Neutrinoless double beta decay and neutrino mass

被引:178
|
作者
Vergados, J. D. [1 ,2 ,3 ]
Ejiri, H. [4 ,5 ]
Simkovic, F. [6 ,7 ,8 ]
机构
[1] Univ Adelaide, Dept Phys, ARC Ctr Excellence Particle Phys CoEPP, Adelaide, SA 5005, Australia
[2] KAIST Univ, IBS, CAPP, Daejeon 305701, South Korea
[3] Tech Educ Inst, Board Trustees, Kozani, Greece
[4] Osaka Univ, RCNP, Osaka 5670047, Japan
[5] Czech Tech Univ, Nucl Sci, Prague, Czech Republic
[6] JINR, Theoret Phys Lab, Dubna 141980, Moscow Region, Russia
[7] Comenius Univ, Dept Nucl Phys & Biophys, Mlynska Dolina F1, SK-84215 Bratislava, Slovakia
[8] Czech Tech Univ, Prague 12800, Czech Republic
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS E | 2016年 / 25卷 / 11期
关键词
Majorana neutrino; neutrino mass; double data decay; nuclear matrix element; NUCLEAR-MATRIX-ELEMENTS; DOUBLE-ELECTRON-CAPTURE; QUASI-PARTICLE RPA; SHELL-MODEL; MAJORANA NEUTRINOS; LEPTON-NUMBER; 2-NU-BETA-BETA DECAY; EXCITED-STATES; MIXINGS STATUS; ECEC PROCESSES;
D O I
10.1142/S0218301316300071
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The observation of neutrinoless double beta decay (DBD) will have important consequences. First it will signal that lepton number is not conserved and the neutrinos are Majorana particles. Second, it represents our best hope for determining the absolute neutrino mass scale at the level of a few tens of meV. To achieve the last goal, however, certain hurdles have to be overcome involving particle, nuclear and experimental physics. Particle physics is important since it provides the mechanisms for neutrinoless DBD. In this review, we emphasize the light neutrino mass mechanism. Nuclear physics is important for extracting the useful information from the data. One must accurately evaluate the relevant nuclear matrix elements (NMEs), a formidable task. To this end, we review the recently developed sophisticated nuclear structure approaches, employing different methods and techniques of calculation. We also examine the question of quenching of the axial vector coupling constant, which may have important consequences on the size of the NMEs. From an experimental point of view it is challenging, since the life times are extremely long and one has to fight against formidable backgrounds. One needs large isotopically enriched sources and detectors with good energy resolution and very low background.
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页数:59
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