Energy calibration of the NEXT-White detector with 1% resolution near Q ββ of 136Xe

Energy calibration of the NEXT-White detector with 1% resolution near Q ββ of 136Xe

Abstract Excellent energy resolution is one of the primary advantages of electroluminescent high-pressure xenon TPCs. These detectors are promising tools in searching for rare physics events, such as neutrinoless double-beta decay (ββ0ν), which require precise energy measurements. Using the NEXT-Whi...

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Main Authors: The NEXT collaboration, J. Renner, G. Díaz López, P. Ferrario, J. A. Hernando Morata, M. Kekic, G. Martínez-Lema, F. Monrabal, J. J. Gómez-Cadenas, C. Adams, V. Álvarez, L. Arazi, I. J. Arnquist, C. D. R Azevedo, K. Bailey, F. Ballester, J. M. Benlloch-Rodríguez, F. I. G. M. Borges, N. Byrnes, S. Cárcel, J. V. Carrión, S. Cebrián, E. Church, C. A. N. Conde, T. Contreras, J. Díaz, M. Diesburg, J. Escada, R. Esteve, R. Felkai, A. F. M. Fernandes, L. M. P. Fernandes, A. L. Ferreira, E. D. C. Freitas, J. Generowicz, S. Ghosh, A. Goldschmidt, D. González-Díaz, R. Guenette, R. M. Gutiérrez, J. Haefner, K. Hafidi, J. Hauptman, C. A. O. Henriques, P. Herrero, V. Herrero, Y. Ifergan, S. Johnston, B. J. P. Jones, L. Labarga, A. Laing, P. Lebrun, N. López-March, M. Losada, R. D. P. Mano, J. Martín-Albo, A. Martínez, A. D. McDonald, C. M. B. Monteiro, F.J. Mora, J. Muñoz Vidal, P. Novella, D. R. Nygren, B. Palmeiro, A. Para, J. Pérez, F. Psihas, M. Querol, J. Repond, S. Riordan, L. Ripoll, Y. Rodríguez García, J. Rodríguez, L. Rogers, B. Romeo, C. Romo-Luque, F. P. Santos, J. M. F. dos Santos, A. Simón, C. Sofka, M. Sorel, T. Stiegler, J. F. Toledo, J. Torrent, A. Usón, J. F. C. A. Veloso, R. Webb, R. Weiss-Babai, J. T. White, K. Woodruff, N. Yahlali
Format: Article
Language:English
Published: SpringerOpen 2019-10-01
Series:Journal of High Energy Physics
Subjects:
Dark Matter and Double Beta Decay (experiments)
Online Access:http://link.springer.com/article/10.1007/JHEP10(2019)230

Internet

http://link.springer.com/article/10.1007/JHEP10(2019)230

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