017, 2019
We review here the main advances made by using effective field theories (EFTs) in classical gravity, with notable focus on those unique to the EFTs of post-Newtonian (PN) gravity. We then proceed to overview the various prospects of using field theory to study the real-world gravitational wave (GW) data, as well as to ameliorate our fundamental ...
arxiv   +1 more source

Quantum gravity fluctuations in the timelike Raychaudhuri equation

open access: yesJournal of High Energy Physics, 2023
We consider a timelike geodesic congruence in the presence of perturbative quantum fluctuations of the spacetime metric. We calculate the change in the volume of a bundle of geodesics due to such fluctuations and thereby obtain a quantum-gravitationally ...
Sang-Eon Bak   +3 more
doaj   +1 more source

On Classical Equivalence Between Noncritical and Einstein Gravity : The AdS/CFT Perspectives [PDF]

open access: yes, 2012
We find that noncritical gravity, a special class of higher derivative gravity, is classically equivalent to Einstein gravity at the full nonlinear level. We obtain the viscosity-to-entropy ratio and the second order transport coefficients of the dual fluid of noncritical gravity to all orders in the coupling of higher derivative terms. We also compute
arxiv   +1 more source

Corners of gravity: the case of gravity as a constrained BF theory

open access: yesJournal of High Energy Physics, 2021
Following recent works on corner charges we investigate the boundary structure in the case of the theory of gravity formulated as a constrained BF theory.
Remigiusz Durka, Jerzy Kowalski-Glikman
doaj   +1 more source

Null infinity as an open Hamiltonian system

open access: yesJournal of High Energy Physics, 2021
When a system emits gravitational radiation, the Bondi mass decreases. If the Bondi energy is Hamiltonian, it can thus only be a time-dependent Hamiltonian. In this paper, we show that the Bondi energy can be understood as a time-dependent Hamiltonian on
Wolfgang Wieland
doaj   +1 more source

How unimodular gravity theories differ from general relativity at quantum level [PDF]

open access: yes, 2015
We investigate path integral quantization of two versions of unimodular gravity. First a fully diffeomorphism-invariant theory is analyzed, which does not include a unimodular condition on the metric, while still being equivalent to other unimodular ...
R. Bufalo   +3 more
semanticscholar   +1 more source

A Macroscopically Effective Lorentz Gauge Theory of Gravity [PDF]

open access: yesClassical and Quantum Gravity, 33 (2016) 235006, 2016
Following the ideas of effective field theories, we derive classically effective field equations of recently developed Lorentz gauge theory of gravity. It is shown that Newton's gravitational constant emerges as an effective coupling parameter if an extremely small length is integrated out of the underlying theory.
arxiv   +1 more source

Gravitational SL(2, ℝ) algebra on the light cone

open access: yesJournal of High Energy Physics, 2021
In a region with a boundary, the gravitational phase space consists of radiative modes in the interior and edge modes at the boundary. Such edge modes are necessary to explain how the region couples to its environment.
Wolfgang Wieland
doaj   +1 more source

Home - About - Disclaimer - Privacy