Observables sensitive to absolute neutrino masses. II

被引：165

作者：

Fogli, G. L. ^{[1
,2
]}

Lisi, E. ^{[2
]}

Marrone, A. ^{[1
,2
]}

Melchiorri, A. ^{[3
,4
]}

Palazzo, A. ^{[5
]}

Rotunno, A. M. ^{[1
,2
]}

Serra, P. ^{[6
]}

Silk, J.

Slosar, A. ^{[7
]}

机构：

[1] Univ Bari, Dipartmento Fis, I-70126 Bari, Italy

[2] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[3] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy

[4] Univ Roma La Sapienza, Sez INFN, I-00185 Rome, Italy

[5] Univ Valencia, CSIC, Inst Fis Corpuscular, AHEP Grp, Valencia 46071, Spain

[6] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[7] Univ Calif Berkeley, Dept Phys, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA

来源：

PHYSICAL REVIEW D | 2008年 / 78卷 / 03期

关键词：

D O I：

10.1103/PhysRevD.78.033010

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this followup to Phys. Rev. D 75, 053001 (2007) , we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0 nu 2 beta decay results in Ge-76 claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0 nu 2 beta limits in Te-130 recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.

引用

页数：5

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