Abstract
The present status of experiments seeking double-beta decay is surveyed. The results of the most sensitive experiments are discussed. Particular attention is given to describing the NEMO-3 detector, which is intended for seeking the neutrinoless double-beta decay of various isotopes (100Mo, 82Se, etc.) with a sensitivity as high as T 1/2 ∼ 1025 yr, which corresponds to a sensitivity to the Majorana neutrino mass at a level of 0.1 to 0.3 eV. The first results obtained with the NEMO-3 detector are presented. A review of the existing projects of double-beta-decay experiments where it is planned to reach a sensitivity to the Majorana neutrino mass at a level of 0.01 to 0.1 eV is given.
Similar content being viewed by others
References
H. V. Klapdor-Kleingrothaus, J. Hellmig, and M. Hirsch, J. Phys. G 24, 483 (1998).
A. Faessler and F. Simkovic, Prog. Part. Nucl. Phys. 46, 233 (2001).
J. D. Vergados, Phys. Rep. 361, 1 (2002).
H. Sobel et al., Nucl. Phys. B (Proc. Suppl.) 91, 127 (2001).
B. T. Cleveland et al., Astrophys. J. 496, 505 (1998).
S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001); 86, 5656 (2001).
V. N. Gavrin et al., Nucl. Phys. B (Proc. Suppl.) 91, 36 (2001).
M. Altman et al., Phys. Lett. B 490, 16 (2000).
Q. R. Ahmad et al., Phys. Rev. Lett. 89, 011301 (2002); 89, 011302 (2002).
P. C. de Holanda and A. Yu. Smirnov, Phys. Rev. D 66, 113005 (2002).
J. N. Bahcall et al., hep-ph/0204314.
M. Maltoni et al., hep-ph/0207227.
K. Eguchi et al., hep-ex/0212021.
A. Yu. Smirnov, Czech. J. Phys. 52, 439 (2002).
S. Pascoli, S. T. Petcov, and W. Rodejohann, hep-ph/0209059.
B. Kayser, hep-ph/0211134.
A. S. Barabash, Pis'ma Zh. Éksp. Teor. Fiz. 68, 3 (1998) [JETP Lett. 68, 1 (1998)].
A. S. Barabash, Eur. Phys. J. A 8, 137 (2000).
G. Gelmini and M. Roncadelli, Phys. Lett. B 99B, 1411 (1981).
R. N. Mohapatra and P. B. Pal, Massive Neutrinos in Physics and Astrophysics (World Sci., Singapore, 1991).
Z. G. Berezhiani, A. Yu. Smirnov, and J. W. F. Valle, Phys. Lett. B 291, 99 (1992).
R. N. Mohapatra and E. Takasugi, Phys. Lett. B 211, 192 (1988).
C. P. Burgess and J. M. Cline, Phys. Lett. B 298, 141 (1993); Phys. Rev. D 49, 5925 (1994).
P. Bamert, C. P. Burgess, and R. N. Mohapatra, Nucl. Phys. B 449, 25 (1995).
C. D. Carone, Phys. Lett. B 308, 85 (1993).
R. N. Mohapatra, A. Perez-Lorenzana, and C. A. S. Pires, Phys. Lett. B 491, 143 (2000).
V. I. Tretyak and Yu. G. Zdesenko, At. Data Nucl. Data Tables 80, 83 (2002).
E. L. Fireman, Phys. Rev. 74, 1238 (1948).
M. G. Inghram and J. H. Reynolds, Phys. Rev. 76, 1265 (1949); 78, 822 (1950).
T. Kirsten, W. Gentner, and O. A. Schaeffer, Z. Phys. 202, 273 (1967).
S. R. Elliott, A. A. Hahn, and M. K. Moe, Phys. Rev. Lett. 59, 2020 (1987).
A. S. Barabash et al., Phys. Lett. B 345, 408 (1995).
A. L. Turkevich, T. E. Economou, and G. A. Cowan, Phys. Rev. Lett. 67, 3211 (1991).
A. Kawashima, K. Takahashi, and A. Masuda, Phys. Rev. C 47, 2452 (1993).
M. E. Wieser and J. R. De Laeter, Phys. Rev. C 64, 024308 (2001).
A. S. Barabash, Czech. J. Phys. 52, 567 (2002).
A. A. Vasenko et al., Mod. Phys. Lett. A 5, 1299 (1990).
H. V. Klapdor-Kleingrothaus et al., Eur. Phys. J. A 12, 147 (2001).
H. V. Klapdor-Kleingrothaus et al., Mod. Phys. Lett. A 16, 2409 (2001).
C. E. Aalseth et al., Mod. Phys. Lett. A 17, 1475 (2002).
F. Feruglio, A. Strumia, and F. Vissani, Nucl. Phys. B 637, 345 (2002).
Yu. G. Zdesenko, F. A. Danevich, and V. I. Tretyak, Phys. Lett. B 546, 206 (2002).
C. E. Aalseth et al., Phys. Rev. C 65, 092007 (2002).
R. Luescher et al., Phys. Lett. B 434, 407 (1998).
C. Arnaboldi et al., hep-ex/0211071.
F. A. Danevich et al., Phys. Rev. C 62, 045501 (2000).
NEMO Collab.
