European Physical Journal C: Particles and Fields (Jul 2021)
Search for double-beta decay of $$\mathrm {^{130}Te}$$ 130 Te to the $$0^+$$ 0 + states of $$\mathrm {^{130}Xe}$$ 130 Xe with CUORE
- D. Q. Adams,
- C. Alduino,
- K. Alfonso,
- F. T. III Avignone,
- O. Azzolini,
- G. Bari,
- F. Bellini,
- G. Benato,
- M. Biassoni,
- A. Branca,
- C. Brofferio,
- C. Bucci,
- J. Camilleri,
- A. Caminata,
- A. Campani,
- L. Canonica,
- X. G. Cao,
- S. Capelli,
- L. Cappelli,
- L. Cardani,
- P. Carniti,
- N. Casali,
- E. Celi,
- D. Chiesa,
- M. Clemenza,
- S. Copello,
- C. Cosmelli,
- O. Cremonesi,
- R. J. Creswick,
- A. D’Addabbo,
- I. Dafinei,
- C. J. Davis,
- S. Dell’Oro,
- S. Di Domizio,
- V. Dompè,
- D. Q. Fang,
- G. Fantini,
- M. Faverzani,
- E. Ferri,
- F. Ferroni,
- E. Fiorini,
- M. A. Franceschi,
- S. J. Freedman,
- S. H. Fu,
- B. K. Fujikawa,
- A. Giachero,
- L. Gironi,
- A. Giuliani,
- P. Gorla,
- C. Gotti,
- T. D. Gutierrez,
- K. Han,
- K. M. Heeger,
- R. G. Huang,
- H. Z. Huang,
- J. Johnston,
- G. Keppel,
- Yu. G. Kolomensky,
- C. Ligi,
- L. Ma,
- Y. G. Ma,
- L. Marini,
- R. H. Maruyama,
- D. Mayer,
- Y. Mei,
- N. Moggi,
- S. Morganti,
- T. Napolitano,
- M. Nastasi,
- J. Nikkel,
- C. Nones,
- E. B. Norman,
- A. Nucciotti,
- I. Nutini,
- T. O’Donnell,
- J. L. Ouellet,
- S. Pagan,
- C. E. Pagliarone,
- L. Pagnanini,
- M. Pallavicini,
- L. Pattavina,
- M. Pavan,
- G. Pessina,
- V. Pettinacci,
- C. Pira,
- S. Pirro,
- S. Pozzi,
- E. Previtali,
- A. Puiu,
- C. Rosenfeld,
- C. Rusconi,
- M. Sakai,
- S. Sangiorgio,
- B. Schmidt,
- N. D. Scielzo,
- V. Sharma,
- V. Singh,
- M. Sisti,
- D. Speller,
- P. T. Surukuchi,
- L. Taffarello,
- F. Terranova,
- C. Tomei,
- K. J. Vetter,
- M. Vignati,
- S. L. Wagaarachchi,
- B. S. Wang,
- B. Welliver,
- J. Wilson,
- K. Wilson,
- L. A. Winslow,
- S. Zimmermann,
- S. Zucchelli
Affiliations
- D. Q. Adams
- Department of Physics and Astronomy, University of South Carolina
- C. Alduino
- Department of Physics and Astronomy, University of South Carolina
- K. Alfonso
- Department of Physics and Astronomy, University of California
- F. T. III Avignone
- Department of Physics and Astronomy, University of South Carolina
- O. Azzolini
- INFN–Laboratori Nazionali di Legnaro
- G. Bari
- INFN–Sezione di Bologna
- F. Bellini
- Dipartimento di Fisica, Sapienza Università di Roma
- G. Benato
- INFN–Laboratori Nazionali del Gran Sasso
- M. Biassoni
- INFN–Sezione di Milano-Bicocca
- A. Branca
- INFN–Sezione di Milano-Bicocca
- C. Brofferio
- INFN–Sezione di Milano-Bicocca
- C. Bucci
- INFN–Laboratori Nazionali del Gran Sasso
- J. Camilleri
- Center for Neutrino Physics, Virginia Polytechnic Institute and State University
- A. Caminata
- INFN–Sezione di Genova
- A. Campani
- INFN–Sezione di Genova
- L. Canonica
- INFN–Laboratori Nazionali del Gran Sasso
- X. G. Cao
- Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University
- S. Capelli
- INFN–Sezione di Milano-Bicocca
- L. Cappelli
- INFN–Laboratori Nazionali del Gran Sasso
- L. Cardani
- INFN–Sezione di Roma
- P. Carniti
- INFN–Sezione di Milano-Bicocca
- N. Casali
- INFN–Sezione di Roma
- E. Celi
- INFN–Laboratori Nazionali del Gran Sasso
- D. Chiesa
- INFN–Sezione di Milano-Bicocca
- M. Clemenza
- INFN–Sezione di Milano-Bicocca
- S. Copello
- INFN–Sezione di Genova
- C. Cosmelli
- Dipartimento di Fisica, Sapienza Università di Roma
- O. Cremonesi
- INFN–Sezione di Milano-Bicocca
