NOSTOS: A new low-energy neutrino experiment

被引：0

作者：

Aune, S ^{[1
]}

Busto, J ^{[1
]}

Colas, P ^{[1
]}

Dolbeau, J ^{[1
]}

Fanourakis, G ^{[1
]}

Ribas, EF ^{[1
]}

Van Der Graaf, H ^{[1
]}

Geralis, T ^{[1
]}

Giomataris, Y ^{[1
]}

Gorodetzky, P ^{[1
]}

Gounaris, GJ ^{[1
]}

Irastorza, IG ^{[1
]}

Kousouris, K ^{[1
]}

Lepeltier, V ^{[1
]}

Patzak, T ^{[1
]}

Paschos, EA ^{[1
]}

Peyaud, B ^{[1
]}

Salin, P ^{[1
]}

Vergados, JD ^{[1
]}

机构：

[1] CEA Saclay, Ctr Etud Saclay, DAPNIA, F-91191 Gif Sur Yvette, France

来源：

IDENTIFICATION OF DARK MATTER | 2005年

关键词：

D O I：

10.1142/9789812701848_0091

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A novel low-energy (a few keV) neutrino-oscillation experiment NOSTOS, combining a strong tritium source and a high pressure spherical TPC detector of 10 m in radius has been recently proposed. The neutrino oscillation of such energies occurs within the detector itself enabling a very precise measurement of the oscillation parameters, and in particular the mixing angle theta(13). This detector could also be sensitive to the neutrino magnetic moment and capable of accurately measure the Weinberg angle at very low energy transfer. The same apparatus filled with high pressure Xenon, would exhibit a high sensitivity as a supernova neutrino detector. Results of a first prototype in operation will be shown in this paper.

引用

页码：607 / 614

页数：8

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