Beyond the cosmological standard model

A Joyce, B Jain, J Khoury, M Trodden - Physics Reports, 2015 - Elsevier
After a decade and a half of research motivated by the accelerating universe, theory and
experiment have reached a certain level of maturity. The development of theoretical models …

Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

K Bamba, S Capozziello, S Nojiri… - Astrophysics and Space …, 2012 - Springer
We review different dark energy cosmologies. In particular, we present the Λ CDM
cosmology, Little Rip and Pseudo-Rip universes, the phantom and quintessence …

Hints, neutrino bounds, and WDM constraints from SDSS DR14 Lyman-α and Planck full-survey data

N Palanque-Delabrouille, C Yèche… - … of Cosmology and …, 2020 - iopscience.iop.org
The Lyman-α forest 1D flux power spectrum is a powerful probe of several cosmological
parameters. Assuming a ΛCDM cosmology including massive neutrinos, we find that the …

The DESI experiment part I: science, targeting, and survey design

A Aghamousa, J Aguilar, S Ahlen, S Alam… - arXiv preprint arXiv …, 2016 - arxiv.org
DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy
experiment that will study baryon acoustic oscillations (BAO) and the growth of structure …

Evolving embedded traversable wormholes in f (R, G) gravity: a comparative study

T Naz, A Malik, MK Asif, I Fayyaz - Physics of the Dark Universe, 2023 - Elsevier
The objective of this paper is to unveil the evolving traversable wormhole solutions within
the perspective of modified f (R, G) gravity, where R is Ricci scalar and G is Gauss Bonnet …

Observational constraining study of new deceleration parameters in frw universe

A Bouali, H Chaudhary, S Mumtaz… - Fortschritte der …, 2023 - Wiley Online Library
In the current paper, a dark energy (DE) model reconstructed from the well‐motivated
deceleration parameter (DP) q (z)= q 0+ q 1 z/(1+ z) 2 q(z)=q_0+q_1z/(1+z)^2 is analyzed. A …

Neutrino mass ordering from oscillations and beyond: 2018 status and future prospects

PF De Salas, S Gariazzo, O Mena… - Frontiers in Astronomy …, 2018 - frontiersin.org
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor
physics, and its determination may provide the key to establish the relationship among the …

The evolution of the intergalactic medium

M McQuinn - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
The bulk of cosmic matter resides in a dilute reservoir that fills the space between galaxies,
the intergalactic medium (IGM). The history of this reservoir is intimately tied to the cosmic …

Robust preference for Dynamical Dark Energy in DESI BAO and SN measurements

W Giarè, M Najafi, S Pan, E Di Valentino… - … of Cosmology and …, 2024 - iopscience.iop.org
Abstract Recent Baryon Acoustic Oscillation (BAO) measurements released by DESI, when
combined with Cosmic Microwave Background (CMB) data from Planck and two different …

Inflation, the Hubble tension, and early dark energy: An alternative overview

W Giarè - Physical Review D, 2024 - APS
I review and discuss the possible implications for inflation resulting from considering new
physics in light of the Hubble tension. My study is motivated by a simple argument that the …