F. Simkovic et al., Phys. Rev. C 60, 055502 (1999).
J. Suhonen, Phys. Lett. B 477, 99 (2000).
J. Suhonen, Phys. Rev. C 62, 042501 (2000).
S. Stoica and H. V. Klapdor-Kleingrothaus, Nucl. Phys. A 694, 269 (2001).
E. Caurier et al., Nucl. Phys. A 654, 973c (1999).
J. H. Hirsch, O. Castanos, and P. O. Hess, Nucl. Phys. A 582, 124 (1995).
J. Suhonen and O. Sivitarese, Phys. Rep. 300, 123 (1998).
K. You et al., Phys. Lett. B 265, 53 (1991).
S. R. Elliot et al., Phys. Rev. C 46, 1535 (1992).
R. Arnold et al., Nucl. Phys. A 658, 299 (1999).
O. K. Manuel, J. Phys. G 17, 221 (1991).
A. De Silva, M. K. Moe, M. A. Nelson, and M. A. Vient, Phys. Rev. C 56, 2451 (1997).
A. S. Barabash, Phys. Lett. B 216, 257 (1989).
R. Arnold et al., Nucl. Phys. A 636, 209 (1998).
M. Hirsch et al., Phys. Lett. B 372, 8 (1996).
M. Gunther et al., Phys. Rev. D 55, 54 (1997).
R. Arnold et al., Nucl. Phys. A 678, 341 (2000).
J. Tanaka and H. Ejiri, Phys. Rev. D 48, 5412 (1993).
O. Cremonesi, hep-ex/0210007.
B. Maier, Nucl. Phys. B (Proc. Suppl.) 35, 358 (1994).
S. K. Dhiman and P. K. Raina, Phys. Rev. C 50, R2660 (1994).
O. Civitarese and J. Suhonen, Nucl. Phys. A 575, 251 (1994).
J. Toivanen and J. Suhonen, Phys. Rev. C 55, 2314 (1997).
C. E. Aalseth et al., hep-ex/0201021.
C. Arnaboldi et al., hep-ex/0212053.
H. V. Klapdor-Kleingrothaus et al., hep-ph/0103074.
A. Piepke, Nucl. Phys. B (Proc. Suppl.) 91, 99 (2001).
R. S. Raghavan, Phys. Rev. Lett. 72, 1411 (1994).
B. Caccianiga and M. G. Giammarchi, Astropart. Phys. 14, 15 (2000).
A. Bakalyarov et al., Pis'ma Zh. Éksp. Teor. Fiz. 76, 643 (2002) [JETP Lett. 76, 545 (2002)].
A. S. Barabash et al., Z. Phys. A 352, 231 (1995).
A. A. Klimenko et al., Czech. J. Phys. 52, 589 (2002).
A. Morales et al., Nuovo Cimento A 100, 525 (1988).
J. Suhonen et al., Z. Phys. A 358, 297 (1997).
A. S. Barabash et al., J. Phys. G 22, 487 (1996).
H. Ejiri et al., Nucl. Phys. A 611, 85 (1996).
A. Piepke et al., Nucl. Phys. A 577, 121 (1994).
A. S. Barabash, A. V. Kopylov, and V. I. Cherehovsky, Phys. Lett. B 249, 186 (1990).
E. Bellotti et al., Europhys. Lett. 3, 889 (1987).
