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Title: 130Te neutrinoless double-beta decay with CUORICINO

Abstract

We report the final result of the CUORICINO experiment. Operated between 2003 and 2008, with a total exposure of 19.75 kg · y of 130Te, CUORICINO was able to set a lower bound on the 130Te 0νββ half-life of 2.8 × 1024 years at 90% C.L. The limit here reported includes the effects of systematic uncertainties that are examined in detail in the paper. The corresponding upper bound on the neutrino Majorana mass is in the range 300-710 meV, depending on the adopted nuclear matrix element evaluation.

Authors:
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Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
Contributing Org.:
CUORICINO Collaboration
OSTI Identifier:
1511330
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astroparticle Physics
Additional Journal Information:
Journal Volume: 34; Journal Issue: 11; Journal ID: ISSN 0927-6505
Publisher:
Elsevier
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Andreotti, E., Arnaboldi, C., Avignone, F. T., Balata, M., Bandac, I., Barucci, M., Beeman, J. W., Bellini, F., Brofferio, C., Bryant, A., Bucci, C., Canonica, L., Capelli, S., Carbone, L., Carrettoni, M., Clemenza, M., Cremonesi, O., Creswick, R. J., Di Domizio, S., Dolinski, M. J., Ejzak, L., Faccini, R., Farach, H. A., Ferri, E., Fiorini, E., Foggetta, L., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Guardincerri, E., Gutierrez, T. D., Haller, E. E., Kazkaz, K., Kraft, S., Kogler, L., Maiano, C., Maruyama, R. H., Martinez, C., Martinez, M., Newman, S., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., Orio, F., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Pirro, S., Previtali, E., Risegari, L., Rosenfeld, C., Rusconi, C., Salvioni, C., Sangiorgio, S., Schaeffer, D., Scielzo, N. D., Sisti, M., Smith, A. R., Tomei, C., Ventura, G., and Vignati, M. 130Te neutrinoless double-beta decay with CUORICINO. United States: N. p., 2011. Web. doi:10.1016/j.astropartphys.2011.02.002.
Andreotti, E., Arnaboldi, C., Avignone, F. T., Balata, M., Bandac, I., Barucci, M., Beeman, J. W., Bellini, F., Brofferio, C., Bryant, A., Bucci, C., Canonica, L., Capelli, S., Carbone, L., Carrettoni, M., Clemenza, M., Cremonesi, O., Creswick, R. J., Di Domizio, S., Dolinski, M. J., Ejzak, L., Faccini, R., Farach, H. A., Ferri, E., Fiorini, E., Foggetta, L., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Guardincerri, E., Gutierrez, T. D., Haller, E. E., Kazkaz, K., Kraft, S., Kogler, L., Maiano, C., Maruyama, R. H., Martinez, C., Martinez, M., Newman, S., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., Orio, F., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Pirro, S., Previtali, E., Risegari, L., Rosenfeld, C., Rusconi, C., Salvioni, C., Sangiorgio, S., Schaeffer, D., Scielzo, N. D., Sisti, M., Smith, A. R., Tomei, C., Ventura, G., & Vignati, M. 130Te neutrinoless double-beta decay with CUORICINO. United States. doi:10.1016/j.astropartphys.2011.02.002.
Andreotti, E., Arnaboldi, C., Avignone, F. T., Balata, M., Bandac, I., Barucci, M., Beeman, J. W., Bellini, F., Brofferio, C., Bryant, A., Bucci, C., Canonica, L., Capelli, S., Carbone, L., Carrettoni, M., Clemenza, M., Cremonesi, O., Creswick, R. J., Di Domizio, S., Dolinski, M. J., Ejzak, L., Faccini, R., Farach, H. A., Ferri, E., Fiorini, E., Foggetta, L., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Guardincerri, E., Gutierrez, T. D., Haller, E. E., Kazkaz, K., Kraft, S., Kogler, L., Maiano, C., Maruyama, R. H., Martinez, C., Martinez, M., Newman, S., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., Orio, F., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Pirro, S., Previtali, E., Risegari, L., Rosenfeld, C., Rusconi, C., Salvioni, C., Sangiorgio, S., Schaeffer, D., Scielzo, N. D., Sisti, M., Smith, A. R., Tomei, C., Ventura, G., and Vignati, M. Wed . "130Te neutrinoless double-beta decay with CUORICINO". United States. doi:10.1016/j.astropartphys.2011.02.002. https://www.osti.gov/servlets/purl/1511330.
@article{osti_1511330,
title = {130Te neutrinoless double-beta decay with CUORICINO},
author = {Andreotti, E. and Arnaboldi, C. and Avignone, F. T. and Balata, M. and Bandac, I. and Barucci, M. and Beeman, J. W. and Bellini, F. and Brofferio, C. and Bryant, A. and Bucci, C. and Canonica, L. and Capelli, S. and Carbone, L. and Carrettoni, M. and Clemenza, M. and Cremonesi, O. and Creswick, R. J. and Di Domizio, S. and Dolinski, M. J. and Ejzak, L. and Faccini, R. and Farach, H. A. and Ferri, E. and Fiorini, E. and Foggetta, L. and Giachero, A. and Gironi, L. and Giuliani, A. and Gorla, P. and Guardincerri, E. and Gutierrez, T. D. and Haller, E. E. and Kazkaz, K. and Kraft, S. and Kogler, L. and Maiano, C. and Maruyama, R. H. and Martinez, C. and Martinez, M. and Newman, S. and Nisi, S. and Nones, C. and Norman, E. B. and Nucciotti, A. and Orio, F. and Pallavicini, M. and Palmieri, V. and Pattavina, L. and Pavan, M. and Pedretti, M. and Pessina, G. and Pirro, S. and Previtali, E. and Risegari, L. and Rosenfeld, C. and Rusconi, C. and Salvioni, C. and Sangiorgio, S. and Schaeffer, D. and Scielzo, N. D. and Sisti, M. and Smith, A. R. and Tomei, C. and Ventura, G. and Vignati, M.},
abstractNote = {We report the final result of the CUORICINO experiment. Operated between 2003 and 2008, with a total exposure of 19.75 kg · y of 130Te, CUORICINO was able to set a lower bound on the 130Te 0νββ half-life of 2.8 × 1024 years at 90% C.L. The limit here reported includes the effects of systematic uncertainties that are examined in detail in the paper. The corresponding upper bound on the neutrino Majorana mass is in the range 300-710 meV, depending on the adopted nuclear matrix element evaluation.},
doi = {10.1016/j.astropartphys.2011.02.002},
journal = {Astroparticle Physics},
number = 11,
volume = 34,
place = {United States},
year = {2011},
month = {2}
}

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