Results from the antarctic Muon and neutrino detector array

被引：110

作者：

Cowen, DF

Ahrens, J

Bai, X

Barwick, SW

Becka, T

Becker, KH

Bernardini, E

Bertrand, D

Binon, F

Biron, A

Böser, S

Botner, O

Bouhali, O

Burgess, T

Carius, S

Castermans, T

Chen, A

Chirkin, D

Conrad, J

Cooley, J

Cowen, DF

Davour, A

De Clercq, C

DeYoung, T

Desiati, P

Dewulf, JP

Doksus, P

Ekström, P

Feser, T

Gaisser, TK

Gaug, M

Gerhardt, L

Goldschmidt, A

Hallgren, A

Halzen, F

Hanson, K

Hardtke, R

Hauschildt, T

Hellwig, M

Herquet, P

Hill, GC

Hulth, PO

Hundertmark, S

Jacobsen, J

Karle, A

Koci, B

Köpke, L

Kuehn, K

Kowalski, M

Lamoureux, JI

机构：

[1] Johannes Gutenberg Univ Mainz, Inst Phys, D-55099 Mainz, Germany

[2] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

[3] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[4] Berg Univ Wuppertal, Fachbereich Phys 8, D-42097 Wuppertal, Germany

[5] DESY, D-15735 Zeuthen, Germany

[6] Free Univ Brussels, Fac Sci, B-1050 Brussels, Belgium

[7] Uppsala Univ, Div High Energy Phys, S-75121 Uppsala, Sweden

[8] Univ Stockholm, SCFAB, Dept Phys, SE-10691 Stockholm, Sweden

[9] Kalmar Univ, Dept Technol, S-39182 Kalmar, Sweden

[10] Univ Mons, B-7000 Mons, Belgium

[11] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[12] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[13] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[14] Free Univ Brussels, Dienst ELEM, B-1050 Brussels, Belgium

[15] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA

[16] Univ Wisconsin, Dept Phys, River Falls, WI 54022 USA

[17] Univ Simon Bolivar, Dept Fis, Caracas 1080A, Venezuela

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2003年 / 118卷

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0920-5632(03)01335-5

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：

We show new results from both the older and newer incarnations of AMANDA (AMANDA-B10 and AMANDA-II, respectively). These results demonstrate that AMANDA is a functioning, multipurpose detector with significant physics and astrophysics reach. They include a new higher-statistics measurement of the atmospheric muon neutrino flux and preliminary results from searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, gamma-ray bursters and diffuse sources producing muons in the detector, and diffuse sources producing electromagnetic or hadronic showers in or near the detector.

引用

页码：371 / 379

页数：9

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