Study of rare nuclear processes with CUORE-Reference-Cited by-同舟云学术

Study of rare nuclear processes with CUORE

Published:2018-03-30 Issue:09 Volume:33 Page:1843002
ISSN:0217-751X
Container-title:International Journal of Modern Physics A
language:en
Short-container-title:Int. J. Mod. Phys. A

Author:

Alduino C.¹,Alfonso K.²,Avignone F. T.,Azzolini O.³,Bari G.⁴,Bellini F.⁵⁶,Benato G.⁷,Bersani A.⁸,Biassoni M.⁹,Branca A.¹⁰¹¹,Brofferio C.⁹¹²,Bucci C.¹³,Camacho A.³,Caminata A.⁸,Canonica L.¹³¹⁴,Cao X. G.¹⁵,Capelli S.⁹¹²,Cappelli L.⁷¹³¹⁶,Cardani L.⁶,Carniti P.⁹¹²,Casali N.⁶,Cassina L.⁹¹²,Chiesa D.⁹¹²,Chott N.¹,Clemenza M.⁹¹²,Copello S.⁸¹⁷,Cosmelli C.⁵⁶,Cremonesi O.⁹,Creswick R. J.¹,Cushman J. S.¹⁸,D’Addabbo A.¹³,D’Aguanno D.¹³¹⁹,Dafinei I.⁶,Davis C. J.¹⁸,Dell’Oro S.²⁰,Deninno M. M.⁴,Di Domizio S.⁸¹⁷,Di Vacri M. L.¹³²¹,Dompè V.¹³²²,Drobizhev A.⁷¹⁶,Fang D. Q.¹⁵,Faverzani M.⁹¹²,Ferri E.⁹,Ferroni F.⁵⁶,Fiorini E.⁹¹²,Franceschi M. A.²³,Freedman S. J.⁷¹⁶,Fujikawa B. K.¹⁶,Giachero A.⁹¹²,Gironi L.⁹¹²,Giuliani A.²⁴,Gladstone L.¹⁴,Gorla P.¹³,Gotti C.⁹¹²,Gutierrez T. D.²⁵,Han K.²⁶,Heeger K. M.¹⁸,Hennings-Yeomans R.⁷¹⁶,Huang H. Z.²,Keppel G.³,Kolomensky Yu. G.⁷¹⁶,Leder A.¹⁴,Ligi C.²³,Lim K. E.¹⁸,Ma Y. G.¹⁵,Marini L.⁸¹⁷,Martinez M.⁵⁶²⁷,Maruyama R. H.¹⁸,Mei Y.¹⁶,Moggi N.⁴²⁸,Morganti S.⁶,Nagorny S. S.¹³²²,Napolitano T.²³,Nastasi M.⁹¹²,Nones C.²⁹,Norman E. B.³⁰³¹,Novati V.²⁴,Nucciotti A.⁹¹²,Nutini I.¹³²²,O’Donnell T.²⁰,Ouellet J. L.¹⁴,Pagliarone C. E.¹³¹⁹,Pallavicini M.⁸¹⁷,Palmieri V.³,Pattavina L.¹³,Pavan M.⁹¹²,Pessina G.⁹,Pira C.³,Pirro S.¹³,Pozzi S.⁹¹²,Previtali E.⁹,Reindl F.⁶,Rosenfeld C.¹,Rusconi C.¹¹³,Sakai M.²,Sangiorgio S.³⁰,Santone D.¹³²¹,Schmidt B.¹⁶,Schmidt J.²,Scielzo N. D.³⁰,Singh V.⁷,Sisti M.⁹¹²,Taffarello L.¹⁰,Terranova F.⁹¹²,Tomei C.⁶,Vignati M.⁶,Wagaarachchi S. L.⁷¹⁶,Wang B. S.³⁰³¹,Wang H. W.¹⁵,Welliver B.¹⁶,Wilson J.¹,Wilson K.¹,Winslow L. A.¹⁴,Wise T.¹⁸³²,Zanotti L.⁹¹²,Zhang G. Q.¹⁵,Zimmermann S.³³,Zucchelli S.⁴²⁸

Affiliation:

1. Department of Physics and Astronomy, University of South Carolina, Columbia, SC 29208, USA

2. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA

3. INFN – Laboratori Nazionali di Legnaro, Legnaro (Padova) I-35020, Italy

4. INFN – Sezione di Bologna, Bologna I-40127, Italy

5. Dipartimento di Fisica, Sapienza Università di Roma, Roma I-00185, Italy

6. INFN – Sezione di Roma, Roma I-00185, Italy

7. Department of Physics, University of California, Berkeley, CA 94720, USA

8. INFN – Sezione di Genova, Genova I-16146, Italy

9. INFN – Sezione di Milano Bicocca, Milano I-20126, Italy

10. INFN – Sezione di Padova, Padova I-35131, Italy

11. Dipartimento di Fisica e Astronomia, Università di Padova, I-35131 Padova, Italy

12. Dipartimento di Fisica, Università di Milano-Bicocca, Milano I-20126, Italy

13. INFN – Laboratori Nazionali del Gran Sasso, Assergi (L’Aquila) I-67100, Italy

14. Massachusetts Institute of Technology, Cambridge, MA 02139, USA

15. Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China

16. Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA

17. Dipartimento di Fisica, Università di Genova, Genova I-16146, Italy

18. Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520, USA

19. Dipartimento di Ingegneria Civile e Meccanica, Università degli Studi di Cassino e del Lazio Meridionale, Cassino I-03043, Italy

20. Center for Neutrino Physics, Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061, USA

21. Dipartimento di Scienze Fisiche e Chimiche, Università dell’Aquila, L’Aquila I-67100, Italy

22. INFN – Gran Sasso Science Institute, L’Aquila I-67100, Italy

23. INFN – Laboratori Nazionali di Frascati, Frascati (Roma) I-00044, Italy

24. CSNSM, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, 91405 Orsay, France

25. Physics Department, California Polytechnic State University, San Luis Obispo, CA 93407, USA

26. INPAC and School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai Laboratory for Particle Physics and Cosmology, Shanghai 200240, China

27. Laboratorio de Fisica Nuclear y Astroparticulas, Universidad de Zaragoza, Zaragoza 50009, Spain

28. Dipartimento di Fisica e Astronomia, Alma Mater Studiorum – Università di Bologna, Bologna I-40127, Italy

29. Service de Physique des Particules, CEA/Saclay, 91191 Gif-sur-Yvette, France

30. Lawrence Livermore National Laboratory, Livermore, CA 94550, USA

31. Department of Nuclear Engineering, University of California, Berkeley, CA 94720, USA

32. Department of Physics, University of Wisconsin, Madison, WI 53706, USA

33. Engineering Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA

Abstract

TeO2 bolometers have been used for many years to search for neutrinoless double beta decay in [Formula: see text]Te. CUORE, a tonne-scale TeO2 detector array, recently published the most sensitive limit on the half-life, [Formula: see text] yr, which corresponds to an upper bound of 140–400 meV on the effective Majorana mass of the neutrino. While it makes CUORE a world-leading experiment looking for neutrinoless double beta decay, it is not the only study that CUORE will contribute to in the field of nuclear and particle physics. As already done over the years with many small-scale experiments, CUORE will investigate both rare decays (such as the two-neutrino double beta decay of [Formula: see text]Te and the hypothesized electron capture in [Formula: see text]Te), and rare processes (e.g. dark matter and axion interactions). This paper describes some of the achievements of past experiments that used TeO2 bolometers, and perspectives for CUORE.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0217751X18430029

Reference82 articles.

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