Alvarez, V.; Borges, FIGM.; Carcel, S.; Castel, J.; Cebrian, S.; Cervera, A.; Conde, CAN.... (2013). Near-intrinsic energy resolution for 30-662 keV gamma rays in a high pressure xenon electroluminescent TPC. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 708:101-114. https://doi.org/10.1016/j.nima.2012.12.123
Por favor, use este identificador para citar o enlazar este ítem: http://hdl.handle.net/10251/45410
Título:
|
Near-intrinsic energy resolution for 30-662 keV gamma rays in a high pressure xenon electroluminescent TPC
|
Autor:
|
Alvarez, V.
Borges, F. I. G. M.
Carcel, S.
Castel, J.
Cebrian, S.
Cervera, A.
Conde, C. A. N.
Dafni, T.
Dias, T. H. V. T.
Diaz, J.
Esteve Bosch, Raul
Marí Romero, Antonio Francisco
Mora Mas, Francisco José
Palma, R.
Pérez Aparicio, José Luis
Toledo Alarcón, José Francisco
|
Entidad UPV:
|
Universitat Politècnica de València. Departamento de Ingeniería Electrónica - Departament d'Enginyeria Electrònica
Universitat Politècnica de València. Instituto de Instrumentación para Imagen Molecular - Institut d'Instrumentació per a Imatge Molecular
Universitat Politècnica de València. Departamento de Mecánica de los Medios Continuos y Teoría de Estructuras - Departament de Mecànica dels Medis Continus i Teoria d'Estructures
|
Fecha difusión:
|
|
Resumen:
|
We present the design, data and results from the NEXT prototype for Double Beta and Dark Matter (NEXT-DBDM) detector, a high-pressure gaseous natural xenon electroluminescent time projection chamber (TPC) that was built ...[+]
We present the design, data and results from the NEXT prototype for Double Beta and Dark Matter (NEXT-DBDM) detector, a high-pressure gaseous natural xenon electroluminescent time projection chamber (TPC) that was built at the Lawrence Berkeley National Laboratory. It is a prototype of the planned NEXT-100 Xe-136 neutrino-less double beta decay (0 nu beta beta) experiment with the main objectives of demonstrating near-intrinsic energy resolution at energies up to 662 keV and of optimizing the NEXT-100 detector design and operating parameters. Energy resolutions of similar to 1% FWHM for 662 keV gamma rays were obtained at 10 and 15 atm and similar to 5% FWHM for 30 keV fluorescence xenon X-rays. These results demonstrate that 0.5% FWHM resolutions for the 2459 keV hypothetical neutrino-less double beta decay peak are realizable. This energy resolution is a factor 7-20 better than that of the current leading 0 nu beta beta experiments using liquid xenon and thus represents a significant advancement. We present also first results from a track imaging system consisting of 64 silicon photo-multipliers recently installed in NEXT-DBDM that, along with the excellent energy resolution, demonstrates the key functionalities required for the NEXT-100 0 nu beta beta search. (c) 2013 Elsevier B.V. All rights reserved.
[-]
|
Palabras clave:
|
Xenon
,
Energy resolution
,
High-pressure
,
TPC
,
Electroluminescence
,
Neutrinoless double beta decay
|
Derechos de uso:
|
Reserva de todos los derechos
|
Fuente:
|
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. (issn:
0168-9002
)
|
DOI:
|
10.1016/j.nima.2012.12.123
|
Editorial:
|
Elsevier
|
Versión del editor:
|
http://dx.doi.org/10.1016/j.nima.2012.12.123
|
Código del Proyecto:
|
info:eu-repo/grantAgreement/DOE//DE-AC02-05CH11231/
info:eu-repo/grantAgreement/DOE//DE-FC52-08NA28752/
info:eu-repo/grantAgreement/MICINN//FPA2009-13697-C04-04/ES/Fisica Experimental De Neutrinos En El Ific/
info:eu-repo/grantAgreement/MICINN//CSD2008-00037/ES/Canfranc Underground Physics/
|
Agradecimientos:
|
We thank Adam Bernstein and Mike Heffner for the loan of the high pressure and storage vessels from LLNL (under LLNL loan 101-3026). This work was supported by the Director, Office of Science, Office of Basic Energy Sciences, ...[+]
We thank Adam Bernstein and Mike Heffner for the loan of the high pressure and storage vessels from LLNL (under LLNL loan 101-3026). This work was supported by the Director, Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This work used resources of the National Energy Research Scientific Computing Center (NERSC). J. Renner (LBNL) acknowledges the support of a US DOE NNSA Stewardship Science Graduate Fellowship under contract no. DE-FC52-08NA28752. This work was also supported by the Ministerio de Economia y Competitividad of Spain under grants CONSOLIDER-Ingenio 2010 CSD2008-0037 (CUP) and FPA2009-13697-C04-04.
[-]
|
Tipo:
|
Artículo
|