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@ARTICLE{Egge:631956,
author = {Egge, Jacob and Meyer, Manuel},
title = {{S}ensitivity of a {G}igahertz {F}abry-{P}érot {R}esonator
for {A}xion {D}ark {M}atter {D}etection},
reportid = {PUBDB-2025-02071, arXiv:2506.03091},
year = {2025},
note = {10 pages, 8 figures, 1 table. Submitted},
abstract = {Axions are hypothetical pseudo-Nambu Goldstone bosons that
could explain the observed cold dark matter density and
solve the strong CP problem of quantum chromodynamics (QCD).
Haloscope experiments commonly employ resonant cavities to
search for a conversion of axion dark matter into photons in
external magnetic fields. As the expected signal power
degrades with increasing frequency, this approach becomes
challenging at frequencies beyond tens of Gigahertz. Here,
we propose a novel haloscope design based on an open
Fabry-Pérot resonator. Operating a small-scale resonator at
cryogenic temperatures and at modest magnetic fields should
already lead to an unparalleled sensitivity for photon-axion
couplings $g_{aγ} \gtrsim
3\times10^{-12}\,\mathrm{GeV}^{-1}$ at 35GHz. We demonstrate
how this sensitivity could be further improved using
graded-phase mirrors and sketch possibilities to probe
benchmark models of the QCD axion.},
cin = {ALPS},
cid = {I:(DE-H253)ALPS-20130318},
pnm = {611 - Fundamental Particles and Forces (POF4-611) / DFG
project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe
(390833306) / AxionDM - Searching for axion and
axion-like-particle dark matter in the laboratory and with
high-energy astrophysical observations (948689)},
pid = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306 /
G:(EU-Grant)948689},
experiment = {EXP:(DE-H253)ALPS-20150101},
typ = {PUB:(DE-HGF)25},
eprint = {2506.03091},
howpublished = {arXiv:2506.03091},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2506.03091;\%\%$},
url = {https://bib-pubdb1.desy.de/record/631956},
}