Non-linear general relativistic effects in the observed redshift
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Publication:5023435
DOI10.1088/1475-7516/2018/09/037OpenAlexW2804825962WikidataQ63391073 ScholiaQ63391073MaRDI QIDQ5023435
Giuseppe Fanizza, Sang Gyu Biern, Jaiyul Yoo
Publication date: 21 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1805.05959
Related Items (9)
Second-order gauge-invariant formalism for the cosmological observables: complete verification of their gauge-invariance ⋮ Covariant decomposition of the non-linear galaxy number counts and their monopole ⋮ Relativistic and non-Gaussianity contributions to the one-loop power spectrum ⋮ Synchronous coordinates and gauge-invariant observables in cosmological spacetimes ⋮ Weak lensing “post-Born” effects are equivalent to pure lens-lens couplings ⋮ Gauge invariance on the light-cone: curvature perturbations and radiative degrees of freedom ⋮ Cutting out the cosmological middle man: general relativity in the light-cone coordinates ⋮ Galaxy two-point correlation function in general relativity ⋮ The cosmological perturbation theory on the Geodesic Light-Cone background
Cites Work
- Gauge-invariant second-order perturbations and non-Gaussianity from inflation
- Relativistic effect in galaxy clustering
- Nonlinear relativistic corrections to cosmological distances, redshift and gravitational lensing magnification: II. Derivation
- Observed angles and geodesic light-cone coordinates
- Emission-angle and polarization-rotation effects in the lensed CMB
- Gauge-transformation properties of cosmological observables and its application to the light-cone average
- Light-cone observables and gauge-invariance in the geodesic light-cone formalism
- Gauge-invariance and infrared divergences in the luminosity distance
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