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Loop Quantum Gravity [PDF]

open access: yesLiving Reviews in Relativity, 2008
The problem of describing the quantum behavior of gravity, and thus understanding quantum spacetime, is still open. Loop quantum gravity is a well-developed approach to this problem. It is a mathematically well-defined background-independent quantization
Rovelli Carlo
doaj   +11 more sources

The volume operator in covariant quantum gravity [PDF]

open access: yesClassical and Quantum Gravity, 2010
A covariant spin-foam formulation of quantum gravity has been recently developed, characterized by a kinematics which appears to match well the one of canonical loop quantum gravity.
Alexandrov S   +30 more
core   +11 more sources

From Classical To Quantum Gravity: Introduction to Loop Quantum Gravity [PDF]

open access: yesProceedings of 3rd Quantum Gravity and Quantum Geometry School — PoS(QGQGS 2011), 2013
We present an introduction to the canonical quantization of gravity performed in loop quantum gravity, based on lectures held at the 3rd quantum geometry and quantum gravity school in Zakopane in 2011.
Giesel, Kristina, Sahlmann, Hanno
core   +2 more sources

Matter in Loop Quantum Gravity [PDF]

open access: yesSymmetry, Integrability and Geometry: Methods and Applications, 2012
Loop quantum gravity, a non-perturbative and manifestly background free, quantum theory of gravity implies that at the kinematical level the spatial geometry is discrete in a specific sense.
Ghanashyam Date, Golam Mortuza Hossain
doaj   +5 more sources

Loop quantum gravity’s boundary maps [PDF]

open access: yesClassical and Quantum Gravity, 2021
Abstract In canonical quantum gravity, the presence of spatial boundaries naturally leads to boundary quantum states, representing quantum boundary conditions for the bulk fields. As a consequence, quantum states of the bulk geometry need to be upgraded to wave-functions valued in the boundary Hilbert space: the bulk becomes quantum ...
Qian Chen, Etera R Livine
openaire   +2 more sources

Perturbatively exact w 1+∞ asymptotic symmetry of quantum self-dual gravity

open access: yesJournal of High Energy Physics, 2022
The infinite tower of positive-helicity soft gravitons in any minimally coupled, tree-level, asymptotically flat four-dimensional (4D) gravity was recently shown to generate a w 1+∞ asymptotic symmetry algebra. It is natural to ask whether this classical
Adam Ball   +3 more
doaj   +1 more source

Does the Loop Quantum μo Scheme Permit Black Hole Formation?

open access: yesUniverse, 2021
We explore the way different loop quantization prescriptions affect the formation of trapped surfaces in the gravitational collapse of a homogeneous dust cloud, with particular emphasis on the so-called μo scheme in which loop quantum cosmology was ...
Bao-Fei Li, Parampreet Singh
doaj   +1 more source

Quaternion-Loop Quantum Gravity [PDF]

open access: yesFoundations of Physics, 2009
It is shown that the Riemannian curvature of the 3-dimensional hypersurfaces in space-time, described by the Wilson loop integral, can be represented by a quaternion quantum operator induced by the SU(2) gauge potential, thus providing a justification for quaternion quantum gravity at the Tev energy scale.
Maia, M. D.   +2 more
openaire   +3 more sources

Loop Quantum Black Hole Extensions Within the Improved Dynamics

open access: yesFrontiers in Astronomy and Space Sciences, 2021
We continue our investigation of an improved quantization scheme for spherically symmetric loop quantum gravity. We find that in the region where the black hole singularity appears in the classical theory, the quantum theory contains semi-classical ...
Rodolfo Gambini   +2 more
doaj   +1 more source

Loop-Quantum-Gravity Vertex Amplitude [PDF]

open access: yesPhysical Review Letters, 2007
Spinfoam theories are hoped to provide the dynamics of non-perturbative loop quantum gravity. But a number of their features remain elusive. The best studied one -the euclidean Barrett-Crane model- does not have the boundary state space needed for this, and there are recent indications that, consequently, it may fail to yield the correct low-energy $n$-
Engle, Jonathan   +2 more
openaire   +5 more sources

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