Light-cone observables and gauge-invariance in the geodesic light-cone formalism

DOI10.1088/1475-7516/2017/06/007OpenAlexW3104495220WikidataQ63390994 ScholiaQ63390994MaRDI QIDQ5024197

Fulvio Scaccabarozzi, Jaiyul Yoo

Publication date: 28 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1703.08552

zbMATH Keywords

gravitygravitational lensingcosmological perturbation theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (8)

Second-order gauge-invariant formalism for the cosmological observables: complete verification of their gauge-invariance ⋮ Observed angles and geodesic light-cone coordinates ⋮ Cosmological information contents on the light-cone ⋮ The gauge invariant cosmological Jacobi map from weak lensing at leading order ⋮ The Hawking energy in a perturbed Friedmann-Lemaître universe ⋮ Non-linear general relativistic effects in the observed redshift ⋮ Galaxy two-point correlation function in general relativity ⋮ The cosmological perturbation theory on the Geodesic Light-Cone background

Cites Work

• Relativistic effect in galaxy clustering
• Corrigendum: The luminosity distance–redshift relation up to second order in the Poisson gauge with anisotropic stress (2015 Class. Quantum Grav. 32 045004)
• How does the cosmic large-scale structure bias the Hubble diagram?
• Gauge-invariance and infrared divergences in the luminosity distance

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