Collective excitations and low-energy ionization signatures of relativistic particles in silicon detectors
Solid-state detectors with a low energy threshold have several applications, including searches of non-relativistic halo dark-matter particles with sub-GeV masses. When searching for relativistic, beyond-the-Standard-Model particles with enhanced cross sections for small energy transfers, a small detector with a low energy threshold may have better sensitivity than a larger detector with a higher energy threshold. In this paper, we calculate the low-energy ionization spectrum from high-velocity particles scattering in a dielectric material. We consider the full material response including the excitation of bulk plasmons. We generalize the energy-loss function to relativistic kinematics, and benchmark existing tools used for halo dark-matter scattering against electron energy-loss spectroscopy data. Compared to calculations commonly used in the literature, such as the Photo-Absorption-Ionization model or the free-electron model, including collective effects shifts the recoil ionization spectrum towards higher energies, typically peaking around 4-6 electron-hole pairs. We apply our results to the three benchmark examples: millicharged particles produced in a beam, neutrinos with a magnetic dipole moment produced in a reactor, and upscattered dark-matter particles. Our results show that the proper inclusion of collective effects typically enhances a detector's sensitivity to these particles, since detector backgrounds, such as dark counts, peak at lower energies.
Authors
- Aman Singal (ORCID: https://orcid.org/0000-0002-9426-1863)
- Rouven Essig (ORCID: https://orcid.org/0000-0002-3066-0486)
- Ryan Plestid (ORCID: https://orcid.org/0000-0003-0779-7289)
Institutions
- California Institute of Technology (US)
- Stony Brook University (US)
Publication Details
- Journal
- Communications Physics
- Published
- 2024-12-19
- DOI
- https://doi.org/10.1038/s42005-024-01904-2
- Citations
- 7
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 4.62
Funders
- National Science Foundation
- U.S. Department of Energy
- Simons Foundation
- Stony Brook University
- Office of Science
- Walter Burke Institute for Theoretical Physics
- High Energy Physics
- Fermilab