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000315507 020__ $$a978-3-935702-59-1
000315507 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-03/giannotti_maurizio
000315507 0247_ $$2ISSN$$a1435-8077
000315507 037__ $$aPUBDB-2016-05914
000315507 041__ $$aEnglish
000315507 1001_ $$0P:(DE-HGF)0$$aGiannotti, Maurizio$$b0$$eCorresponding author
000315507 1112_ $$0C14-06-29.1$$2inspire$$a10th Patras Workshop on Axions, WIMPs and WISPs$$cGeneva$$d2014-06-29 - 2014-07-04$$gAXION-WIMP 2014$$wSwitzerland
000315507 245__ $$aStellar Evolution Bounds on the ALP-Photon Coupling: new Results and Perspectives
000315507 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2014
000315507 29510 $$aGiannotti, Maurizio "Stellar Evolution Bounds on the ALP-Photon Coupling: new Results and Perspectives " in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)  / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
000315507 300__ $$a71-74
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000315507 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315507 520__ $$aStellar evolution considerations are of fundamental importance in our understanding of the axion/ALP-photon coupling, $ g_{a\gamma} $. Helium burning stars are the best laboratories to study this coupling. Here, we will review the bounds from massive and low mass helium burning stars, and present a new analysis of the bound from the horizontal branch stars. The analysis provides the strongest bound to date on $ g_{a\gamma} $ in a wide mass range.
000315507 7870_ $$0PUBDB-2016-05897$$aTsesmelis, Emmanuel et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2014-03$$tProceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014
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