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000316725 020__ $$a978-3-935702-43-0
000316725 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2015-02/giannotti_maurizio
000316725 0247_ $$2ISSN$$a1435-8077
000316725 037__ $$aPUBDB-2017-00123
000316725 041__ $$aEnglish
000316725 1001_ $$0P:(DE-HGF)0$$aGiannotti, Maurizio $$b0$$eCorresponding author
000316725 1112_ $$0C15-06-22.2$$2inspire$$a11th Patras Workshop on Axions, WIMPs and WISPs$$cZaragoza$$d2015-06-22 - 2015-06-26$$gAXION-WIMP 2015$$wSpain
000316725 245__ $$aALP Hints from Cooling Anomalies
000316725 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2015
000316725 29510 $$aGiannotti, Maurizio "ALP Hints from Cooling Anomalies" in Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) / Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel, Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J., Luzon, Gloria (eds.), Verlag Deutsches Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 - 2015-06-26, Zaragoza
000316725 300__ $$a26-30
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000316725 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000316725 520__ $$aWe review the current status of the anomalies in stellar cooling and argue that, among the new physics candidates, an axion-like particle would represent the best option to account for the hinted additional cooling.
000316725 7870_ $$0PUBDB-2017-00118$$aIrastorza, Igor G. et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2015-02$$tProceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
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000316725 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$aBarry University - Miami Shores - US$$b0
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