Dark Matter Axions Modulate Dark State Scintillation

arXiv:1709.08726 · cond-mat.str-el, cond-mat.supr-con · Submitted 2017-09-25 · Read on arXiv

cond-mat.str-el, cond-mat.supr-con

Submitted: 2017-09-25

Updated: 2026-10-15

Comments: 7 pages, 2 figures, presented at 20th Patras Workshop on Axions, WIMPs, and WISPs, 22-26 September 2025, Tenerife, Spain

License: http://creativecommons.org/licenses/by/4.0/

The gist: The decay rate of the thallium-iodine dark state in the popular alkali-halide scintillator NaI(Tl) modulates in phase with the dipole anisotropy of the cosmic microwave background (CMB), it is argued.

Terminology

Abstract

The decay rate of the thallium-iodine dark state in the popular alkali-halide scintillator NaI(Tl) modulates in phase with the dipole anisotropy of the cosmic microwave background (CMB), it is argued. Axion dark matter particles --- at rest in the local CMB rest-frame --- couple to the static magnetic field created in their rest-frame by the static electric quadrupole field within the tetragonally-distorted thallium-iodine octahedron surrounding each dark state. For axions with rest-mass energy near the roughly 0.5 eV dark state activation energy in NaI(Tl), the resulting near-infrared electric field created by this axion electrodynamic interaction modulates the dark state scintillation lifetime by bringing home the excited hole --- from the four in-plane iodine 5p orbitals that share it --- to the Tl 6s shell where it can recombine with the excited Tl 6p electron to produce the scintillation light.

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