The IAXO Helioscope

dc.authoridTR3959en_US
dc.contributor.authorRibas, Esther F.
dc.contributor.authorArmengaud, Eric
dc.contributor.authorAvignone, Frank T.
dc.contributor.authorBetz, Michael
dc.contributor.authorBrax, Philippe H.
dc.contributor.authorBurn, P.
dc.contributor.authorÇetin, Serkant Ali
dc.date.accessioned2016-03-21T09:11:14Z
dc.date.available2016-03-21T09:11:14Z
dc.date.issued2015-11-16
dc.departmentDoğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümüen_US
dc.descriptionÇetin, Serkant Ali (Dogus Author) -- Conference full title: 7th International Symposium on Large TPCs for Low-Energy Rare Event Detection; Institute of Astroparticle Physics (APC) Campus - Paris Diderot UniversityParis; France; 15 December 2014 through 17 December 2014en_US
dc.description.abstractThe IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on gaγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.en_US
dc.identifier.citationRibas, E. F., Armengaud, E., Avignone, F. T., Betz, M., Brax, P. H., Brun, P. ... Zioutas, K. (2015). In I. Irastorza, I. Giomataris, T. Patzak & P. Colas (Eds.), Journal of Physics: Conference Series (Volume 650) (pp. 1-8). Bristol: IOP Publishing. https://dx.doi.org/10.1088/1742-6596/650/1/012009en_US
dc.identifier.doi10.1088/1742-6596/650/1/012009
dc.identifier.endpage8en_US
dc.identifier.issn1742-6588
dc.identifier.issue1en_US
dc.identifier.other012009 (Scopus)
dc.identifier.scopus2-s2.0-84957837713en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage1en_US
dc.identifier.urihttps://dx.doi.org/10.1088/1742-6596/650/1/012009
dc.identifier.urihttps://hdl.handle.net/11376/2426
dc.identifier.volume650en_US
dc.identifier.wosWOS:000368140400009en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.institutionauthorÇetin, Serkant Ali
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.ispartofJournal of Physics: Conference Seriesen_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectDetectable Signalen_US
dc.subjectFeasibility Studiesen_US
dc.subjectFourth Generationen_US
dc.subjectLow Background Detectorsen_US
dc.subjectTechnical Designen_US
dc.subjectToroidal Magnetsen_US
dc.subjectX-ray Focusing Opticsen_US
dc.titleThe IAXO Helioscopeen_US
dc.typeConference Objecten_US

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