activity
20052026
most citedA facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case

782 citations · 6.5k across the 78 of their papers we have counts for

collaborators

82 papers

hep-ph2026

Improved Big Bang Nucleosynthesis constraints on decaying massive relics

Sara Bianco, Jonas Frerick, Marco Hufnagel +1

We present updated and improved Big Bang Nucleosynthesis (BBN) constraints on heavy, long-lived beyond the Standard Model (BSM) relics decaying into pairs of Standard Model par…

astro-ph.IM2026

The Cosmological Simulation Code OpenGadget3 - Implementation of Self-Interacting Dark Matter

Moritz S. Fischer, Marc Wiertel, Cenanda Arido +7

Dark matter (DM) could be subject to non-gravitational self-interactions which is relevant to resolve potential problems of cold DM on small scales. Their impact on astrophysical o…

hep-ph2026

Tuning the violins: dark sector phase transition models for the PTA signal

Torsten Bringmann, Thomas Konstandin, Jonas Matuszak +2

First-order phase transitions in a dark sector have been invoked as an intriguing possibility to explain the observed stochastic gravitational wave background at nanohertz frequenc…

astro-ph.CO2025

Accretion of self-interacting dark matter onto supermassive black holes

V. M. Sabarish, Marcus Brüggen, Kai Schmidt-Hoberg +1

Dark matter (DM) spikes around supermassive black holes (SMBHs) may lead to interesting physical effects such as enhanced DM annihilation signals or dynamical friction within binar…

hep-ph2025

Photo- and Hadrodisintegration constraints on massive relics decaying into neutrinos

Sara Bianco, Paul Frederik Depta, Jonas Frerick +3

We perform a detailed study of the cosmological constraints on the decay of a relic particle into neutrinos, , in particular those arising from the observe…

hep-ph2024

Early Matter Domination at Colliders: Long Live the Glueball!

Fady Bishara, Filippo Sala, Kai Schmidt-Hoberg

We prove that collider searches for long-lived particles (LLPs) can test the dynamics responsible for matter domination in the early universe. In this letter we concentrate on the…