First real-time detection of solar pp neutrinos by Borexino

被引：0

作者：

Pallavicini, M. ^{[1
,2
]}

Bellini, G. ^{[3
,4
]}

Benziger, J. ^{[5
]}

Bick, D. ^{[6
]}

Bonfini, G. ^{[7
]}

Bravo, D. ^{[8
]}

Caccianiga, B. ^{[3
,4
]}

Calaprice, F. ^{[9
]}

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

Cavalcante, P. ^{[7
]}

Chavarria, A. ^{[9
]}

Chepurnov, A. ^{[10
]}

D'Angelo, D. ^{[3
,4
]}

Davini, S. ^{[11
]}

Derbin, A. ^{[12
]}

Empl, A. ^{[11
]}

Etenko, A. ^{[13
]}

Fomenko, K. ^{[7
,14
]}

Franco, D. ^{[15
]}

Gabriele, F. ^{[7
]}

Galbiati, C. ^{[9
]}

Gazzana, S. ^{[7
]}

Ghiano, C. ^{[1
,2
]}

Giammarchi, M. ^{[3
,4
]}

Goeger-Neff, M. ^{[16
]}

Goretti, A. ^{[9
]}

Gromov, M. ^{[10
]}

Hagner, C. ^{[6
]}

Hungerford, E. ^{[11
]}

Ianni, Al. ^{[7
]}

Ianni, An. ^{[9
]}

Kayser, M. ^{[6
]}

Kobychev, V. ^{[26
]}

Korablev, D. ^{[14
]}

Korga, G. ^{[12
]}

Kryn, D. ^{[15
]}

Laubenstein, M. ^{[7
]}

Lehnert, B. ^{[18
]}

Lewke, T. ^{[16
]}

Litvinovich, E. ^{[17
]}

Lombardi, F. ^{[7
]}

Lombardi, P. ^{[3
,4
]}

Ludhova, L. ^{[3
,4
]}

Lukyanchenko, G. ^{[13
]}

Machulin, I. ^{[17
]}

Manecki, S. ^{[8
]}

Maneschg, W. ^{[20
,21
]}

Marcocci, S. ^{[25
]}

Meindl, Q. ^{[6
]}

Meroni, E. ^{[3
,4
]}

机构：

[1] Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy

[2] Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

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

[4] Ist Nazl Fis Nucl, I-20133 Milan, Italy

[5] Princeton Univ, Dept Chem Engn, Princeton, NJ 08544 USA

[6] Univ Hamburg, Inst Expt Phys, Hamburg, Germany

[7] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Assergi, Italy

[8] Virginia Polytech Inst & State Univ, Dept Phys, Blacksburg, VA 24061 USA

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

[10] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119234, Russia

[11] Univ Houston, Dept Phys, Houston, TX 77204 USA

[12] St Petersburg Nucl Phys Inst, Gatchina 188350, Russia

[13] NRC Kurchatov Inst, Moscow 123182, Russia

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

[15] Univ Paris Diderot, Observ Paris, APC, CNRS IN2P3,CEA Irfu,Sorbonne Paris Cite, Paris, France

[16] Tech Univ Munich, Phys Dept, D-85747 Garching, Germany

[17] Natl Nucl Res Univ MEPhI, 31 Kashirskoe Shosse, Moscow, Russia

[18] Tech Univ Dresden, Inst Kern & Teilchenphys, Zellescher Weg 19, D-01068 Dresden, Germany

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

[20] Univ Perugia, Dipartimento Chim Biol & Biotecnol, I-06123 Perugia, Italy

[21] Ist Nazl Fis Nucl, I-06123 Perugia, Italy

[22] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA

[23] Univ Calif Los Angeles, Phys Ans Astron Dept, Los Angeles, CA 90095 USA

[24] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany

[25] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy

[26] Kiev Inst Nucl Res, UA-06380 Kiev, Ukraine

来源：

ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS 2014 (RICAP-14) | 2016年 / 121卷

基金：

美国国家科学基金会;

关键词：

D O I：

10.1051/epjconf/201612101001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra-pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.

引用

页数：8

共 50 条

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