Journal Article PUBDB-2025-00177

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Polarimetric searches for axion dark matter and high-frequency gravitational waves using optical cavities

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2025
American Physical Society Ridge, NY

Physical review / D 112(2), 023031 () [10.1103/26vg-wcfx]
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Report No.: DESY-25-002; arXiv:2501.08382

Abstract: We revisit birefringence effects associated with the evolution of the polarization of light as it propagates through axion dark matter or the background of a passing gravitational wave (GW). We demonstrate that this can be described by a unified formalism, highlighting a synergy between searches for axions and high-frequency GWs. We show that by exploiting this framework, the optical cavities used by the ALPS II experiment can potentially probe axion masses in the range $m_a \sim 10^{-9} - 10^{-6} \, \mathrm{eV}$, offering competitive sensitivity with existing laboratory and astrophysical searches. Also building on this approach, we propose using these optical cavities to search for high-frequency GWs by measuring changes in the polarization of their laser. This makes it a promising method for exploring, in the near future, GWs with frequencies above $100$ MHz and strain sensitivities on the order of $10^{-14} \, \mathrm{Hz}^{-1/2}$. Such sensitivity allows the exploration of currently unconstrained parameter space, complementing other high-frequency GW experiments. This work contributes to the growing community investigating novel approaches for high-frequency GW detection.

Classification:

Note: 32 pages, 8 figures

Contributing Institute(s):
  1. Any Light Particle Search (ALPS)
  2. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. DFG project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe (390833306) (390833306)
  3. DFG project G:(GEPRIS)491245950 - Open-Access-Publikationskosten / 2025-2027 / DESY Hamburg (491245950) (491245950)
Experiment(s):
  1. Any Light Particle Search
  2. No specific instrument

Appears in the scientific report 2025
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Polarimetric searches for axion dark matter and high-frequency gravitational waves using optical cavities
[10.3204/PUBDB-2024-07880]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2025-01-14, last modified 2025-08-06