KM3NeT: Toward a cubic kilometre volume neutrino telescope in the Mediterranean Sea

被引:2
作者
Markou, C. [1 ]
机构
[1] NCSR Demokritos, Inst Nucl Phys, GR-15310 Athens, Greece
关键词
Neutrino astronomy; Neutrino telescopes; KM3NeT;
D O I
10.1016/j.nima.2008.07.009
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
High energy neutrino astronomy is emerging as one of the most exciting options for studying astrophysical processes. To establish neutrino detectability from specific sources, neutrino telescopes of km(3) scale are needed. In order to complement the IceCube detector currently under construction in the South Pole, a corresponding Northern Hemisphere detector is needed. The three neutrino telescope projects in the Mediterranean, ANTARES, NEMO and NESTOR have joined forces in order to develop, prepare, construct and operate such a research facility, KM3NeT. To this end, the EU is funding a 3-year design study. In the present paper, the status of the design study is presented and options for the various technical problems are discussed. (C) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码:54 / 57
页数:4
相关论文
共 14 条
[1]   Operation and performance of the NESTOR test detector [J].
Aggouras, G ;
Anassontzis, EG ;
Ball, AE ;
Bourlis, G ;
Chinowsky, W ;
Fahrun, E ;
Grammatikakis, G ;
Green, C ;
Grieder, P ;
Katrivanos, P ;
Koske, P ;
Leisos, A ;
Ludvig, J ;
Markopoulos, E ;
Minkowsky, P ;
Nygren, D ;
Papageorgiou, K ;
Przybylski, G ;
Resvanis, LK ;
Siotis, I ;
Sopher, J ;
Staveris, T ;
Tsagli, V ;
Tsirigotis, A ;
Zhukovk, VA .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2005, 552 (03) :420-439
[2]  
AHARONIAN F, 2005, ASTROPH0511678 H E S
[3]   Detection of TeV γ-ray emission from the shell-type supernova remnant RX J0852.0-4622 with HESS [J].
Aharonian, FA ;
Akhperjanian, AGA ;
Bazer-Bachi, AR ;
Beilicke, MB ;
Benbow, WB ;
Berge, DB ;
Bernlöhr, K ;
Boisson, C ;
Bolz, O ;
Borrel, V ;
Braun, I ;
Breitling, F ;
Brown, AM ;
Chadwick, PM ;
Chounet, LM ;
Cornils, R ;
Costamante, L ;
Degrange, B ;
Dickinson, HJ ;
Djannati-Atai, A ;
Drury, LOC ;
Dubus, G ;
Emmanoulopoulos, D ;
Espigat, P ;
Feinstein, F ;
Fontaine, G ;
Fuchs, Y ;
Funk, S ;
Gallant, YA ;
Giebels, B ;
Gillessen, S ;
Glicenstein, JF ;
Goret, P ;
Hadjichristidis, C ;
Hauser, M ;
Heinzelmann, G ;
Henri, G ;
Hermann, G ;
Hinton, JA ;
Hofmann, W ;
Holleran, M ;
Horns, D ;
Jacholkowska, A ;
de Jager, OC ;
Khélifi, B ;
Komin, N ;
Konopelko, A ;
Latham, IJ ;
Le Gallou, R ;
Lemière, A .
ASTRONOMY & ASTROPHYSICS, 2005, 437 (01) :L7-L10
[4]  
ANASSONTZIS E, 2005, P VER LARG VOL NEUTR
[5]  
BRAEM A, CERNPHEP2006025
[6]  
CHIARUSI T, 2005, P INT COSM RAY C ICR
[7]   Potential neutrino signals from galactic γ-ray sources [J].
Kappes, Alexander ;
Hinton, Jim ;
Stegmann, Christian ;
Aharonian, Felix A. .
ASTROPHYSICAL JOURNAL, 2007, 656 (02) :870-878
[8]   Guaranteed and prospective Galactic TeV neutrino sources [J].
Kistler, Matthew D. ;
Beacom, John F. .
PHYSICAL REVIEW D, 2006, 74 (06)
[9]  
KOOIJMAN P, 2007, P INT COSM RAY C ICR
[10]  
KUCH S, 2007, THESIS U ERLANGEN NU