The Baikal neutrino experiment

被引：32

作者：

Avrorin, A. ^{[1
]}

Aynutdinov, V. ^{[1
]}

Balkanov, V. ^{[1
]}

Belolaptikov, I. ^{[4
]}

Berezhnev, S. ^{[3
]}

Bogorodsky, D. ^{[2
]}

Budnev, N. ^{[2
]}

Danilchenko, I. ^{[1
]}

Domogatsky, G. ^{[1
]}

Doroshenko, A. ^{[1
]}

Dyachok, A. ^{[2
]}

Dzhilkibaev, Zh ^{[1
]}

Ermakov, G. ^{[3
]}

Fialkovsky, S. ^{[6
]}

Gaponenko, O. ^{[1
]}

Golubkov, K. ^{[4
]}

Gres', O. ^{[2
]}

Gres', T. ^{[2
]}

Grishin, N. ^{[3
]}

Grishin, O. ^{[2
]}

Klabukov, A. ^{[1
]}

Klimov, A. ^{[8
]}

Kochanov, A. ^{[2
]}

Konischev, K. ^{[4
]}

Korobchenko, A. ^{[2
]}

Koshechkin, A. ^{[1
]}

Kulepov, V. ^{[6
]}

Kuleshov, D. ^{[1
]}

Kuzmichev, L. ^{[3
]}

Middell, E. ^{[5
]}

Mikheyev, S. ^{[1
]}

Milenin, M. ^{[6
]}

Mirgazov, R. ^{[2
]}

Osipova, E. ^{[3
]}

Pan'kov, A. ^{[2
]}

Pan'kov, L. ^{[2
]}

Panfilov, A. ^{[1
]}

Petukhov, D. ^{[1
]}

Pliskovsky, E. ^{[4
]}

Pokhil, P. ^{[1
]}

Poleschuk, V. ^{[1
]}

Popova, E. ^{[3
]}

Prosin, V. ^{[3
]}

Rozanov, M. ^{[7
]}

Rubtzov, V. ^{[2
]}

Sheifler, A. ^{[1
]}

Shirokov, A. ^{[3
]}

Shoibonov, B. ^{[4
]}

Spiering, Ch ^{[5
]}

Suvorova, O. ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

[2] Irkutsk State Univ, Irkutsk 664003, Russia

[3] Skobeltsyn Inst Nucl Phys MSU, Moscow, Russia

[4] Joint Inst Nucl Res, Dubna, Russia

[5] DESY, Zeuthen, Germany

[6] Nizhnii Novgorod State Tech Univ, Nizhnii Novgorod, Russia

[7] St Petersburg State Marine Univ, St Petersburg, Russia

[8] Kurchatov Inst, Moscow, Russia

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2011年 / 626卷

关键词：

Neutrino telescopes; Baikal; GAMMA-RAY BURSTS; TELESCOPE; SEARCH; PERSPECTIVES; NT200;

D O I：

10.1016/j.nima.2010.06.209

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

We review the status of the Lake Baikal Neutrino Experiment. Preparation towards a km(3)-scale Gigaton Volume Detector (GVD) in Lake Baikal is currently a central activity. As an important milestone, a km(3)-prototype string comprising of 12 optical modules and based on a completely new technology, has been installed and was put in operation together with NT200+ in April, 2009. We also present recent results from the long-term operation of NT200, including an improved limit on the diffuse astrophysical neutrino flux. (c) 2010 Elsevier B.V. All rights reserved.

引用

页码：S13 / S18

页数：6

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