The cosmological perturbation theory on the Geodesic Light-Cone background
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Publication:5027426
DOI10.1088/1475-7516/2021/02/014zbMath1484.83114arXiv2009.14134OpenAlexW3090572420MaRDI QIDQ5027426
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Publication date: 4 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2009.14134
Relativistic cosmology (83F05) Singular perturbations in context of PDEs (35B25) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15)
Related Items (6)
Gauge invariants of linearized gravity with a general background metric ⋮ Synchronous coordinates and gauge-invariant observables in cosmological spacetimes ⋮ The gauge invariant cosmological Jacobi map from weak lensing at leading order ⋮ Gauge invariance on the light-cone: curvature perturbations and radiative degrees of freedom ⋮ Cosmological perturbations and invariant observables in geodesic lightcone coordinates ⋮ Linearized propagation equations for metric fluctuations in a general (non-vacuum) background geometry
Cites Work
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- How does the cosmic large-scale structure bias the Hubble diagram?
- Light-cone observables and gauge-invariance in the geodesic light-cone formalism
- Gauge-invariance and infrared divergences in the luminosity distance
- Generalized covariant prescriptions for averaging cosmological observables
- Cutting out the cosmological middle man: general relativity in the light-cone coordinates
- Observation angles, Fermi coordinates, and the Geodesic-Light-Cone gauge
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