Results 51 to 60 of about 178,240 (316)

Double scaling limits of Dirac ensembles and Liouville quantum gravity [PDF]

open access: yesJournal of Physics A: Mathematical and Theoretical, 2022
In this paper we study ensembles of finite real spectral triples equipped with a path integral over the space of possible Dirac operators. In the noncommutative geometric setting of spectral triples, Dirac operators take the center stage as a replacement
Hamed Hessam   +2 more
semanticscholar   +1 more source

The semiclassical gravitational path integral and random matrices (toward a microscopic picture of a dS2 universe)

open access: yesJournal of High Energy Physics, 2021
We study the genus expansion on compact Riemann surfaces of the gravitational path integral Z grav m $$ {\mathcal{Z}}_{\mathrm{grav}}^{(m)} $$ in two spacetime dimensions with cosmological constant Λ > 0 coupled to one of the non-unitary minimal models ...
Dionysios Anninos, Beatrix Mühlmann
doaj   +1 more source

Towards background independent quantum gravity with tensor models [PDF]

open access: yesClassical and quantum gravity, 2018
We explore whether the phase diagram of tensor models could feature a pregeometric, discrete and a geometric, continuum phase for the building blocks of space. The latter are associated to rank d tensors of size N.
A. Eichhorn   +3 more
semanticscholar   +1 more source

Effective dynamics of scalar cosmological perturbations from quantum gravity [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2021
We derive an effective dynamics for scalar cosmological perturbations from quantum gravity, in the framework of group field theory condensate cosmology. The emergent spacetime picture is obtained from the mean-field hydrodynamic regime of the fundamental
L. Marchetti, D. Oriti
semanticscholar   +1 more source

Quantum singularities in a model of f(R) gravity [PDF]

open access: yesThe European Physical Journal C, 2012
The formation of a naked singularity in a model of f(R) gravity having as source a linear electromagnetic field is considered in view of quantum mechanics. Quantum test fields obeying the Klein-Gordon, Dirac and Maxwell equations are used to probe the classical timelike naked singularity developed at r=0.
Gürtuğ, Özay   +2 more
openaire   +5 more sources

(Loop) quantum gravity and the inflationary scenario [PDF]

open access: yes, 2015
Quantum gravity, as a fundamental theory of space-time, is expected to reveal how the universe may have started, perhaps during or before an inflationary epoch.
Bojowald, Martin
core   +2 more sources

Mass and horizon Dirac observables in effective models of quantum black-to-white hole transition [PDF]

open access: yesClassical and quantum gravity, 2019
In the past years, black holes and the fate of their singularity have been heavily studied within loop quantum gravity. Effective spacetime descriptions incorporating quantum geometry corrections are provided by the so-called polymer models.
N. Bodendorfer   +2 more
semanticscholar   +1 more source

Positivity in Lorentzian Barrett–Crane models of quantum gravity [PDF]

open access: yesClassical and Quantum Gravity, 2006
The Barrett-Crane models of Lorentzian quantum gravity are a family of spin foam models based on the Lorentz group. We show that for various choices of edge and face amplitudes, including the Perez-Rovelli normalization, the amplitude for every triangulated closed 4-manifold is a non-negative real number.
Cherrington, J. Wade   +1 more
openaire   +2 more sources

Two dimensional nearly de Sitter gravity

open access: yesJournal of High Energy Physics, 2021
We study some aspects of the de Sitter version of Jackiw-Teitelboim gravity. Though we do not have propagating gravitons, we have a boundary mode when we compute observables with a fixed dilaton and metric at the boundary.
Juan Maldacena   +2 more
doaj   +1 more source

Discrete Lorentzian Quantum Gravity [PDF]

open access: yes, 2000
Just as for non-abelian gauge theories at strong coupling, discrete lattice methods are a natural tool in the study of non-perturbative quantum gravity. They have to reflect the fact that the geometric degrees of freedom are dynamical, and that therefore
Loll, R.
core   +4 more sources

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