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Simulation of backgrounds in detectors and energy deposition in superconducting magnets at {mu}{sup +}{mu}{sup {minus}} colliders

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.50907· OSTI ID:288260
 [1];  [2]
  1. Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510 (United States)
  2. Institute for High Energy Physics, Protvino, 142284 (Russia)
A calculational approach is described to study beam induced radiation effects in detector and storage ring components at high-energy high-luminosity {mu}{sup +}{mu}{sup {minus}} colliders. The details of the corresponding physics process simulations used in the MARS code are given. Contributions of electromagnetic showers, synchrotron radiation, hadrons and daughter muons to the background rates in a generic detector for a 2{times}2 TeV {mu}{sup +}{mu}{sup {minus}} collider are investigated. Four configurations of the inner triplet and a detector are examined for two sources: muon decays and beam halo interactions in the lattice elements. The beam induced power density in superconducting magnets is calculated and ways to reduce it are proposed. {copyright} {ital 1996 American Institute of Physics.}
Research Organization:
Fermi National Accelerator Laboratory
Sponsoring Organization:
USDOE
DOE Contract Number:
AC02-76CH03000
OSTI ID:
288260
Report Number(s):
CONF-9510295--
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 372; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English