Search for diffuse neutrino flux from astrophysical sources with MACRO

被引:36
作者
Ambrosio, M
Antolini, R
Auriemma, G
Bakari, D
Baldini, A
Barbarino, GC
Barish, BC
Battistoni, G
Becherini, Y
Bellotti, R
Bemporad, C
Bernardini, P
Bilokon, H
Bloise, C
Bower, C
Brigida, M
Bussino, S
Cafagna, F
Calicchio, M
Campana, D
Carboni, M
Caruso, R
Cecchini, S
Cei, F
Chiarella, V
Choudhary, BC
Coutu, S
Cozzi, M
De Cataldo, G
Dekhissi, H
De Marzo, C
De Mitri, I
Derkaoui, J
De Vincenzi, M
Di Credico, A
Erriquez, O
Favuzzi, C
Forti, C
Fusco, P
Giacomelli, G
Giannini, G
Giglietto, N
Giorgini, M
Grassi, M
Grillo, A
Guarino, F
Gustavino, C
Habig, A
Hanson, K
Heinz, R
机构
[1] Univ Naples Federico II, Dipartimento Fis, I-80125 Naples, Italy
[2] Ist Nazl Fis Nucl, I-80125 Naples, Italy
[3] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Laquila, Italy
[4] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[5] Ist Nazl Fis Nucl, I-00185 Rome, Italy
[6] Univ Basilicata, I-85100 Potenza, Italy
[7] Univ Bologna, Dipartimento Fis, I-40126 Bologna, Italy
[8] Ist Nazl Fis Nucl, I-40126 Bologna, Italy
[9] Univ Mohammed 1, Fac Sci, LPTP, Oujda, Morocco
[10] Univ Pisa, Dipartimento Fis, I-56010 Pisa, Italy
[11] Ist Nazl Fis Nucl, I-56010 Pisa, Italy
[12] CALTECH, Pasadena, CA 91125 USA
[13] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[14] Ist Nazl Fis Nucl, I-20133 Milan, Italy
[15] Univ Bari, Dipartimento Fis, I-70126 Bari, Italy
[16] INFN, I-70126 Bari, Italy
[17] Univ Lecce, Dipartimento Fis, I-73100 Lecce, Italy
[18] Ist Nazl Fis Nucl, Sez Lecce, I-73100 Lecce, Italy
[19] Indiana Univ, Dept Phys & Astron, Bloomington, IN 47405 USA
[20] Univ Roma Tre, Dipartimento Fis, I-00146 Rome, Italy
[21] Ist Nazl Fis Nucl, Sez Roma Tre, I-00146 Rome, Italy
[22] Univ Aquila, Dipartimento Fis, I-67100 Laquila, Italy
[23] Ist Nazl Fis Nucl, I-67100 Laquila, Italy
[24] CNR, Ist IASF, I-40129 Bologna, Italy
[25] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[26] Penn State Univ, Dept Phys, University Pk, PA 16801 USA
[27] Univ Trieste, I-34100 Trieste, Italy
[28] Ist Nazl Fis Nucl, I-34100 Trieste, Italy
[29] Boston Univ, Dept Phys, Boston, MA 02215 USA
[30] Univ Minnesota, Duluth Phys Dept, Duluth, MN 55812 USA
[31] Univ Rome, Dipartimento Energet, I-00185 Rome, Italy
[32] MIT, Dept Phys, Cambridge, MA 02139 USA
[33] Intervideo Inc, Torrance, CA 90505 USA
[34] Univ Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
[35] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA
[36] Macalester Coll, Dept Phys & Astron, St Paul, MN 55105 USA
[37] Univ Turin, Dipartimento Fis Sperimentale, I-10125 Turin, Italy
[38] Ist Nazl Fis Nucl, I-10125 Turin, Italy
[39] Inst Space Sci, Bucharest 76900, Romania
[40] Univ Piemonte Orientale, Dipartimento Sci & Tecnol Avanzate, I-1500 Alessandria, Italy
[41] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[42] Resonance Photon, Markham, ON L3R 5B1, Canada
基金
美国国家科学基金会;
关键词
neutrino; AGNs; GRBs;
D O I
10.1016/S0927-6505(02)00190-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Many galactic and extragalactic astrophysical sources are currently considered promising candidates as high-energy neutrino emitters. Astrophysical neutrinos can be detected as upward-going muons produced in charged-current interactions with the medium surrounding the detector. The expected neutrino fluxes from various models start to dominate on the atmospheric neutrino background at neutrino energies above some tens of TeV. We present the results of a search for an excess of high-energy upward-going muons among the sample of data collected by MACRO during similar to5.8 years of effective running time. No significant evidence for this signal was found. As a consequence, an upper limit on the flux of upward-going muons from high-energy neutrinos was set at the level of 1.7 x 10(-14) cm(-2) s(-1) sr(-1). The corresponding upper limit for the diffuse neutrino flux was evaluated assuming a neutrino power law spectrum. Our result was compared with theoretical predictions and upper limits from other experiments. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:1 / 13
页数:13
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