pith. machine review for the scientific record. sign in

arxiv: 1712.06598 · v2 · submitted 2017-12-18 · ✦ hep-ph · astro-ph.CO· hep-ex

Recognition: unknown

Detection of Light Dark Matter With Optical Phonons in Polar Materials

Authors on Pith no claims yet
classification ✦ hep-ph astro-ph.COhep-ex
keywords darkmatterphononsdetectionexcellentgaasmaterialsoptical
0
0 comments X
read the original abstract

We show that polar materials are excellent targets for direct detection of sub-GeV dark matter due to the presence of gapped optical phonons as well as acoustic phonons with high sound speed. We take the example of Gallium Arsenide (GaAs), which has the properties needed for experimental realization, and where many results can be estimated analytically. We find GaAs has excellent reach to dark photon absorption, can completely cover the freeze-in benchmark for scattering via an ultralight dark photon, and is competitive with other proposals to detect sub-MeV dark matter scattering off nuclei.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Electronic Direct Detection of Light Dark Matter with Intermediate-Mass Mediators

    hep-ph 2026-05 unverdicted novelty 5.0

    For sub-GeV dark matter, the light and heavy mediator mass limits in direct detection are separated by up to three orders of magnitude in mediator mass, enabling precise sensitivity calculations for Si, Ge, and DAMIC-...

  2. Dive deeper with SUBMARINE: SUB-Mev dArk matter diRect detectIon using bilayer grapheNE

    hep-ph 2026-04 unverdicted novelty 5.0

    Bilayer graphene enables sub-MeV dark matter detection via electronic excitations with small exposure and sidereal modulation signatures.

  3. Extracting Dark-Matter Mass from Angular Scanning

    hep-ph 2026-04 unverdicted novelty 5.0

    Curvature of the angular spectrum of dark matter events in directional 2D detectors encodes the dark matter mass scale.