TY  - CONF
AU  - Zioutas, Konstantin
AU  - Vafeiadis, Theodoros
AU  - Tsagri, Mary
AU  - Semertzidis, Yannis K
AU  - Papaevangelou, Thomas
AU  - Dafni, Theopisti
AU  - Anastassopoulos, Vassilis
TI  - Signatures for Solar Axions/WISPs
IS  - arXiv:1011.0629
CY  - Hamburg
PB  - Verlag Deutsches Elektronen-Synchrotron
M1  - PUBDB-2016-01351
M1  - arXiv:1011.0629
M1  - DESY-PROC-2010-03
SP  - 89-94
PY  - 2010
AB  - 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.
T2  - 6th Patras Workshop on Axions, WIMPs and WISPs
CY  - 5 Jul 2010 - 9 Jul 2010, Zürich (Switzerland)
Y2  - 5 Jul 2010 - 9 Jul 2010
M2  - Zürich, Switzerland
KW  - axion: solar (INSPIRE)
KW  - signature (INSPIRE)
KW  - new physics (INSPIRE)
KW  - X-ray: solar (INSPIRE)
KW  - experimental results (INSPIRE)
LB  - PUB:(DE-HGF)8 ; PUB:(DE-HGF)15
DO  - DOI:10.3204/DESY-PROC-2010-03/zioutas_konstantin
UR  - https://bib-pubdb1.desy.de/record/296198
ER  -