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20242026
most citedA User's Guide to Extracting Cosmological Information from Line-Intensity Maps

80 citations · 126 across the 10 of their papers we have counts for

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8 papers · 1 filter

astro-ph.CO2024

Towards a multi-tracer neutrino mass measurement with line-intensity mapping

Gali Shmueli, Sarah Libanore, Ely D. Kovetz

Accurately determining neutrino masses is a main objective of contemporary cosmology. Since massive neutrinos affect structure formation and evolution, probes of large scale struct…

astro-ph.CO2024

Early Dark Energy Effects on the 21cm Signal

Tal Adi, Jordan Flitter, Ely D. Kovetz

Early dark energy (EDE) is one of the leading models proposed to resolve the perplexing Hubble tension. Despite extensive scrutiny and testing against various observables, conclusi…

astro-ph.CO2024

Towards alleviating the and tensions with Early Dark Energy - Dark Matter drag

Théo Simon, Tal Adi, José Luis Bernal +3

Early dark energy, an additional component of dark energy active in the decade of redshift before recombination, has emerged as one of the most effective models at reducing the $H_…

astro-ph.CO2024

New Bounds on Fuzzy Dark Matter from Galaxy-Galaxy Strong-Lensing Observations

Tatyana Shevchuk, Ely D. Kovetz, Adi Zitrin

Fuzzy Dark Matter (FDM) has recently gained attention as a motivated candidate for the dark matter (DM) content of the Universe, as opposed to the commonly assumed cold DM (CDM), s…

astro-ph.CO2024

Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history

Sarah Libanore, Jordan Flitter, Ely D. Kovetz +2

Different star-formation models at Cosmic Dawn produce detectable signatures in the observables of upcoming 21-cm experiments. In this work, we consider the physical scenario of fe…

astro-ph.CO2024

Probing ultralight scalar, vector and tensor dark matter with pulsar timing arrays

Caner Unal, Federico R. Urban, Ely D. Kovetz

Pulsar timing arrays (PTAs) are sensitive to oscillations in the gravitational potential along the line-of-sight due to ultralight particle pressure. We calculate the probing power…