19 citations · 31 across the 5 of their papers we have counts for
6 papers
Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions
Bryce Cyr, Nabila Aghanim, Ethan Baker +37
The frequency spectrum of the cosmic microwave background is the most precise blackbody ever measured in nature, with deviations constrained at the level of almost one part per mil…
The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures
Fereshteh Majidi, Xunyu Liang, Michael Sekatchev +2
Axion quark nuggets (AQNs) are macroscopic dark-matter candidates, with masses of the order of a few grams to a kilogram and sub-micron radius, thought to form at the Quantum Chrom…
The Glow of Axion Quark Nugget Dark Matter: (III) The Mysteries of the Milky Way UV Background
Michael Sekatchev, Xunyu Liang, Fereshteh Majidi +3
Axion quark nuggets (AQNs) are hypothetical objects with nuclear density that would have formed during the quark-hadron transition and could make up most of the dark matter today.…
The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
Julian S. Sommer, Klaus Dolag, Ludwig M. Böss +8
(abridged) We analyze the emission of axion quark nuggets in a large sample of 161 simulated galaxy clusters using the SLOW simulation. These clusters are divided into a sub-sample…
The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
Fereshteh Majidi, Xunyu Liang, Ludovic Van Waerbeke +5
Axion quark nuggets (AQNs) are hypothetical objects with a mass greater than a few grams and sub-micrometer size, formed during the quark-hadron transition. Originating from the ax…
Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
Matteo Martinelli, Roohi Dalal, Fereshteh Majidi +3
Upcoming galaxy surveys will allow us to probe the growth of the cosmic large-scale structure with improved sensitivity compared to current missions, and will also map larger areas…