Holographic dark energy
We review the paradigm of holographic dark energy (HDE), which arises from a theoretical
attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making …
attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making …
Observational probes of cosmic acceleration
The accelerating expansion of the universe is the most surprising cosmological discovery in
many decades, implying that the universe is dominated by some form of “dark energy” with …
many decades, implying that the universe is dominated by some form of “dark energy” with …
Constraining early dark energy with large-scale structure
An axion-like field comprising∼ 10% of the energy density of the Universe near matter-
radiation equality is a candidate to resolve the Hubble tension; this is the “early dark …
radiation equality is a candidate to resolve the Hubble tension; this is the “early dark …
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space
We investigate the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey
(BOSS) Data Release 12 sample, which consists of 1198 006 galaxies in the redshift range …
(BOSS) Data Release 12 sample, which consists of 1198 006 galaxies in the redshift range …
The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1
We perform a joint determination of the distance–redshift relation and cosmic expansion rate
at redshifts z= 0.44, 0.6 and 0.73 by combining measurements of the baryon acoustic peak …
at redshifts z= 0.44, 0.6 and 0.73 by combining measurements of the baryon acoustic peak …
Nonlinear perturbation theory extension of the Boltzmann code CLASS
We present a new open-source code that calculates one-loop power spectra and cross
spectra for matter fields and biased tracers in real and redshift space. These spectra …
spectra for matter fields and biased tracers in real and redshift space. These spectra …
Large-scale structure of the Universe and cosmological perturbation theory
F Bernardeau, S Colombi, E Gaztanaga… - Physics reports, 2002 - Elsevier
We review the formalism and applications of non-linear perturbation theory (PT) to
understanding the large-scale structure of the Universe. We first discuss the dynamics of …
understanding the large-scale structure of the Universe. We first discuss the dynamics of …
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: testing gravity with redshift space distortions using the power spectrum multipoles
We analyse the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey
(BOSS) CMASS Data Release 11 (DR11) sample, which consists of 690 827 galaxies in the …
(BOSS) CMASS Data Release 11 (DR11) sample, which consists of 690 827 galaxies in the …
The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at z ∼ 1.4
We measure the redshift-space correlation function from a spectroscopic sample of 2783
emission line galaxies from the FastSound survey. The survey, which uses the Subaru …
emission line galaxies from the FastSound survey. The survey, which uses the Subaru …
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z = 0.57 from …
We analyse the anisotropic clustering of massive galaxies from the Sloan Digital Sky Survey
III Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 9 (DR9) sample, which …
III Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 9 (DR9) sample, which …