activity
20182025
most citedDirect Detection is testing Freeze-in

86 citations · 262 across the 8 of their papers we have counts for

collaborators

8 papers

hep-ph2025

Compact Stars as Portals to Extra-Dimensional Dark Matter

Raghuveer Garani, Chris Kouvaris, Michel H. G. Tytgat +1

We investigate hydrostatic configurations of asymmetric dark matter (DM) spheres in scenarios where fermionic DM can propagate into extra spatial dimensions, while Standard Model f…

hep-ph2023★ 8 cited

Matter-antimatter asymmetry and dark matter stability from baryon number conservation

Mar Císcar-Monsalvatje, Alejandro Ibarra, Jérôme Vandecasteele

There is currently no evidence for a baryon asymmetry in our Universe. Instead, cosmological observations have only demonstrated the existence of a quark-antiquark asymmetry, which…

hep-ph2022★ 23 cited

Condensed dark matter with a Yukawa interaction

Raghuveer Garani, Michel H. G. Tytgat, Jérôme Vandecasteele

We explore the possible phases of a condensed dark matter (DM) candidate taken to be in the form of a fermion with a Yukawa coupling to a scalar particle, at zero temperature but a…

hep-ph2019

Strong dynamics and dark matter: investigating a minimal setup

Benjamin Fuks, Federica Giacchino, Laura Lopez-Honorez +2

We discuss the phenomenology of a dark matter scenario in which we extend the Standard Model by a real scalar particle and a vector-like heavy quark. Such a model can be seen as a…

hep-ph2019★ 84 cited

Dark matter from dark photons: a taxonomy of dark matter production

Thomas Hambye, Michel H. G. Tytgat, Jérôme Vandecasteele +1

We analyse how dark matter (DM) can be produced in the early universe, working in the framework of a hidden sector charged under a U(1)' gauge symmetry and interacting with the Sta…

hep-ph2018★ 86 cited

Direct Detection is testing Freeze-in

Thomas Hambye, Michel H. G. Tytgat, Jérôme Vandecasteele +1

Dark Matter (DM) may belong to a hidden sector that is only feebly interacting with the Standard Model (SM) and may have never been in thermal equilibrium in the Early Universe. In…