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.

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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

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article

Collective excitations and low-energy ionization signatures of relativistic particles in silicon detectors

Aman Singal, Rouven Essig, Ryan Plestid
7 citations
Communications Physics
Dark Matter and Cosmic Phenomena
4.62
article

Collective excitations and low-energy ionization signatures of relativistic particles in silicon detectors

Aman Singal, Rouven Essig, Ryan Plestid
article en
7 citations

Abstract

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.

Communications PhysicsVol. 7(1)
California Institute of Technology (US), Stony Brook University (US)
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
Affordable and clean energy
Openalex Percentile: Top 4%
Dark Matter and Cosmic Phenomena
4.62
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