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000056340 005__ 20200221144253.0
000056340 0247_ $$2doi$$a10.1088/1742-6596/718/6/062033
000056340 0248_ $$2sideral$$a95709
000056340 037__ $$aART-2016-95709
000056340 041__ $$aeng
000056340 100__ $$aA Laing on behalf of the NEXT collaboration
000056340 245__ $$aThe NEXT double beta decay experiment
000056340 260__ $$c2016
000056340 5060_ $$aAccess copy available to the general public$$fUnrestricted
000056340 5203_ $$aNEXT (Neutrino Experiment with a Xenon TPC) is a neutrinoless double- beta (ßß0¿) decay experiment at Laboratorio Subterra ´neo de Canfranc (LSC). It is an electroluminescent Time Projection Chamber filled with high pressure 136Xe gas with separated function capabilities for calorimetry and tracking. Energy resolution and background suppression are the two key features of any neutrinoless double beta decay experiment. NEXT has both good energy resolution (< 1% FWHM) and an extra handle for background identification provided by track reconstruction. We expect a background rate of 4 × 10-4 counts keV-1 kg-1 yr-1, and a sensitivity to the Majorana neutrino mass of between 80–160 meV (depending on NME) after a run of 3 effective years of the 100 kg scale NEXT-100 detector. The initial phase of NEXT-100, called NEW, is currently being commissioned at LSC. It will validate the NEXT background rate expectations and will make first measurements of the two neutrino ßß2¿ mode of 136Xe. Furthermore, the NEXT technique can be extrapolated to the tonne scale, thus allowing the full exploration of the inverted hierarchy of neutrino masses. These proceedings review NEXT R&D results, the status of detector commissioning at LSC and the NEXT physics case.
000056340 536__ $$9info:eu-repo/grantAgreement/ES/MINECO/FIS2014-53371-C04$$9info:eu-repo/grantAgreement/ES/MINECO/Consolider-Ingenio-2010/CSD2008-00037$$9info:eu-repo/grantAgreement/EC/FP7/339787/EU/Towards the NEXT generation of bb0nu experimets/NEXT
000056340 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000056340 592__ $$a0.24$$b2016
000056340 593__ $$aPhysics and Astronomy (miscellaneous)$$c2016$$dQ3
000056340 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000056340 700__ $$aCebrian, S
000056340 773__ $$g718 (2016), 062033 [5 pp.]$$pJ. Phys.: Conf. Ser.$$tJournal of physics. Conference series$$x1742-6588
000056340 8564_ $$s790038$$uhttps://zaguan.unizar.es/record/56340/files/texto_completo.pdf$$yVersión publicada
000056340 8564_ $$s94249$$uhttps://zaguan.unizar.es/record/56340/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000056340 909CO $$ooai:zaguan.unizar.es:56340$$particulos$$pdriver
000056340 951__ $$a2020-02-21-13:28:36
000056340 980__ $$aARTICLE