Manifestly gauge-invariant general relativistic perturbation theory: II. FRW background and first order

DOI10.1088/0264-9381/27/5/055006zbMath1186.83005arXiv0711.0117OpenAlexW2038855700MaRDI QIDQ3549991

No author found.

Publication date: 30 March 2010

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0711.0117

zbMATH Keywords

cosmologyequations of motionexact solutionsEinstein's equationsgravitational wavesCauchy problemscanonical formalismgeneral structure

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (13)

Coherent states, quantum gravity, and the Born-Oppenheimer approximation. I. General considerations ⋮ Effective dynamics of scalar cosmological perturbations from quantum gravity ⋮ Synchronous coordinates and gauge-invariant observables in cosmological spacetimes ⋮ Loop quantum gravity ⋮ The Holst spin foam model via cubulations ⋮ Dynamics of Dirac observables in canonical cosmological perturbation theory ⋮ One-loop quantum gravitational backreaction on the local Hubble rate ⋮ Graviton backreaction on the local cosmological expansion in slow-roll inflation ⋮ Gauge invariant perturbation theory via homotopy transfer ⋮ Loop quantum cosmology: An overview ⋮ Gauge invariant variables for cosmological perturbation theory using geometrical clocks ⋮ Graviton corrections to the Newtonian potential using invariant observables ⋮ Cosmological perturbations and invariant observables in geodesic lightcone coordinates

This page was built for publication: Manifestly gauge-invariant general relativistic perturbation theory: II. FRW background and first order