Sensitivity of NEXT-100 to neutrinoless double beta decay
Abstract
NEXT-100 is an electroluminescent high-pressure xenon gas time projection chamber that will search for the neutrinoless double beta () decay of Xe-136. The detector possesses two features of great value for searches: energy resolution better than 1\% FWHM at the value of Xe-136 and track reconstruction for the discrimination of signal and background events. This combination results in excellent sensitivity, as discussed in this paper. Material-screening measurements and a detailed Monte Carlo detector simulation predict a background rate for NEXT-100 of at most counts keV kg yr. Accordingly, the detector will reach a sensitivity to the \bbonu-decay half-life of years (90\% CL) for an exposure of 100 , or years after a run of 3 effective years.
Keywords
Cite
@article{arxiv.1511.09246,
title = {Sensitivity of NEXT-100 to neutrinoless double beta decay},
author = {NEXT Collaboration and J. Martín-Albo and J. Muñoz Vidal and P. Ferrario and M. Nebot-Guinot and J. J. Gómez-Cadenas and V. Álvarez and C. D. R. Azevedo and F. I. G. Borges and S. Cárcel and S. Cebrián and A. Cervera and C. A. N. Conde and J. Díaz and M. Diesburg and R. Esteve and L. M. P. Fernandes and A. L. Ferreira and E. D. C. Freitas and A. Goldschmidt and D. González-Díaz and R. M. Gutiérrez and J. Hauptman and C. A. O. Henriques and J. A. Hernando Morata and L. Labarga and A. Laing and P. Lebrun and I. Liubarsky and N. López-March and D. Lorca and M. Losada and G. Martínez-Lema and A. Martínez and F. Monrabal and C. M. B. Monteiro and F. J. Mora and L. M. Moutinho and P. Novella and D. Nygren and B. Palmeiro and A. Para and J. Pérez and M. Querol and J. Renner and L. Ripoll and J. Rodríguez and F. P. Santos and J. M. F. dos Santos and L. Serra and D. Shuman and A. Simón and C. Sofka and M. Sorel and T. Stiegler and J. F. Toledo and J. Torrent and Z. Tsamalaidze and J. F. C. A. Veloso and R. Webb and J. T. White and N. Yahlali and H. Yepes-Ramírez},
journal= {arXiv preprint arXiv:1511.09246},
year = {2016}
}
Comments
Accepted for publication in the Journal of High Energy Physics (JHEP)