Artigo Revisado por pares

An upper limit on the flux of extraterrestrial neutrinos

1987; IOP Publishing; Volume: 315; Linguagem: Inglês

10.1086/165146

ISSN

1538-4357

Autores

R. Svoboda, R. M. Bionta, Geoffrey Blewitt, C. B. Bratton, D. Casper, P. Chrysicopoulou, A. Ciocio, R. Claus, B. Cortez, S. Dye, S. Errede, G. W. Foster, W. Gajewski, K. S. Ganezer, M. Goldhaber, T. J. Haines, T.W. Jones, D. Kiełczewska, W. R. Kropp, J. G. Learned, J. M. LoSecco, J. Matthews, H. S. Park, F. Reines, J. Schultz, S. Seidel, E. Shumard, D. Sinclair, H. W. Sobel, J. L. Stone, L. Sulak, G. Thornton, J. C. van der Velde, C. Wuest,

Tópico(s)

Geophysics and Gravity Measurements

Resumo

view Abstract Citations (51) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS An Upper Limit on the Flux of Extraterrestrial Neutrons Svoboda, R. ; Bionta, R. M. ; Blewitt, G. ; Bratton, C. B. ; Casper, D. ; Chrysicopoulou, P. ; Ciocio, A. ; Claus, R. ; Cortez, B. ; Dye, S. T. ; Errede, S. ; Foster, G. W. ; Gajewski, W. ; Ganezer, K. S. ; Goldhaber, M. ; Haines, T. J. ; Jones, T. W. ; Kielczewska, D. ; Kropp, W. R. ; Learned, J. G. ; Losecco, J. M. ; Matthews, J. ; Park, H. S. ; Reines, F. ; Schultz, J. ; Seidel, S. ; Shumard, E. ; Sinclair, D. ; Sobel, H. W. ; Stone, J. L. ; Sulak, L. ; Thornton, G. ; van der Velde, J. C. ; Wuest, C. Abstract A search is made for neutrino-induced muons from Cyg X-3, Her X-1, LMC X-4, Vela X-1, Geminga (= 2CG 195+4), the Crab Nebula, Cen A, 3C 273, SS 433, and the center of our Galaxy using a large underground ring-imaging water Cerenkov detector. For this study, the detector is used to measure the track direction of upward-going muons (energy >2 GeV) produced by neutrino interactions in the surrounding rock. The measured flux is 2.41±0.21×10-13cm-2s-1sr-1 for zenith angles greater than 98°. This overall rate is consistent with that expected from ordinary cosmic-ray interactions with Earth's atmosphere, which is calculated to be 2.36±0.12 (statistical) ±0.35 (systematic) ×10-13cm-2sr-1. Upper limits are placed on the incident neutrino flux and luminosity of each object based on detailed computer simulations of the detector's effective area, efficiency, and energy threshold. Publication: The Astrophysical Journal Pub Date: April 1987 DOI: 10.1086/165146 Bibcode: 1987ApJ...315..420S Keywords: Cosmic Rays; Extraterrestrial Radiation; Neutrinos; Particle Flux Density; X Ray Sources; Crab Nebula; Milky Way Galaxy; Muons; Particle Tracks; Radiation Detectors; Space Radiation; COSMIC RAYS: GENERAL; NEUTRINOS; X-RAYS: SOURCES full text sources ADS | data products SIMBAD (10) NED (2)

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