Muon simulations for Super-Kamiokande, KamLAND, and CHOOZ

Alfred Tang, Glenn Horton-Smith, Vitaly A. Kudryavtsev, and Alessandra Tonazzo
Phys. Rev. D 74, 053007 – Published 15 September 2006

Abstract

Muon backgrounds at Super-Kamiokande, KamLAND, and CHOOZ are calculated using MUSIC. A modified version of the Gaisser sea-level muon distribution and a well-tested Monte Carlo integration method are introduced. Average muon energy, flux, and rate are tabulated. Plots of average energy and angular distributions are given. Implications for muon tracker design in future experiments are discussed.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
9 More
  • Received 7 April 2006

DOI:https://doi.org/10.1103/PhysRevD.74.053007

©2006 American Physical Society

Authors & Affiliations

Alfred Tang and Glenn Horton-Smith

  • Physics Department, Kansas State University, Manhattan, Kansas 66506, USA

Vitaly A. Kudryavtsev

  • Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom

Alessandra Tonazzo

  • APC and Université Paris 7, 75005 Paris, France

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 74, Iss. 5 — 1 September 2006

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×