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Main Authors: Kondo, Dan, Morimoto, Takahiro, Osaki, Genta, Sichanugrist, Thanaporn
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2505.17007
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author Kondo, Dan
Morimoto, Takahiro
Osaki, Genta
Sichanugrist, Thanaporn
author_facet Kondo, Dan
Morimoto, Takahiro
Osaki, Genta
Sichanugrist, Thanaporn
contents We propose a novel method to detect axion dark matter based on a topological phenomenon known as the shift current. We exploit the second-order nonlinearity of the shift current by applying a strong oscillating electric field. This field enhances the axion-induced shift current signal and downconverts its frequency to a more accessible range. The non-dissipative nature of the shift current allows us to achieve broadband detection via difference frequency generation. We demonstrate, using Type-I Weyl semimetal TaAs property, the possibility of probing the parameter space of the QCD axion in the mass range of $\mathcal{O}(10)$ - $\mathcal{O}(100) \ \rm meV$ corresponding to the photon coupling of $g_{aγγ}\simeq$ $\mathcal{O}(10^{-12})$ - $\mathcal{O}(10^{-11})~\text{GeV}^{-1}$, respectively.
format Preprint
id arxiv_https___arxiv_org_abs_2505_17007
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Broadband Search for Axion Dark Matter via Shift Current
Kondo, Dan
Morimoto, Takahiro
Osaki, Genta
Sichanugrist, Thanaporn
High Energy Physics - Phenomenology
We propose a novel method to detect axion dark matter based on a topological phenomenon known as the shift current. We exploit the second-order nonlinearity of the shift current by applying a strong oscillating electric field. This field enhances the axion-induced shift current signal and downconverts its frequency to a more accessible range. The non-dissipative nature of the shift current allows us to achieve broadband detection via difference frequency generation. We demonstrate, using Type-I Weyl semimetal TaAs property, the possibility of probing the parameter space of the QCD axion in the mass range of $\mathcal{O}(10)$ - $\mathcal{O}(100) \ \rm meV$ corresponding to the photon coupling of $g_{aγγ}\simeq$ $\mathcal{O}(10^{-12})$ - $\mathcal{O}(10^{-11})~\text{GeV}^{-1}$, respectively.
title Broadband Search for Axion Dark Matter via Shift Current
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2505.17007