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001     295156
005     20211110133413.0
024 7 _ |a arXiv:1112.4329
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024 7 _ |a 10.3204/DESY-PROC-2011-04/zioutas_konstantin
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024 7 _ |a inspire:1082055
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088 1 _ |a arXiv:1112.4329
088 _ _ |a arXiv:1112.4329
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100 1 _ |a Zioutas, K.
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111 2 _ |a 7th Patras Workshop on Axions, WIMPs and WISPs
|g AXION-WIMP 2011
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|d 2011-06-27 - 2011-07-01
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245 _ _ |a Solar flares as harbinger of new physics
260 _ _ |c 2011
300 _ _ |a 120-124
336 7 _ |a Conference Paper
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520 _ _ |a This work provides additional evidence on the involvement of exotic particles like axions and/or other WISPs, following recent measurements during the quietest Sun and flaring Sun. Thus, SPHINX mission observed a minimum basal soft X-rays emission in the extreme solar minimum in 2009. The same scenario (with ~17 meV axions) fits also the dynamical behaviour of white-light solar flares, like the measured spectral components in the visible and in soft X-rays, and, the timing between them. Solar chameleons remain a viable candidate, since they may preferentially convert to photons in outer space.
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700 1 _ |a Tsagri, M.
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700 1 _ |a Semertzidis, Y.
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700 1 _ |a Papaevangelou, T.
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700 1 _ |a Georgiopoulou, E.
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700 1 _ |a Gardikiotis, A.
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700 1 _ |a Dafni, T.
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700 1 _ |a Tsagri, M.
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700 1 _ |a Semertzidis, Y.
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700 1 _ |a Papaevangelou, T.
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700 1 _ |a Georgiopoulou, E.
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700 1 _ |a Dafni, T.
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700 1 _ |a Gardikiotis, A.
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773 _ _ |a 10.3204/DESY-PROC-2011-04/zioutas_konstantin
787 0 _ |a Schumann, Marc et.al.
|d 2011
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|t Proceedings, 7th Patras Workshop on Axions, WIMPs and WISPs
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