- R. J. Creswick
- Department of Physics and Astronomy, University of South Carolina
- A. D’Addabbo
- INFN–Laboratori Nazionali del Gran Sasso
- I. Dafinei
- INFN–Sezione di Roma
- C. J. Davis
- Wright Laboratory, Department of Physics, Yale University
- S. Dell’Oro
- INFN–Sezione di Milano-Bicocca
- S. Di Domizio
- INFN–Sezione di Genova
- V. Dompè
- INFN–Laboratori Nazionali del Gran Sasso
- D. Q. Fang
- Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University
- G. Fantini
- Dipartimento di Fisica, Sapienza Università di Roma
- M. Faverzani
- INFN–Sezione di Milano-Bicocca
- E. Ferri
- INFN–Sezione di Milano-Bicocca
- F. Ferroni
- INFN–Sezione di Roma
- E. Fiorini
- INFN–Sezione di Milano-Bicocca
- M. A. Franceschi
- INFN–Laboratori Nazionali di Frascati
- S. J. Freedman
- Department of Physics, University of California
- S. H. Fu
- Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University
- B. K. Fujikawa
- Nuclear Science Division, Lawrence Berkeley National Laboratory
- A. Giachero
- INFN–Sezione di Milano-Bicocca
- L. Gironi
- INFN–Sezione di Milano-Bicocca
- A. Giuliani
- Université Paris-Saclay, CNRS/IN2P3, IJCLab
- P. Gorla
- INFN–Laboratori Nazionali del Gran Sasso
- C. Gotti
- INFN–Sezione di Milano-Bicocca
- T. D. Gutierrez
- Physics Department, California Polytechnic State University
- K. Han
- INPAC and School of Physics and Astronomy, Shanghai Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University
- K. M. Heeger
- Wright Laboratory, Department of Physics, Yale University
- R. G. Huang
- Department of Physics, University of California
- H. Z. Huang
- Department of Physics and Astronomy, University of California
- J. Johnston
- Massachusetts Institute of Technology
- G. Keppel
- INFN–Laboratori Nazionali di Legnaro
- Yu. G. Kolomensky
- Department of Physics, University of California
- C. Ligi
- INFN–Laboratori Nazionali di Frascati
- L. Ma
- Department of Physics and Astronomy, University of California
- Y. G. Ma
- Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University
- L. Marini
- Department of Physics, University of California
- R. H. Maruyama
- Wright Laboratory, Department of Physics, Yale University
- D. Mayer
- Massachusetts Institute of Technology
- Y. Mei
- Nuclear Science Division, Lawrence Berkeley National Laboratory
- N. Moggi
- INFN–Sezione di Bologna
- S. Morganti
- INFN–Sezione di Roma
- T. Napolitano
- INFN–Laboratori Nazionali di Frascati
- M. Nastasi
- INFN–Sezione di Milano-Bicocca
- J. Nikkel
- Wright Laboratory, Department of Physics, Yale University
- C. Nones
- Service de Physique des Particules, CEA/Saclay
- E. B. Norman
- Lawrence Livermore National Laboratory
- A. Nucciotti
- INFN–Sezione di Milano-Bicocca
- I. Nutini
- INFN–Sezione di Milano-Bicocca
- T. O’Donnell
- Center for Neutrino Physics, Virginia Polytechnic Institute and State University
- J. L. Ouellet
- Massachusetts Institute of Technology
- S. Pagan
- Wright Laboratory, Department of Physics, Yale University
- C. E. Pagliarone
- INFN–Laboratori Nazionali del Gran Sasso
- L. Pagnanini
- INFN–Laboratori Nazionali del Gran Sasso
- M. Pallavicini
- INFN–Sezione di Genova
- L. Pattavina
- INFN–Laboratori Nazionali del Gran Sasso
- M. Pavan
- INFN–Sezione di Milano-Bicocca
- G. Pessina
- INFN–Sezione di Milano-Bicocca
- V. Pettinacci
- INFN–Sezione di Roma
- C. Pira
- INFN–Laboratori Nazionali di Legnaro
- S. Pirro
