Global Constraints on Neutrino Masses and Their Ordering

被引:0
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作者
Marrone, Antonio [4 ,5 ]
Capozzi, Francesco [1 ]
Di Valentino, Eleonora [2 ,3 ]
Lisi, Eligio [4 ]
Melchiorri, Alessandro [6 ,7 ]
Palazzo, Antonio [5 ]
机构
[1] Ohio State Univ, Dept Phys, 174 W 18th Ave, Columbus, OH 43210 USA
[2] CNRS, Inst Astrophys Paris, UMR7095, F-75014 Paris, France
[3] UPMC Sorbonne Univ, F-75014 Paris, France
[4] Ist Nazl Fis Nucl, Sez Bari, Via Orabona 4, I-70126 Bari, Italy
[5] Dipartimento Interateneo Fis Michelangelo Merlin, Via Amendola 173, I-70126 Bari, Italy
[6] Univ Roma La Sapienza, Dipartimento Fis, Ple Aldo Moro 2, I-00185 Rome, Italy
[7] Ist Nazl Fis Nucl, Sez Roma 1, Ple Aldo Moro 2, I-00185 Rome, Italy
来源
WORKSHOP ON CALCULATION OF DOUBLE-BETA-DECAY MATRIX ELEMENTS (MEDEX'17) | 2017年 / 1894卷
关键词
D O I
10.1063/1.5007640
中图分类号
O59 [应用物理学];
学科分类号
摘要
In this work we focus on the absolute neutrino masses and their ordering, still not known in the standard phenomenology of three massive neutrinos. Interesting constraints on the sum of neutrino masses and on mass ordering (either normal, NO or inverted, IO) can be derived from the combination of neutrino oscillation data, neutrinoless double beta (0 nu beta beta) decay experiments, and cosmological data. We derive current bounds on absolute neutrino mass observables by combining in a global data analysis the latest results from oscillation experiments, 0 nu beta beta decay limits from the KamLAND-Zen experiment, and constraints from Planck measurements and other cosmological data sets. We found that NO appears to be favored with respect to IO at the level of similar to 2 sigma, mainly by neutrino oscillation data (especially atmospheric), corroborated by cosmological data in some cases.
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页数:4
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