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@INPROCEEDINGS{Zioutas:296198,
author = {Zioutas, Konstantin and Vafeiadis, Theodoros and Tsagri,
Mary and Semertzidis, Yannis K and Papaevangelou, Thomas and
Dafni, Theopisti and Anastassopoulos, Vassilis},
title = {{S}ignatures for {S}olar {A}xions/{WISP}s},
address = {Hamburg},
publisher = {Verlag Deutsches Elektronen-Synchrotron},
reportid = {PUBDB-2016-01351, arXiv:1011.0629. DESY-PROC-2010-03},
pages = {89-94},
year = {2010},
abstract = {Standard solar physics cannot account for the X-ray
emission and other puzzles, the most striking example being
the solar corona mystery. The corona temperature rise above
the non-flaring magnetized sunspots, while the photosphere
just underneath becomes cooler, makes this mystery more
intriguing. The paradoxical Sun is suggestive of some sort
of exotic solution, axions being the (only?) choice for the
missing ingredient. We present atypical axion signatures,
which depict solar axions with a rest mass max ~17 meV/c2.
Then, the Sun has been for decades the overlooked harbinger
of new particle physics.},
month = {Jul},
date = {2010-07-05},
organization = {6th Patras Workshop on Axions, WIMPs
and WISPs, Zürich (Switzerland), 5 Jul
2010 - 9 Jul 2010},
keywords = {axion: solar (INSPIRE) / signature (INSPIRE) / new physics
(INSPIRE) / X-ray: solar (INSPIRE) / experimental results
(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 = {1011.0629},
howpublished = {arXiv:1011.0629},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1011.0629;\%\%$},
doi = {10.3204/DESY-PROC-2010-03/zioutas_konstantin},
url = {https://bib-pubdb1.desy.de/record/296198},
}