000056303 001__ 56303
000056303 005__ 20170327111924.0
000056303 0248_ $$2sideral$$a95516
000056303 037__ $$aART-2015-95516
000056303 041__ $$aeng
000056303 100__ $$0(orcid)0000-0002-8921-910X$$aDafni, Theopisti$$uUniversidad de Zaragoza
000056303 245__ $$aThe latest results from CAST and the IAXO project
000056303 260__ $$c2015
000056303 5060_ $$aAccess copy available to the general public$$fUnrestricted
000056303 5203_ $$aThe CAST experiment has been the most sensitive helioscope so far. It has extended its sensitivity to the upper bounds of axion masses allowed by cosmology, entering well into the QCD-axion band. The preliminary analysis of the data taken with sensitivity to axion masses of the range 0.64 eV to 1.17 eV show no excess of signal above background and the coupling constant is restricted to ga¿ < 3.3 × 10-10 GeV-1 . While CAST continues with the aim to improve its results in the vacuum phase, IAXO is the new project proposed to build a dedicated magnet for axion searches that will supersede CAST’s sensitivity by one order of magnitude in ga¿.
000056303 540__ $$9info:eu-repo/semantics/openAccess$$aby-nc-sa$$uhttp://creativecommons.org/licenses/by-nc-sa/3.0/es/
000056303 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000056303 7102_ $$12004$$2390$$aUniversidad de Zaragoza$$bDepartamento de Física Teórica$$cFísica Atómica, Molecular y Nuclear
000056303 773__ $$gEPS-HEP 2013 (2015), [7 PP.]$$pPos proc. sci.$$tPos proceedings of science$$x1824-8039
000056303 85641 $$uhttp://pos.sissa.it/cgi-bin/reader/contribution.cgi?id=180/394$$zTexto completo de la revista
000056303 8564_ $$s223019$$uhttp://zaguan.unizar.es/record/56303/files/texto_completo.pdf$$yVersión publicada
000056303 8564_ $$s42544$$uhttp://zaguan.unizar.es/record/56303/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000056303 909CO $$ooai:zaguan.unizar.es:56303$$particulos$$pdriver
000056303 951__ $$a2016-08-16-13:08:17
000056303 980__ $$aARTICLE