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| 001 | 619745 | ||
| 005 | 20250801212047.0 | ||
| 024 | 7 | _ | |a Garcia-Cely:2025mgu |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:2869334 |2 inspire |
| 024 | 7 | _ | |a arXiv:2501.08382 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2024-07880 |2 datacite_doi |
| 037 | _ | _ | |a PUBDB-2024-07880 |
| 041 | _ | _ | |a English |
| 088 | _ | _ | |a DESY-25-002 |2 DESY |
| 088 | _ | _ | |a arXiv:2501.08382 |2 arXiv |
| 100 | 1 | _ | |a García-Cely, Camilo |0 P:(DE-HGF)0 |b 0 |
| 245 | _ | _ | |a Polarimetric searches for axion dark matter and high-frequency gravitational waves using optical cavities |
| 260 | _ | _ | |c 2025 |
| 336 | 7 | _ | |a Preprint |b preprint |m preprint |0 PUB:(DE-HGF)25 |s 1754048615_3349140 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a WORKING_PAPER |2 ORCID |
| 336 | 7 | _ | |a Electronic Article |0 28 |2 EndNote |
| 336 | 7 | _ | |a preprint |2 DRIVER |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a Output Types/Working Paper |2 DataCite |
| 500 | _ | _ | |a 32 pages, 8 figures |
| 520 | _ | _ | |a 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. |
| 536 | _ | _ | |a 611 - Fundamental Particles and Forces (POF4-611) |0 G:(DE-HGF)POF4-611 |c POF4-611 |f POF IV |x 0 |
| 536 | _ | _ | |a DFG project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe (390833306) |0 G:(GEPRIS)390833306 |c 390833306 |x 1 |
| 588 | _ | _ | |a Dataset connected to INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-H253)ALPS-20150101 |5 EXP:(DE-H253)ALPS-20150101 |e Any Light Particle Search |x 0 |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 1 |
| 700 | 1 | _ | |a Marsili, Luca |0 P:(DE-HGF)0 |b 1 |e Corresponding author |
| 700 | 1 | _ | |a Ringwald, Andreas |0 P:(DE-H253)PIP1001650 |b 2 |
| 700 | 1 | _ | |a Spector, Aaron D. |0 P:(DE-H253)PIP1025345 |b 3 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/619745/files/HTML-Approval_of_scientific_publication.html |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/619745/files/PDF-Approval_of_scientific_publication.pdf |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/619745/files/2501.08382v1.pdf |y OpenAccess |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/619745/files/2501.08382v1.pdf?subformat=pdfa |x pdfa |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:619745 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 2 |6 P:(DE-H253)PIP1001650 |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 3 |6 P:(DE-H253)PIP1025345 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-611 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Fundamental Particles and Forces |x 0 |
| 914 | 1 | _ | |y 2025 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a Published |0 StatID:(DE-HGF)0580 |2 StatID |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 4.0 |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |
| 920 | 1 | _ | |0 I:(DE-H253)ALPS-20130318 |k ALPS |l Any Light Particle Search |x 0 |
| 920 | 1 | _ | |0 I:(DE-H253)T-20120731 |k T |l Theorie-Gruppe |x 1 |
| 980 | _ | _ | |a preprint |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a I:(DE-H253)ALPS-20130318 |
| 980 | _ | _ | |a I:(DE-H253)T-20120731 |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | 1 | _ | |a FullTexts |
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