A SEARCH FOR ASTROPHYSICAL SOURCES OF LOW-ENERGY NEUTRINOS USING THE IMB DETECTOR

被引：7

作者：

MILLER, RS

BECKERSZENDY, R

BRATTON, CB

BREAULT, J

CASPER, D

DYE, ST

GAJEWSKI, W

GOLDHABER, M

HAINES, TJ

HALVERSON, PG

KIELCZEWSKA, D

KROPP, WR

LEARNED, JG

LOSECCO, J

MATSUNO, S

MATTHEWS, J

MCGRATH, G

MCGREW, C

PRICE, L

REINES, F

SCHULTZ, J

SINCLAIR, D

SOBEL, HW

STONE, JL

SULAK, LR

SVOBODA, R

VANDERVELDE, JC

机构：

[1] LOUISIANA STATE UNIV,BATON ROUGE,LA 70803

[2] SLAC,STANFORD,CA 94309

[3] CLEVELAND STATE UNIV,CLEVELAND,OH 44115

[4] UNIV CALIF IRVINE,IRVINE,CA 92717

[5] CERN,CH-1211 GENEVA 23,SWITZERLAND

[6] BOSTON UNIV,BOSTON,MA 02215

[7] BROOKHAVEN NATL LAB,UPTON,NY 11973

[8] UNIV MARYLAND,COLL PK,MD 20742

[9] UNIV WARSAW,PL-00325 WARSAW,POLAND

[10] UNIV HAWAII,HONOLULU,HI 96822

[11] UNIV NOTRE DAME,NOTRE DAME,IN 46556

[12] UNIV MICHIGAN,ANN ARBOR,MI 48109

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 428卷 / 02期

关键词：

ISM; COSMIC RAYS; ELEMENTARY PARTICLES; GAMMA-RAYS; BURSTS; SUPERNOVAE; GENERAL;

D O I：

10.1086/174272

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The temporal structure of low-energy (20-60 MeV) neutrino interactions within the IMB-3 detector during 863 days of livetime between 1986 May and 1991 March has been analyzed. The neutrino data are consistent with expected cosmic-ray-induced neutrino interactions with no bursts evident (excluding SN 1987A). When combined with the 327 effective livedays of IMB-1 data, we place a 90% C.L. upper limit of less-than-or-equal-to 0.71 Galactic supernovae yr-1. We have also performed a temporal correlation analysis with gamma-ray bursts (GRBs) using a subset of the low-energy neutrino data. No significant correlations were observed for coincidence windows of 1 minute, 1 hour, or 1 day.

引用

页码：629 / 632

页数：4

共 50 条

[21] Large-Volume Detector at the Baksan Neutrino Observatory for Studies of Natural Low-Energy Neutrinos as Geo- and Astrophysical Probes
Veresnikova, A. A.
Barabanov, I. R.
Bezrukov, L. B.
Gurentsov, V. I.
Sinev, V. V.
PHYSICS OF PARTICLES AND NUCLEI, 2018, 49 (04) : 678 - 684
[22] BOREXINO - A REAL-TIME DETECTOR FOR LOW-ENERGY SOLAR NEUTRINOS
BONETTI, S
NUCLEAR PHYSICS B, 1992, : 486 - 490
[23] NEW RESULTS ON DETECTOR DEVELOPMENTS FOR LOW-ENERGY NEUTRINOS AND DARK MATTER
GONZALEZMESTRES, L
PERRETGALLIX, D
QUEST FOR THE FUNDAMENTAL CONSTANTS IN COSMOLOGY, 1989, : 337 - 358
[24] BOREXINO - A REAL-TIME DETECTOR FOR LOW-ENERGY SOLAR NEUTRINOS
BENZIGER, JB
CALAPRICE, FP
BOGELAAR, RB
ABSTRACTS OF PAPERS OF THE AMERICAN CHEMICAL SOCIETY, 1994, 208 : 67 - NUCL
[25] High energy neutrinos from charm in astrophysical sources
Enberg, Rikard
Reno, Mary Hall
Sarcevic, Ina
PHYSICAL REVIEW D, 2009, 79 (05):
[26] High Energy Neutrinos from Charm in Astrophysical Sources
Sarcevic, Ina
INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS, 2009, 1182 : 40 - 43
[27] LOW-ENERGY ATMOSPHERIC NEUTRINOS
LEE, H
BLUDMAN, SA
PHYSICAL REVIEW D, 1988, 37 (01): : 122 - 125
[28] Type IIn supernovae as sources of high energy astrophysical neutrinos
Zirakashvili, V. N.
Ptuskin, V. S.
ASTROPARTICLE PHYSICS, 2016, 78 : 28 - 34
[29] Inferring the Flavor of High-Energy Astrophysical Neutrinos at Their Sources
Bustamante, Mauricio
Ahlers, Markus
PHYSICAL REVIEW LETTERS, 2019, 122 (24)
[30] High energy neutrinos from astrophysical sources: An upper bound
Waxman, E
Bahcall, J
PHYSICAL REVIEW D, 1999, 59 (02)

← 1 2 3 4 5 →