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000299846 1001_ $$0P:(DE-HGF)0$$aGiannotti, Maurizio$$b0
000299846 245__ $$aCool WISPs for stellar cooling excesses
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000299846 520__ $$aSeveral stellar systems (white dwarfs, red giants, horizontal branch stars and possibly the neutron star in the supernova remnant Cassiopeia A) show a preference for a mild non-standard cooling mechanism when compared with theoretical models. This exotic cooling could be provided by Weakly Interacting Slim Particles (WISPs), produced in the hot cores and abandoning the star unimpeded, contributing directly to the energy loss. Taken individually, these excesses do not show a strong statistical weight. However, if one mechanism could consistently explain several of them, the hint could be significant. We analyze the hints in terms of neutrino anomalous magnetic moments, minicharged particles, hidden photons and axion-like particles (ALPs). Among them, the ALP represents the best solution. Interestingly, the hinted ALP parameter space is accessible to the next generation proposed ALP searches, such as ALPS II and IAXO.
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000299846 7001_ $$0P:(DE-HGF)0$$aIrastorza, Igor$$b1
000299846 7001_ $$0P:(DE-HGF)0$$aRedondo, Javier$$b2
000299846 7001_ $$0P:(DE-H253)PIP1001650$$aRingwald, Andreas$$b3$$eCorresponding author$$udesy
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