Isolating relativistic effects in large-scale structure
From MaRDI portal
Publication:2936160
DOI10.1088/0264-9381/31/23/234002zbMath1306.83059arXiv1409.2224OpenAlexW2119457133WikidataQ63391043 ScholiaQ63391043MaRDI QIDQ2936160
Publication date: 5 January 2015
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1409.2224
Applications of statistics to physics (62P35) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (10)
Dark energy homogeneity in general relativity: Are we applying it correctly? ⋮ General relativistic cosmological N-body simulations. Part I. Time integration ⋮ Probing beyond-Horndeski gravity on ultra-large scales ⋮ Relativistic effects in the large-scale structure with effective dark energy fluids ⋮ Modeling relativistic contributions to the halo power spectrum dipole ⋮ Fluctuating dark energy and the luminosity distance ⋮ Imprints of local lightcone projection effects on the galaxy bispectrum IV: second-order vector and tensor contributions ⋮ Observed galaxy power spectrum in cubic Galileon model ⋮ Relativistic cosmological large scale structures at one-loop ⋮ The flat sky approximation to galaxy number counts
This page was built for publication: Isolating relativistic effects in large-scale structure
