activity
20242026
collaborators

5 papers

hep-ph2026

Probing Cosmic-Ray-Boosted and Supernova-Sourced Sub-GeV Dark Matter with Paleo-Detectors

Xiaoyong Chu, Yue-Lin Sming Tsai, Mei-Wen Yang

Astrophysical dark matter particles with masses well below GeV-scale can be difficult to detect using conventional nuclear recoil experiments due to their low velocities in our Mil…

hep-ph2025

From SIMP miracles to WIMP dead ends: navigating the freeze out of MeV-mass dark matter

Xiaoyong Chu, Josef Pradler

We summarize here our studies \cite{Chu:2022xuh,Chu:2023jyb,Chu:2024rrv} on two distinct scenarios for MeV-mass thermal dark matter freeze-out. First, we determine the minimal viab…

hep-ph2024

Even SIMP miracles are possible

Xiaoyong Chu, Marco Nikolic, Josef Pradler

Strongly interacting massive particles have been advocated as prominent dark matter candidates when they regulate their relic abundance through odd-numbered annih…

hep-ph2024

Dark matter bound-state formation in the Sun

Xiaoyong Chu, Raghuveer Garani, Camilo García-Cely +1

The Sun may capture asymmetric dark matter (DM), which can subsequently form bound-states through the radiative emission of a sub-GeV scalar. This process enables generation of sca…

hep-ph2024

On the minimal mass of thermal dark matter and the viability of millicharged particles affecting 21cm cosmology

Xiaoyong Chu, Josef Pradler

Thermal freeze-out offers an attractive explanation of the dark matter density free from fine-tuning of initial conditions. For dark matter with a mass below tens of MeV, photons,…