The Hawking energy in a perturbed Friedmann-Lemaître universe
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Publication:6094198
DOI10.1088/1475-7516/2023/08/033arXiv2305.00711OpenAlexW4385814209MaRDI QIDQ6094198
Enea Di Dio, Ruth Durrer, Dennis Stock
Publication date: 13 September 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.00711
cosmological perturbation theoryquasi-local energylight deflectioncosmic background radiationHawking energy
Relativistic cosmology (83F05) Gravitational energy and conservation laws; groups of motions (83C40)
Cites Work
- Quasi-local energy-momentum and angular momentum in general relativity
- Anisotropies in the cosmic microwave background: Theoretical foundations
- The magnitude–redshift relation in a perturbed Friedmann universe
- The luminosity distance–redshift relation up to second order in the Poisson gauge with anisotropic stress
- Galaxy two-point correlation function in general relativity
- Light-cone observables and gauge-invariance in the geodesic light-cone formalism
- The Hawking energy on the past lightcone in cosmology
- Applications of the Hawking energy on lightcones in cosmology
- The observed galaxy power spectrum in General Relativity
- General Relativity
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