collaborators

6 papers

astro-ph.CO2026

Reionization, UV Luminosity and 21cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses

Gaétan Facchinetti, Alexander Korochkin, Laura Lopez-Honorez +1

Magnetic fields with field strengths between G and a few Nanogauss are expected to exist today in the intergalactic medium (IGM). Their origin is unknown, but may be of…

astro-ph.CO2026

Non-Cold Dark Matter from Memory-Burdened Primordial Black Holes

Valentin Thoss, Laura Lopez-Honorez, Florian Kühnel +1

Non-cold dark matter particles can arise from the evaporation of primordial black holes (PBHs). In this paper, we further investigate how the memory-burden effect, which delays the…

hep-ph2026

Minimal Dark Matter: Generalized Framework and Direct-Detection Sensitivity

Spencer Griffith, Juri Smirnov, Laura Lopez-Honorez +1

Minimal electroweak dark matter models are compelling due to their simplicity, though calculations of their freezeout abundance are complicated by nonperturbative effects due to So…

astro-ph.CO2026

Constraining long-lived dark sector particles with CMB and Lyman-

Laura Lopez-Honorez, Sonali Verma

We use measurements of the intergalactic medium (IGM) temperature from the Lyman- forest to place new limits on models in which long-lived dark sector (DS) particles, with life…

astro-ph.CO2025

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter

Virgile Dandoy, Christian Döring, Gaétan Facchinetti +2

The cm signal originating from Cosmic Dawn to the Epoch of Reionisation is highly sensitive to the processes governing star formation in the early universe as well as new phy…

hep-ph2025

t-channel dark matter at the LHC -- a whitepaper

Chiara Arina, Benjamin Fuks, Luca Panizzi +67

This report, summarising work achieved in the context of the LHC Dark Matter Working Group, investigates the phenomenology of -channel dark matter models, spanning minimal setup…