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Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …
description of a wide range of astrophysical and cosmological data. However, there are a …
[HTML][HTML] String cosmology: From the early universe to today
We review applications of string theory to cosmology, from primordial times to the present-
day accelerated expansion. Starting with a brief overview of cosmology and string …
day accelerated expansion. Starting with a brief overview of cosmology and string …
DESI 2024 VI: Cosmological constraints from the measurements of baryon acoustic oscillations
We present cosmological results from the measurement of baryon acoustic oscillations
(BAO) in galaxy, quasar and Lyman-α forest tracers from the first year of observations from …
(BAO) in galaxy, quasar and Lyman-α forest tracers from the first year of observations from …
Validation of the scientific program for the Dark Energy Spectroscopic Instrument
Abstract The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a
survey covering 14,000 deg 2 over 5 yr to constrain the cosmic expansion history through …
survey covering 14,000 deg 2 over 5 yr to constrain the cosmic expansion history through …
Overview of the instrumentation for the dark energy spectroscopic instrument
The goal of the Dark Energy Spectroscopic Instrument (DESI) is to determine the nature of
dark energy through the most precise measurement of the expansion history of the universe …
dark energy through the most precise measurement of the expansion history of the universe …
Is the observable Universe consistent with the cosmological principle?
The cosmological principle (CP)—the notion that the Universe is spatially isotropic and
homogeneous on large scales—underlies a century of progress in cosmology. It is …
homogeneous on large scales—underlies a century of progress in cosmology. It is …
A Tale of Many H0
▪ The Hubble parameter, H 0, is not an univocally defined quantity: It relates redshifts to
distances in the near Universe, but it is also a key parameter of the ΛCDM standard …
distances in the near Universe, but it is also a key parameter of the ΛCDM standard …
Challenges for ΛCDM: An update
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …
few years as the accuracy of cosmological observations improves. In this review we discuss …
DESI 2024 IV: Baryon acoustic oscillations from the Lyman alpha forest
We present the measurement of Baryon Acoustic Oscillations (BAO) from the Lyman-α (Lyα)
forest of high-redshift quasars with the first-year dataset of the Dark Energy Spectroscopic …
forest of high-redshift quasars with the first-year dataset of the Dark Energy Spectroscopic …
Target selection and validation of DESI luminous red galaxies
Abstract The Dark Energy Spectroscopic Instrument (DESI) is carrying out a five-year survey
that aims to measure the redshifts of tens of millions of galaxies and quasars, including 8 …
that aims to measure the redshifts of tens of millions of galaxies and quasars, including 8 …