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@INPROCEEDINGS{Betz:295133,
author = {Betz, M. and Caspers, F. and Gasior, M. and Thumm, M.},
title = {{S}tatus report of the {CERN} light shining through the
wall experiment with microwave axions and related aspects},
reportid = {PUBDB-2016-01081, arXiv:1204.4370},
pages = {76-81},
year = {2011},
abstract = {One way to proof or exclude the existence of axion like
particles is a microwave light shining through the wall
experiment. In this publication we will emphasize on the
engineering aspects of such a setup, currently under
development at CERN. One critical point, to achieve
meaningful results, is the electromagnetic shielding between
axion-emitter and -receiver cavity, which needs to be in the
order of 300 dB to improve over existing experimental
bounds. The RF leakage or electromagnetic crosstalk between
both cavities must be well controlled and quantified during
the complete duration of the experiment. A very narrow band
(in the $10^-6$ Hz range) homodyne detection method is used
to reveal the axion signal from background thermal noise.
The current status of the experiment is presented.},
month = {Jun},
date = {2011-06-27},
organization = {7th Patras Workshop on Axions, WIMPs
and WISPs, Mykonos (Greece), 27 Jun
2011 - 1 Jul 2011},
keywords = {background: thermal (INSPIRE) / noise: thermal (INSPIRE) /
axion (INSPIRE) / electromagnetic (INSPIRE) / microwaves
(INSPIRE) / CERN Lab (INSPIRE) / cavity (INSPIRE) / critical
phenomena (INSPIRE) / activity report (INSPIRE) /
engineering (INSPIRE) / shielding (INSPIRE)},
cin = {L},
cid = {I:(DE-H253)L-20120731},
pnm = {899 - ohne Topic (POF3-899)},
pid = {G:(DE-HGF)POF3-899},
experiment = {EXP:(DE-H253)HERA(machine)-20150101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)15},
eprint = {1204.4370},
howpublished = {arXiv:1204.4370},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1204.4370;\%\%$},
doi = {10.3204/DESY-PROC-2011-04/betz_michael},
url = {https://bib-pubdb1.desy.de/record/295133},
}