A. S. Barabash et al., Eur. Phys. J. A 11, 143 (2001).
E. Bellotti et al., J. Phys. G 17, S231 (1991).
C. Arpesella et al., Nucl. Phys. B (Proc. Suppl.) 70, 249 (1999).
C. Arpesella et al., Nucl. Phys. B (Proc. Suppl.) 48, 247 (1996).
E. Bellotti et al., Lett. Nuovo Cimento 33, 273 (1982).
M. Doi and T. Kotani, Prog. Theor. Phys. 87, 1207 (1992).
J. Suhonen, Phys. Rev. C 48, 574 (1993).
M. Hirsch et al., Z. Phys. A 347, 151 (1994).
A. S. Barabash, Pis'ma Zh. Éksp. Teor. Fiz. 59, 644 (1994) [JETP Lett. 59, 677 (1994)].
A. S. Barabash and R. R. Saakyan, Yad. Fiz. 59, 197 (1996) [Phys. At. Nucl. 59, 179 (1996)].
E. B. Norman and M. A. De Faccio, Phys. Lett. B 148B, 31 (1984).
A. P. Meshik et al., Phys. Rev. C 64, 035205 (2001).
C. Saenz et al., Phys. Rev. C 50, 1170 (1994).
S. I. Vasil'ev et al., Pis'ma Zh. Éksp. Teor. Fiz. 57, 614 (1993) [JETP Lett. 57, 320 (1993)].
P. Belli et al., Astropart. Phys. 10, 115 (1999).
A. S. Barabash et al., Z. Phys. A 357, 351 (1997).
H. Ejiri et al., Phys. Rev. C 63, 065501 (2001).
H. Ejiri et al., Phys. Lett. B 531, 190 (2002).
C. Brofferio et al., Czech. J. Phys. 52, 531 (2002).
V. A. Artemiev et al., Yad. Fiz. 63, 1312 (2000) [Phys. At. Nucl. 63, 1238 (2000)].
NEMO-3 Proposal, Preprint No. 94-29, LAL (Orsay, 1994).
NEMO Collab., Preprint No. 02-30, LAL (Orsay, 2002).
R. Arnold et al., Nucl. Instrum. Methods Phys. Res. A 354, 338 (1995).
A. S. Barabash, Czech. J. Phys. 52, 575 (2002).
M. Danilov et al., Phys. Lett. B 480, 12 (2000).
M. Moe, Phys. Rev. C 44, R931 (1991).
H. Ejiri, Phys. Rev. Lett. 85, 2917 (2000).
G. Bellini et al., Phys. Lett. B 493, 216 (2000).
Author information
Authors and Affiliations
Additional information
__________
Translated from Yadernaya Fizika, Vol. 67, No. 3, 2004, pp. 458–472.
Original Russian Text Copyright © 2004 by Barabash.
Rights and permissions
About this article
Cite this article
Barabash, A.S. Double-beta-decay experiments: Present status and prospects for the future. Phys. Atom. Nuclei 67, 438–452 (2004). https://doi.org/10.1134/1.1690048
Received:
Issue Date:
DOI: https://doi.org/10.1134/1.1690048