Light Magnetic Dipole-Coupled Dark Matter
APA
Trickle, T. (2025). Light Magnetic Dipole-Coupled Dark Matter. Perimeter Institute. https://pirsa.org/25110077
MLA
Trickle, Tanner. Light Magnetic Dipole-Coupled Dark Matter. Perimeter Institute, Nov. 18, 2025, https://pirsa.org/25110077
BibTex
@misc{ pirsa_PIRSA:25110077,
doi = {10.48660/25110077},
url = {https://pirsa.org/25110077},
author = {Trickle, Tanner},
keywords = {Particle Physics},
language = {en},
title = {Light Magnetic Dipole-Coupled Dark Matter},
publisher = {Perimeter Institute},
year = {2025},
month = {nov},
note = {PIRSA:25110077 see, \url{https://pirsa.org}}
}
Abstract
The past decade has seen rapid advancement in electron excitation-based direct detection experiments, which target light, MeV-GeV mass dark matter. Recently, the DAMIC-M collaboration began to probe the benchmark light dark matter models, renewing questions about the broader range of dark matter models these experiments can detect, and the necessity of new experiments to search beyond. In this talk we'll discuss a novel mechanism to cosmologically produce light, keV-GeV mass, dark matter coupled to electrons via a magnetic dipole moment. We consider a minimally extended dark sector in which only heavier states are charged under the kinetically mixed dark photon. These states are produced via freeze-in and subsequently thermalize the rest of the dark sector, efficiently populating the lighter, neutral, magnetic dipole-coupled dark matter. Finally, we'll discuss how magnons, collective excitations of spin waves, can be used to search for keV-MeV mass magnetic dipole-coupled dark matter, outside the reach of any semiconductor based direct detection technology.