Study of neutrino electromagnetic properties with the prototype of the Borexino detector

被引：23

作者：

Back, HO ^{[1
]}

Balata, M

de Bari, A

Beau, T

de Bellefon, A

Bellini, G

Benziger, J

Bonetti, S

Buck, C

Caccianiga, B

Cadonati, L

Calaprice, F

Cecchet, G

Chen, M

Di Credico, A

Dadoun, O

D'Angelo, D

Derbin, A

Deutsch, M

Elisei, F

Etenko, A

von Feilitzsch, F

Fernholz, R

Ford, R

Franco, D

Freudiger, B

Galbiati, C

Gatti, F

Gazzana, S

Giammarchi, MG

Giugni, D

Goeger-Neff, M

Goretti, A

Grieb, C

Hagner, C

Harding, E

Heusser, G

Ianni, A

Ianni, AM

de Kerret, H

Kiko, J

Kirsten, T

Kobychev, V

Korga, G

Korschinek, G

Kozlov, Y

Kryn, D

Laubenstein, M

Lendvai, C

Lombardi, P

机构：

[1] Virginia Polytech Inst & State Univ, Blacksburg, VA 24061 USA

[2] LNGS SS, I-67010 Assergi, AQ, Italy

[3] Univ Pavia, Dipartimento Fis Nucl & Teor, I-27100 Pavia, Italy

[4] Lab Phys Corpusculaire & Cosmol, F-75231 Paris, France

[5] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy

[6] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[7] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany

[8] Queens Univ, Dept Phys, Kingston, ON K7L 3N6, Canada

[9] Tech Univ Munich, D-85747 Garching, Germany

[10] Joint Inst Nucl Res, Dubna 141980, Russia

[11] MIT, Dept Phys, Cambridge, MA 02139 USA

[12] Univ Perugia, Dipartimento Chim, I-06123 Perugia, Italy

[13] RRC Kurchatov Inst, Moscow 123182, Russia

[14] Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy

[15] Ist Nazl Fis Nucl, I-16146 Genoa, Italy

[16] KFKI, RMKI, H-1121 Budapest, Hungary

[17] Bell Labs, Lucent Technol, Murray Hill, NJ 07974 USA

[18] Jagiellonian Univ, M Smoluchowski Inst Phys, PL-30059 Krakow, Poland

来源：

PHYSICS LETTERS B | 2003年 / 563卷 / 1-2期

关键词：

solar neutrinos; charge radius; magnetic moment;

D O I：

10.1016/S0370-2693(03)00579-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The results of background measurements with the prototype of the Borexino detector (CTF) have been used to obtain an upper bound on the neutrino magnetic moment, mu(nu). The new upper limit for mu(nu) from pp and Be-7 solar neutrinos is (5.5 x 10(-10))mu(B) (90% c.l.) in the Standard Solar Model scenario. This is the first limit on mu(nu) obtained using sub-MeV neutrinos. The sensitivity of the prototype to the neutrino charge radius and the neutrino radiative decay are also presented. (C) 2003 Published by Elsevier Science B.V.

引用

页码：35 / 47

页数：13

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