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Improved constraints on the 21 cm EoR power spectrum and the X-ray heating of the IGM with HERA phase I observations
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 …
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
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 …
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 …
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 …
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
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 …
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
Massive neutrinos modify the expansion history of the universe and suppress the structure
formation below their free streaming scale. Cosmic microwave background (CMB) …
formation below their free streaming scale. Cosmic microwave background (CMB) …
Euclid preparation
The Euclid mission will measure cosmological parameters with unprecedented precision. To
distinguish between cosmological models, it is essential to generate realistic mock …
distinguish between cosmological models, it is essential to generate realistic mock …
Euclid preparation. Sensitivity to neutrino parameters
M Archidiacono, J Lesgourgues, S Casas… - ar**
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 …
and the nature of dark energy at low and high redshifts by map** the large-scale structure …