activity
20172026
most citedThe Dawn of FIMP Dark Matter: A Review of Models and Constraints

532 citations · 1.4k across the 28 of their papers we have counts for

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Showing 2026Show all

9 papers · 1 filter

astro-ph.CO2026

The Loud Tail of the Supermassive Black Hole Binary Population: Multimessenger Candidates and Prospects for SKAO

Juhan Raidal, Ville Vaskonen, Juan Urrutia +1

We assess whether electromagnetically identified supermassive black hole (SMBH) binary candidates populate the rare, high-amplitude tail of the gravitational wave (GW) amplitude di…

hep-ex2026

Technical Proposal for the Atom Interferometer CERN Experiment (AICE) Facility

Gianluigi Arduini, Nadja Augst, Mark G. Bason +79

We present the technical proposal for the Atom Interferometer CERN Experiment (AICE), a m vertical atom interferometer to be installed against the wall of the PX…

hep-ph2026

Axion Misalignment Across First-Order Phase Transitions

Galymzhan Baltabay, Francesco D'Eramo, Ville Vaskonen

When the axion mass is generated during a first-order phase transition and becomes non-vanishing only inside expanding true-vacuum bubbles, the standard picture of misalignment pro…

astro-ph.CO2026

Constraints on primordial black holes from the first part of LIGO-Virgo-KAGRA fourth observing run

M. Andrés-Carcasona, A. J. Iovino, E. Vallejo-Pagès +4

We analyse primordial black hole (PBH) populations using state-of-the-art modelling of PBH binaries, deriving the strongest bounds on PBH abundance in the - rang…

astro-ph.CO2026

JWST Constraints on Primordial Magnetic Fields

Malcolm Fairbairn, María Olalla Olea-Romacho, Juan Urrutia +1

Primordial magnetic fields (PMFs) enhance small-scale structure formation through the Lorentz force acting on baryons, boosting the abundance of low-mass halos and their hosted gal…

astro-ph.CO2026

The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background

Juhan Raidal, Juan Urrutia, Ville Vaskonen +1

We study the non-Gaussian features of the gravitational wave (GW) background generated by a population of inspiraling supermassive black hole (SMBH) binaries. We show that the SMBH…