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Contribution to a conference proceedings/Internal Report | PUBDB-2016-01092 |
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2011
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2011-04/zioutas_konstantin
Report No.: arXiv:1112.4329
Abstract: 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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