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Main Authors: Pandey, Swadha, Hall, Evan D., Evans, Matthew
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2404.12517
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author Pandey, Swadha
Hall, Evan D.
Evans, Matthew
author_facet Pandey, Swadha
Hall, Evan D.
Evans, Matthew
contents Axions and axion-like particles are strongly motivated dark matter candidates that are the subject of many current ground based dark matter searches. We present first results from the Axion Dark-Matter Birefringent Cavity (ADBC) experiment, which is an optical bow-tie cavity probing the axion-induced birefringence of electromagnetic waves. Our experiment is the first optical axion detector that is tunable and quantum noise limited, making it sensitive to a wide range of axion masses. We have iteratively probed the axion mass range 40.9-43.3$\text{ neV/c}^2$, 49.3-50.6$\text{ neV/c}^2$, and 54.4-56.7$\text{ neV/c}^2$, and found no dark matter signal. On average, we constrain the ALP-photon coupling at the level $g_{aγγ} \leq 1.9\times 10^{-8} \text{ GeV}^{-1}$. We also present prospects for future axion dark matter detection experiments using optical cavities.
format Preprint
id arxiv_https___arxiv_org_abs_2404_12517
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle First results from the Axion Dark-Matter Birefringent Cavity (ADBC) experiment
Pandey, Swadha
Hall, Evan D.
Evans, Matthew
High Energy Physics - Experiment
Cosmology and Nongalactic Astrophysics
Axions and axion-like particles are strongly motivated dark matter candidates that are the subject of many current ground based dark matter searches. We present first results from the Axion Dark-Matter Birefringent Cavity (ADBC) experiment, which is an optical bow-tie cavity probing the axion-induced birefringence of electromagnetic waves. Our experiment is the first optical axion detector that is tunable and quantum noise limited, making it sensitive to a wide range of axion masses. We have iteratively probed the axion mass range 40.9-43.3$\text{ neV/c}^2$, 49.3-50.6$\text{ neV/c}^2$, and 54.4-56.7$\text{ neV/c}^2$, and found no dark matter signal. On average, we constrain the ALP-photon coupling at the level $g_{aγγ} \leq 1.9\times 10^{-8} \text{ GeV}^{-1}$. We also present prospects for future axion dark matter detection experiments using optical cavities.
title First results from the Axion Dark-Matter Birefringent Cavity (ADBC) experiment
topic High Energy Physics - Experiment
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2404.12517