Results 81 to 90 of about 13,060 (254)
Cosmology with photometric redshift surveys [PDF]
We explore the utility of future photometric redshift imaging surveys for delineating the large-scale structure of the Universe, and assess the resulting constraints on the cosmological model.
Blake, Chris, Bridle, Sarah
core +4 more sources
Baryon Acoustic Oscillation Intensity Mapping of Dark Energy [PDF]
The expansion of the Universe appears to be accelerating, and the mysterious antigravity agent of this acceleration has been called "dark energy." To measure the dynamics of dark energy, baryon acoustic oscillations (BAO) can be used. Previous discussions of the BAO dark energy test have focused on direct measurements of redshifts of as many as 10(9 ...
Tzu-Ching, Chang +3 more
openaire +2 more sources
Systematic Dynamical Analysis in Palatini f(R) Gravity
This paper aims to explore the evolution of the universe in the background of Palatini f(R) gravity. Considering Amendola Gannouji Polarski Tsujikawa (AGPT) f(R) gravity model, we perform a dynamical system analysis within the FLRW universe in order to analyze the impacts of this gravity model on large‐scale structure and dynamics of universe. With the
Fizza Saeed +3 more
wiley +1 more source
We find that combined Planck cosmic microwave background, baryon acoustic oscillations, and supernovae data analyzed under Λ cold dark matter (ΛCDM) are in 4.9σ tension with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Lyα forest in ...
Keir K. Rogers, Vivian Poulin
doaj +1 more source
A model of interacting dark fluids tested with supernovae and Baryon Acoustic Oscillations data
We compare supernovae and Baryon Acoustic Oscillations data to the predictions of a cosmological model of interacting dark matter and dark energy. This theoretical model can be derived from the effective field theory of Einstein–Cartan gravity with two ...
Damien Bégué +2 more
doaj +1 more source
The sound horizon scale is a key theoretical prediction of the cosmological model that depends on the speed of sound in the baryon-photon fluid and the rate of expansion of the early Universe, before matter and radiation decoupled.
Tonghua Liu +3 more
doaj +1 more source
Analyzing the H0 tension in F(R) gravity models
The Hubble constant tension problem is analyzed in the framework of a class of modified gravity, the so-called F(R) gravity. To do so, we explore two models: an exponential and a power-law F(R) gravities, which includes an early dark energy (EDE) term in
Sergei D. Odintsov +2 more
doaj +1 more source
Theoretical uncertainty in baryon oscillations
We discuss the systematic uncertainties in the recovery of dark energy properties from the use of baryon acoustic oscillations as a standard ruler. We demonstrate that while unknown relativistic components in the universe prior to recombination would ...
D. J. Eisenstein +6 more
core +1 more source
Features of the Acoustic Mechanism of Core-Collapse Supernova Explosions [PDF]
In the context of 2D, axisymmetric, multi-group, radiation/hydrodynamic simulations of core-collapse supernovae over the full 180$^{\circ}$ domain, we present an exploration of the progenitor dependence of the acoustic mechanism of explosion.
A. Burrows +7 more
core +2 more sources
In this work, we perform a comprehensive joint analysis of three representative dark energy models—ΛCDM, the Chevallier–Polarski–Linder (CPL) parameterization, and the Generalized Emergent Dark Energy (GEDE) model—using the latest observational data sets:
Tonghua Liu, Xiaolei Li, Jieci Wang
doaj +1 more source

