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000316760 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2015-02/ayala_adrian
000316760 0247_ $$2ISSN$$a1435-8077
000316760 037__ $$aPUBDB-2017-00158
000316760 041__ $$aEnglish
000316760 1001_ $$0P:(DE-HGF)0$$aAyala, Adrian$$b0
000316760 1112_ $$0C15-06-22.2$$2inspire$$a11th Patras Workshop on Axions, WIMPs and WISPs$$cZaragoza$$d2015-06-22 - 2015-06-26$$gAXION-WIMP 2015$$wSpain
000316760 245__ $$aEffects of Hidden Photons during the Red Giant Branch (RGB) Phase
000316760 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2015
000316760 29510 $$aAyala, Adrian "Effects of Hidden Photons during the Red Giant Branch (RGB) Phase" in Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) / Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel, Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J., Luzon, Gloria (eds.), Verlag Deutsches Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 - 2015-06-26, Zaragoza
000316760 300__ $$a189-192
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000316760 520__ $$aFeatures in the globular cluster luminosity functions (LF) of the post-main sequence stellar evolution can be used to investigate modifications of standard stellar models and to look for new physics fingerprints, like axions or hidden photons. Here, we investigate the possible effects of hidden photons during the red giant branch (RGB) phase. In a follow-up analysis, these results will be applied to discuss signatures and observational effects in the globular cluster LF.
000316760 7001_ $$0P:(DE-HGF)0$$aStraniero, Oscar$$b1
000316760 7001_ $$0P:(DE-HGF)0$$aGiannotti, Maurizio$$b2
000316760 7001_ $$0P:(DE-HGF)0$$aMirizzi, Alessandro$$b3
000316760 7001_ $$0P:(DE-HGF)0$$aDominguez, Inma$$b4
000316760 7870_ $$0PUBDB-2017-00118$$aIrastorza, Igor G. et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2015-02$$tProceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
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