English

Directional Detectability of Dark Matter With Single Phonon Excitations: Target Comparison

High Energy Physics - Phenomenology 2022-01-12 v2 Cosmology and Nongalactic Astrophysics Materials Science

Abstract

Single phonon excitations are sensitive probes of light dark matter in the keV-GeV mass window. For anisotropic target materials, the signal depends on the direction of the incoming dark matter wind and exhibits a daily modulation. We discuss in detail the various sources of anisotropy, and carry out a comparative study of 26 crystal targets, focused on sub-MeV dark matter benchmarks. We compute the modulation reach for the most promising targets, corresponding to the cross section where the daily modulation can be observed for a given exposure, which allows us to combine the strength of DM-phonon couplings and the amplitude of daily modulation. We highlight Al2_2O3_3 (sapphire), CaWO4_4 and h-BN (hexagonal boron nitride) as the best polar materials for recovering a daily modulation signal, which feature O(1100)%\mathcal{O}(1 - 100)\% variations of detection rates throughout the day, depending on the dark matter mass and interaction. The directional nature of single phonon excitations offers a useful handle to mitigate backgrounds, which is crucial for fully realizing the discovery potential of near future experiments.

Keywords

Cite

@article{arxiv.2102.09567,
  title  = {Directional Detectability of Dark Matter With Single Phonon Excitations: Target Comparison},
  author = {Ahmet Coskuner and Tanner Trickle and Zhengkang Zhang and Kathryn M. Zurek},
  journal= {arXiv preprint arXiv:2102.09567},
  year   = {2022}
}

Comments

13 pages, 11 figures; updated to match published version