First results of the Laser-Interferometric Detector for Axions (LIDA)
Joscha Heinze, Alex Gill, Artemiy Dmitriev, Jiri Smetana and, Tianliang Yan, Vincent Boyer, Denis Martynov, Matthew Evans

TL;DR
This paper introduces a novel laser interferometry detector for axions, demonstrating initial sensitivity and pioneering direct detection efforts in a challenging mass range, with potential for significant sensitivity improvements.
Contribution
First experimental implementation of a laser interferometric axion detector, achieving unprecedented sensitivity and opening new avenues for direct axion searches.
Findings
Achieved a sensitivity of 1.51×10^{-10} GeV^{-1} to axion-photon coupling.
Operated at a high optical intensity of 4.7 MW/cm^2 in a high-finesse cavity.
Established the detector as one of the most sensitive in its measurement band.
Abstract
We present the operating principle and the first observing run of a novel kind of direct detector for axions and axion-like particles in the galactic halo. Sensitive to the polarisation rotation of linearly polarised laser light induced by an axion field, our experiment is the first detector of its kind collecting scientific data. We discuss our current peak sensitivity of (95 % confidence level) to the axion-photon coupling strength in the axion mass range of - which is, for instance, motivated by supersymmetric grand-unified theories. We also report on effects that arise in our high-finesse in-vacuum cavity at an unprecedented optical continuous-wave intensity of . Our detector already belongs to the most sensitive direct searches within its measurement band, and our results pave the way towards…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Pulsars and Gravitational Waves Research
