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Silicon carbide detectors for sub-GeV dark matter

Griffin, Sinéad M.; Hochberg, Yonit; Inzani, Katherine; Kurinsky, Noah; Lin, Tongyan; Yu, To Chin

Authors

Sinéad M. Griffin

Yonit Hochberg

Noah Kurinsky

Tongyan Lin

To Chin Yu



Abstract

We propose the use of silicon carbide (SiC) for direct detection of sub-GeV dark matter. SiC has properties similar to both silicon and diamond but has two key advantages: (i) it is a polar semiconductor which allows sensitivity to a broader range of dark matter candidates; and (ii) it exists in many stable polymorphs with varying physical properties and hence has tunable sensitivity to various dark matter models. We show that SiC is an excellent target to search for electron, nuclear and phonon excitations from scattering of dark matter down to 10 keV in mass, as well as for absorption processes of dark matter down to 10 meV in mass. Combined with its widespread use as an alternative to silicon in other detector technologies and its availability compared to diamond, our results demonstrate that SiC holds much promise as a novel dark matter detector.

Citation

Griffin, S. M., Hochberg, Y., Inzani, K., Kurinsky, N., Lin, T., & Yu, T. C. (2021). Silicon carbide detectors for sub-GeV dark matter. Physical Review D, 103(7), Article 075002. https://doi.org/10.1103/PhysRevD.103.075002

Journal Article Type Article
Acceptance Date Jan 5, 2021
Online Publication Date Apr 6, 2021
Publication Date Apr 1, 2021
Deposit Date Mar 19, 2025
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 103
Issue 7
Article Number 075002
DOI https://doi.org/10.1103/PhysRevD.103.075002
Public URL https://nottingham-repository.worktribe.com/output/46736051
Publisher URL https://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.075002