The AMANDA neutrino telescope

被引：6

作者：

Andrés, EC ^{[1
]}

Askebjer, P

Barwick, SW

Bay, RC

Bergström, L

Biron, A

Booth, J

Botner, O

Bouchta, A

Carius, S

Carlson, M

Chinowsky, W

Chirkin, D

Conrad, J

Costa, CGS

Cowen, D

Dalberg, E

DeYoung, T

Edsjö, J

Ekström, P

Goobar, A

Gray, L

Hallgren, A

Halzen, F

Hardtke, R

Hart, S

He, Y

de los Heros, CP

Hill, G

Hulth, PO

Hundertmark, S

Jacobsen, J

Jones, A

Kandhadai, V

Karle, A

Kim, J

Leich, H

Leuthold, M

Lindahl, P

Liubarsky, I

Loaiza, P

Lowder, D

Marciniewski, P

Miller, TC

Miocinovic, P

Mock, PC

Morse, R

Newcomer, M

Niessen, P

Nygren, D

机构：

[1] Univ Stockholm, S-10691 Stockholm, Sweden

[2] Univ Calif Berkeley, Berkeley, CA 94720 USA

[3] Univ Calif Irvine, Irvine, CA 92717 USA

[4] Univ Penn, Philadelphia, PA 19104 USA

[5] Univ Wisconsin, Madison, WI 53706 USA

[6] Uppsala Univ, Uppsala, Sweden

[7] Kalmar Univ, Kalmar, Sweden

[8] DESY, Inst High Energy Phys, Hamburg, Germany

[9] Lawrence Berkeley Lab, Berkeley, CA 94720 USA

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 77卷

关键词：

D O I：

10.1016/S0920-5632(99)00469-7

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

With an effective telescope area of order 10(4) m(2) for TeV neutrinos, a threshold near similar to 50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

引用

页码：474 / 485

页数：12

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