Improved constraints on the 21 cm EoR power spectrum and the X-ray heating of the IGM with HERA phase I observations

T Adams, JE Aguirre, P Alexander, ZS Ali… - The Astrophysical …, 2023 - iopscience.iop.org
We report the most sensitive upper limits to date on the 21 cm epoch of reionization power
spectrum using 94 nights of observing with Phase I of the Hydrogen Epoch of Reionization …

Measuring the reionization optical depth without large-scale CMB polarization

W Giarè, E Di Valentino, A Melchiorri - Physical Review D, 2024 - APS
We study the possibility of measuring the optical depth at reionization τ without relying on
large-scale cosmic microwave background (CMB) polarization. Our analysis is driven by the …

An effective model for the cosmic-dawn 21-cm signal

JB Muñoz - Monthly Notices of the Royal Astronomical Society, 2023 - academic.oup.com
The 21-cm signal holds the key to understanding the first structure formation during cosmic
dawn. Theoretical progress over the last decade has focused on simulations of this signal …

Cosmology before noon with multiple galaxy populations

H Ebina, M White - Journal of Cosmology and Astroparticle …, 2024 - iopscience.iop.org
Near-future facilities observing the high-redshift universe (2< z< 5) will have an opportunity
to take advantage of" multi-tracer" cosmology by observing multiple tracers of the matter …

Lower tensor-to-scalar ratio as possible signature of modified gravity

AJS Capistrano, RC Nunes, LA Cabral - Physical Review D, 2024 - APS
This paper simplifies the induced four-dimensional gravitational equations originating from a
five-dimensional bulk within the framework of Nash's embeddings, incorporating them into a …

Mitigating the optical depth degeneracy in the cosmological measurement of neutrino masses using 21-cm observations

G Shmueli, D Sarkar, ED Kovetz - Physical Review D, 2023 - APS
Massive neutrinos modify the expansion history of the universe and suppress the structure
formation below their free streaming scale. Cosmic microwave background (CMB) …

Euclid preparation

E Collaboration, T Castro, A Fumagalli, RE Angulo… - A&A, 2024 - aanda.org
The Euclid mission will measure cosmological parameters with unprecedented precision. To
distinguish between cosmological models, it is essential to generate realistic mock …

Euclid preparation. Sensitivity to neutrino parameters

M Archidiacono, J Lesgourgues, S Casas… - ar**
AM Dizgah, E Bellini, GK Keating - The Astrophysical Journal, 2024 - iopscience.iop.org
Line intensity map** (LIM) can provide a powerful means to constrain the theory of gravity
and the nature of dark energy at low and high redshifts by map** the large-scale structure …