- INFN–Laboratori Nazionali del Gran Sasso
- S. Pozzi
- INFN–Sezione di Milano-Bicocca
- E. Previtali
- INFN–Sezione di Milano-Bicocca
- A. Puiu
- INFN–Laboratori Nazionali del Gran Sasso
- C. Rosenfeld
- Department of Physics and Astronomy, University of South Carolina
- C. Rusconi
- Department of Physics and Astronomy, University of South Carolina
- M. Sakai
- Department of Physics, University of California
- S. Sangiorgio
- Lawrence Livermore National Laboratory
- B. Schmidt
- Nuclear Science Division, Lawrence Berkeley National Laboratory
- N. D. Scielzo
- Lawrence Livermore National Laboratory
- V. Sharma
- Center for Neutrino Physics, Virginia Polytechnic Institute and State University
- V. Singh
- Department of Physics, University of California
- M. Sisti
- INFN–Sezione di Milano-Bicocca
- D. Speller
- Department of Physics and Astronomy, The Johns Hopkins University
- P. T. Surukuchi
- Wright Laboratory, Department of Physics, Yale University
- L. Taffarello
- INFN–Sezione di Padova
- F. Terranova
- INFN–Sezione di Milano-Bicocca
- C. Tomei
- INFN–Sezione di Roma
- K. J. Vetter
- Department of Physics, University of California
- M. Vignati
- INFN–Sezione di Roma
- S. L. Wagaarachchi
- Department of Physics, University of California
- B. S. Wang
- Lawrence Livermore National Laboratory
- B. Welliver
- Nuclear Science Division, Lawrence Berkeley National Laboratory
- J. Wilson
- Department of Physics and Astronomy, University of South Carolina
- K. Wilson
- Department of Physics and Astronomy, University of South Carolina
- L. A. Winslow
- Massachusetts Institute of Technology
- S. Zimmermann
- Engineering Division, Lawrence Berkeley National Laboratory
- S. Zucchelli
- INFN–Sezione di Bologna
- DOI
- https://doi.org/10.1140/epjc/s10052-021-09317-z
- Journal volume & issue
-
Vol. 81,
no. 7
pp. 1 – 14
Abstract
Abstract The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) in the isotope $$\mathrm {^{130}Te}$$ 130 Te . In this work we present the latest results on two searches for the double beta decay (DBD) of $$\mathrm {^{130}Te}$$ 130 Te to the first $$0^{+}_2$$ 0 2 + excited state of $$\mathrm {^{130}Xe}$$ 130 Xe : the $$0\nu \beta \beta $$ 0 ν β β decay and the Standard Model-allowed two-neutrinos double beta decay ( $$2\nu \beta \beta $$ 2 ν β β ). Both searches are based on a 372.5 kg $$\times $$ × yr TeO $$_2$$ 2 exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90% Credible Interval (C.I.) of the given searches were estimated as $$\mathrm {S^{0\nu }_{1/2} = 5.6 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 0 ν = 5.6 × 10 24 yr for the $${0\nu \beta \beta }$$ 0 ν β β decay and $$\mathrm {S^{2\nu }_{1/2} = 2.1 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 2 ν = 2.1 × 10 24 yr for the $${2\nu \beta \beta }$$ 2 ν β β decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $$90\%$$ 90 % C.I. on the decay half lives is obtained as: $$\mathrm {(T_{1/2})^{0\nu }_{0^+_2} > 5.9 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 0 ν > 5.9 × 10 24 yr for the $$0\nu \beta \beta $$ 0 ν β β mode and $$\mathrm {(T_{1/2})^{2\nu }_{0^+_2} > 1.3 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 2 ν > 1.3 × 10 24 yr for the $$2\nu \beta \beta $$ 2 ν β β mode. These represent the most stringent limits on the DBD of $$^{130}$$ 130 Te to excited states and improve by a factor $$\sim 5$$ ∼ 5 the previous results on this process.