Cosmology with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …
cosmological focus: to probe the expansion rate of the universe, and to understand …
New horizons for fundamental physics with LISA
KG Arun, E Belgacem, R Benkel, L Bernard… - Living Reviews in …, 2022 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders
about the fundamental theory of nature at play in the extreme gravity regime, where the …
about the fundamental theory of nature at play in the extreme gravity regime, where the …
In the realm of the Hubble tension—a review of solutions
The simplest ΛCDM model provides a good fit to a large span of cosmological data but
harbors large areas of phenomenology and ignorance. With the improvement of the number …
harbors large areas of phenomenology and ignorance. With the improvement of the number …
Footprints of the QCD crossover on cosmological gravitational waves at pulsar timing arrays
Pulsar timing arrays (PTAs) have reported evidence for a stochastic gravitational wave (GW)
background at nanohertz frequencies, possibly originating in the early Universe. We show …
background at nanohertz frequencies, possibly originating in the early Universe. We show …
Euclid preparation-i. the euclid wide survey
R Scaramella, J Amiaux, Y Mellier, C Burigana… - Astronomy & …, 2022 - aanda.org
Euclid is a mission of the European Space Agency that is designed to constrain the
properties of dark energy and gravity via weak gravitational lensing and galaxy clustering. It …
properties of dark energy and gravity via weak gravitational lensing and galaxy clustering. It …
On the evolution of the Hubble constant with the SNe Ia pantheon sample and baryon acoustic oscillations: a feasibility study for GRB-cosmology in 2030
MG Dainotti, B De Simone, T Schiavone, G Montani… - Galaxies, 2022 - mdpi.com
The difference from 4 to 6 σ in the Hubble constant (H 0) between the values observed with
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …
Modified gravity and cosmology
The dawn of the twenty-first century came with very positive prospects for gravity, cosmology,
and astrophysics. Technological progress made it possible for cosmology to enter to its …
and astrophysics. Technological progress made it possible for cosmology to enter to its …
The Karl G. Jansky very large array sky survey (VLASS). Science case and survey design
M Lacy, SA Baum, CJ Chandler… - Publications of the …, 2020 - iopscience.iop.org
Abstract The Very Large Array Sky Survey (VLASS) is a synoptic, all-sky radio sky survey
with a unique combination of high angular resolution (≈ 2 farcs 5), sensitivity (a 1σ goal of …
with a unique combination of high angular resolution (≈ 2 farcs 5), sensitivity (a 1σ goal of …
Planck 2018 results-I. Overview and the cosmological legacy of Planck
N Aghanim, Y Akrami, F Arroja, M Ashdown… - Astronomy & …, 2020 - aanda.org
The European Space Agency's Planck satellite, which was dedicated to studying the early
Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the …
Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the …
Constraints on multifield inflation from the BOSS galaxy survey
We use redshift-space galaxy clustering data from the BOSS survey to constrain local
primordial non-Gaussianity (LPNG). This is of particular importance due to the consistency …
primordial non-Gaussianity (LPNG). This is of particular importance due to the consistency …