On the Capability Of SuperKamiokande Detector To Define the Primary Parameters Of Muon And Electron Events
نویسنده
چکیده
We develop a new discrimination procedure for separating electron neutrinos from muon neutrinos, based on detailed simulations carried out with GEANT 3.21 and with newly derived mean angular distribution functions for the charged particles concerned (muons and electrons/positrons), as well as the corresponding functions for the relative fluctuations. These angular distribution functions are constructed introducing a “moving point” approximation. Using our type definition procedure we are able to discriminate muons from electrons in Fully Contained Events with a probability of error of less than several %. At the same time, our geometrical reconstruction procedure, considering only the ring-like structure of the Cherenkov image, gives an unsatisfactory resolution for 1 GeV e and μ, with a mean vertex position error, δr, of 5–10m and a mean directional error, δθ, of about 6◦–20◦. In contrast, a geometrical reconstruction procedure utilizing the full image and using a detailed approximation of the event angular distribution works much better: for a 1 GeV e, δr ∼2m and δθ ∼3◦; for a 1 GeV μ, δr ∼3m and δθ ∼5◦. At 5 GeV, the corresponding values are ∼1.4m and ∼2◦ for e and ∼2.9m and ∼4.3◦ for μ. The numerical values depend on a single PMT contribution threshold. The values quoted above are the minima with respect to this threshold. Even the methodologically correct approach we have adopted, based on detailed simulations using closer approximations than those adopted in the SK analysis, cannot reproduce the accuracies for particle discrimination, momentum resolution, interaction vertex location, and angular resolution obtained by the SK simulations, suggesting the assumptions in these may be inadequate. PACS numbers: 13.15.+g, 14.60.-z
منابع مشابه
Investigating the capability of plastic scintillation detectors in design of a muon radiography system by Geant4 code
Imaging and identifying materials with high atomic numbers and densities, especially radioactive materials, is one of the issues that have been especially considered in recent years. Due to some limitations in conventional and old imaging techniques, finding an alternative method is very important. The cosmic muons with an infinite source are one of the sources that have been recently studied f...
متن کاملCan One Extract the Neutrino Oscillation Signature from the SuperKamiokande Experiment ? An Analysis of Neutrino Events Occurring outside the Detector
The SuperKamiokande group assert that they have found an oscillatory signature in atmospheric neutrinos through the analysis of Fully Contained Events and Partially Contained Events. We have performed an L/E (length/energy) analysis of Upward Through-Going Muon Events and Stopping Muon Events in a numerical computer simulations both with and without neutrino oscillations but were unable to find...
متن کاملThe Electron / Muon Ratio in Eas at Andabove the " Knee
New data on the electron/muon ratio measured by the KASCADE extensive air shower experiment are presented. This ratio has been proven to be an important parameter for the determination of the mass of the primary particle. The electron and muon detector responses and reconstruction accuracies of the shower parameters have been studied in detailed simulations. Due to the extended lateral distribu...
متن کاملضریب گشتاور مغناطیسی لپتون باردار در فضا- زمان ناجابهجایی
The g-factor of the charged leptons has always been considered by many physicists, both experimentaly as well as theoretically. In fact the electron and muon g-factor play the main role in testing the QED as well as the standard model. Meanwhile, there is a discrepancy between the standard model prediction of the muon anomalies magnetic moment and its experimental determination as large as (25...
متن کاملسطح مقطع طولی در بهمنهای گسترده هوایی؛ نتایج ضمنی برای مطالعه ترکیب جرمی پرتوهای کیهانی
Nµ/Ne, muon to electron population ratio in extensive air showers at high altitudes has been shown to be a suitable estimator of primary cosmic rays mass composition. This study is based on simulated extensive air showers. The Nµ/Ne ratio has been obtained in 100 depths from the top of the atmosphere to the sea level for different primary particle masses and energies. An empirical relation bet...
متن کامل