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Revista mexicana de física

versão impressa ISSN 0035-001X

Rev. mex. fis. vol.54  supl.3 México Dez. 2008

 

Neutrino masses and neutrinoless double–beta decay

 

Maura Pavan

 

Dipartimento di Fisica dell'Università di Milano, Bicocca and sezione INFN di Milano Bicocca, Italy.

 

Recibido el 13 de abril de 2008
Aceptado el 23 de junio de 2008

 

Abstract

The potentialities of Double Beta Decay experiments in the field of neutrino study are here discussed. Sensitivity and results are compared with the information coming from oscillation, cosmology and beta decay measurements.

Keywords: Double–beta decay; neutrino masses; Majorana neutrino.

 

Resumen

Se discuten las potencialidades de experimentos decaimiento doble–beta en el área de física de neutrinos. Se comparen las sensibilidades y los resultados con la información de oscilaciones de neutrinos, cosmología y mediciones de decaimiento beta.

Descriptores: Decaimiento doble–beta; masas de neutrinos; neutrino de Majorana.

 

PACS: 29.40; 23.40.–s

 

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References

1. B. Pontecorvo, Zh. Eksp. Teor. Fiz. (JETP) 33 (1957) 549;         [ Links ] Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28 (1962) 870.        [ Links ]

2. M. Maltoni et al., New J. Phys. 6 (2004) 122 and arXiv:hep–ph/0405172 v5;         [ Links ] S. Choubey, arXiv:hep–ph/0509217;         [ Links ] S. Goswami, Int. J. Mod. Phys. A 21 (2006) 1901;         [ Links ] A. Bandyopadhyay et al., Phys. Lett. B 608 (2005) 115;         [ Links ] G. L. Fogli et al. Prog. Part. Nucl. Phys. 57 (2006) 742.        [ Links ]

3. B.T. Cleveland et al., Astrophys. J. 496 (1998) 505;         [ Links ] J. N. Abdurashitov et al. (SAGE Collaboration), J. Exp. Theor. Phys. 95 (2002) 181;         [ Links ] W. Hampel et al. (GALLEX Collaboration), Phys. Lett. B 447 (1999) 127;         [ Links ] S. Fukuda et al. (Super–Kamiokande Collaboration), Phys. Lett. B 539 (2002) 179;         [ Links ] B. Aharmim et al. (SNO Collaboration), Phys. Rev. C 72 (2005) 055502.        [ Links ]

4. Y. Ashie et al. (Super–Kamiokande Collaboration), Phys. Rev. D 71 (2005) 112005.        [ Links ]

5. T. Araki et al. (KamLAND Collaboration), Phys. Rev. Lett. 94 (2005) 081801.        [ Links ]

6. E. Aliu et al. (K2K Collaboration), Phys. Rev. Lett. 94 (2005) 081802.         [ Links ] D. G. Michael et al. (MINOS Collaboration), Phys. Rev. Lett. 97 (2006) 191801.        [ Links ]

7. C. Athanassopoulos et al., Phys. Rev. Lett. 75 (1995) 2650;         [ Links ] A. Aguilar et al., Phys. Rev. D 64 (2001) 112007;         [ Links ] C. Athanassopoulos et al., Phys. Rev. Lett. 81 (1998) 1774 and Phys. Rev. C 54 (1996) 2685.        [ Links ]

8. A.A. Aguilar–Arevalo et al., Phys. Rev. Lett. 98 (2007) 231801;         [ Links ] M. Maltoni and T. Schwetz, arXiv:hep–ph/0705.0107 (2007).        [ Links ]

9. S. Goswami and W. Rodejohann, arXiv:hep–ph/0706.1462 (2007).        [ Links ]

10. A. Strumia and F. Vissani, arXiv::hep–ph/0606054 (2006).        [ Links ]

11. Y. Y. Keum et al., arXiv: :hep–ph/0803.2393 (2008).        [ Links ]

12. C. Kraus et al., Euro. Phys. J. C 40 (2005) 447;         [ Links ] V. M. Lobashev et al. Phys. Lett. 460 (1999) 227.        [ Links ]

13. The KATRIN Collaboration, hep–ex/0109033.        [ Links ]

14. MARE collaboration, http://mare.dfm.uninsubria.it/frontend/exec.php        [ Links ]

15. A. Morales and J. Morales, Nucl. Phys. B (Proc. Suppl.) 114 (2003) 141.;         [ Links ] O. Cremonesi, Nucl. Phys. B (Proc. Suppl.) 118 (2003) 287;         [ Links ] K. Zuber, Acta Polonica B 37 (2006) 1905;         [ Links ] F. T. Avignone et al., Rev. Mod. Phys., submitted May 30 (2007).        [ Links ]

16. V.A. Rodin et al., Nucl. Phys. A 766 (2006) 107;         [ Links ] Erratum: V.A. Rodin et al., arXiv::nucl–th/0706.4304 (2007).        [ Links ]

17. O. Civitarese and J. Suhonen, Nucl. Phys. A 761 (2005) 313.        [ Links ]

18. J. Menendez et al., arXiv::nucl–th/0801.3760 (2008).        [ Links ]

19. H.V. Klapdor–Kleingrothaus et al., Eur. Phys. J. A, 12 (2001) 147.        [ Links ]

20. H. V. Klapdor–Kleingrothaus et al., Mod. Phys. Lett. A, 16 (2001) 2409.         [ Links ] H. V. Klapdor–Kleingrothaus et al, NIM A, 522 (2004) 371.        [ Links ]

21. A. M. Bakalyarov et al., Proc. of NANP2003, Dubna, Russia, 24 June 2003;         [ Links ] C. E. Aalseth et al., Mod. Phys. Lett. A 17 (2002) 1475;         [ Links ] F. Feruglio, A. Strumia and F. Vissani, Nucl. Phys. B 637 (2002) 345, and Addendum, Nucl. Phys. B 659, (2003) 359.        [ Links ]

22. NEMO collaboration, http://nemo.in2p3.fr        [ Links ]

23. C. Arnaboldi et al., Phys. Rev. Lett., 95 (2005) 14501.        [ Links ]

24. I. Abdt et al., arXiv::hep–ex/0404039 (2004).        [ Links ]

25. C. E. Aalseth et al., Nucl. Phys. B (Proc. Suppl.) 138 (2005) 217.        [ Links ]

26. C. Arnaboldi et al., NIM A 518 (2004) 775.        [ Links ]

27. EXO collaboration, http://www–project.slac.stanford.edu/exo        [ Links ]

28. S. Pirro et al., NANP2005 Proceedings (2005), arXiv::nucl–ex/0510074.        [ Links ]

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