The IAXO Helioscope
dc.authorid | TR3959 | en_US |
dc.contributor.author | Ribas, Esther F. | |
dc.contributor.author | Armengaud, Eric | |
dc.contributor.author | Avignone, Frank T. | |
dc.contributor.author | Betz, Michael | |
dc.contributor.author | Brax, Philippe H. | |
dc.contributor.author | Burn, P. | |
dc.contributor.author | Çetin, Serkant Ali | |
dc.date.accessioned | 2016-03-21T09:11:14Z | |
dc.date.available | 2016-03-21T09:11:14Z | |
dc.date.issued | 2015-11-16 | |
dc.department | Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü | en_US |
dc.description | Çetin, 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 2014 | en_US |
dc.description.abstract | The 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.citation | Ribas, 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/10.1088/1742-6596/650/1/012009 | en_US |
dc.identifier.doi | 10.1088/1742-6596/650/1/012009 | |
dc.identifier.endpage | 8 | en_US |
dc.identifier.issn | 1742-6588 | |
dc.identifier.issue | 1 | en_US |
dc.identifier.other | 012009 (Scopus) | |
dc.identifier.scopus | 2-s2.0-84957837713 | en_US |
dc.identifier.scopusquality | Q3 | en_US |
dc.identifier.startpage | 1 | en_US |
dc.identifier.uri | https://dx.doi.org/10.1088/1742-6596/650/1/012009 | |
dc.identifier.uri | https://hdl.handle.net/11376/2426 | |
dc.identifier.volume | 650 | en_US |
dc.identifier.wos | WOS:000368140400009 | en_US |
dc.identifier.wosquality | N/A | en_US |
dc.indekslendigikaynak | Web of Science | en_US |
dc.indekslendigikaynak | Scopus | en_US |
dc.institutionauthor | Çetin, Serkant Ali | |
dc.language.iso | en | en_US |
dc.publisher | IOP Publishing | en_US |
dc.relation.ispartof | Journal of Physics: Conference Series | en_US |
dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.subject | Detectable Signal | en_US |
dc.subject | Feasibility Studies | en_US |
dc.subject | Fourth Generation | en_US |
dc.subject | Low Background Detectors | en_US |
dc.subject | Technical Design | en_US |
dc.subject | Toroidal Magnets | en_US |
dc.subject | X-ray Focusing Optics | en_US |
dc.title | The IAXO Helioscope | en_US |
dc.type | Conference Object | en_US |