6533b834fe1ef96bd129ce40
RESEARCH PRODUCT
Rejection Power of A Horizontal Rpc Telescope For Left and Right Coming Cosmic Muons
G. C. BarbarinoM. AmbrosioA. LanzaP. PistilliR. SantonicoL. ScarsiF. RomanoG. BressiF. D'aquinoA. NigroRoberto CardarelliF. GuarinoSalvatore NuzzoV. SilvestriniG. MariniM. IacovacciB. BartoliMichele GuidaGiuseppe IaselliD. CampanaM. BonoriA. RanieriG. OsteriaS. Del Sordosubject
PhysicsNuclear and High Energy PhysicsResistive touchscreenCOSMIC cancer databaseMuonPhysics::Instrumentation and DetectorsSURFACE NEUTRINO DETECTORAstrophysics::High Energy Astrophysical PhenomenaTrack (disk drive)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyKAMIOKANDE-II DETECTORlaw.inventionTelescopeNEUTRINOSlawHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyInstrumentationdescription
Abstract The possibility of performing neutrino astronomy by means of a detector above the ground depends critically on the feasibility of a rejection power on the order of 10 11 required to discriminate the enormous background of cosmic downward going muons from the signal of upward going muons produced by neutrinos. In order to check whether and how this rejection is obtainable, we have built in the Physics Department of the University of Bari a horizontal cosmic muon telescope (MINI) instrumented with resistive plate counters. By performing time-of-flight measurements, we have estimated the rejection power of our telescope for left and right coming cosmic muons. The rejection dependence on a few fundamental parameters like minimum number of points per track, telescope length, RPC time resolution and on trigger configuration has been investigated.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 1993-01-01 |