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Title: Target and orbit feedback simulations of a muSR beam line at BNL

Abstract

Well-polarized positive surface muons are a tool to measure the magnetic properties of materials since the precession rate of the spin can be determined from the observation of the positron directions when the muons decay. For a dc beam an ideal µSR flux for surface µ+ should be about 40 kHz/mm2. In this report we show how this flux could be achieved in a beam line using the AGS complex at BNL for a source of protons. We also determined that an orbit feedback system with a pair of thin silicon position monitors and kickers would miss the desired flux by at least an order of magnitude, even with perfect time resolution and no multiple scattering.

Authors:
 [1];  [1];  [1];  [1]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States)
Publication Date:
Research Org.:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP)
OSTI Identifier:
1210188
Report Number(s):
BNL-108273-2015-IR
R&D Project: KBCH139; 18031; KB0202011
DOE Contract Number:  
SC00112704
Resource Type:
Technical Report
Country of Publication:
United States
Language:
English
Subject:
43 PARTICLE ACCELERATORS

Citation Formats

MacKay, W., Blaskiewicz, M., Fischer, W., and Pile, P. Target and orbit feedback simulations of a muSR beam line at BNL. United States: N. p., 2015. Web. doi:10.2172/1210188.
MacKay, W., Blaskiewicz, M., Fischer, W., & Pile, P. Target and orbit feedback simulations of a muSR beam line at BNL. United States. https://doi.org/10.2172/1210188
MacKay, W., Blaskiewicz, M., Fischer, W., and Pile, P. 2015. "Target and orbit feedback simulations of a muSR beam line at BNL". United States. https://doi.org/10.2172/1210188. https://www.osti.gov/servlets/purl/1210188.
@article{osti_1210188,
title = {Target and orbit feedback simulations of a muSR beam line at BNL},
author = {MacKay, W. and Blaskiewicz, M. and Fischer, W. and Pile, P.},
abstractNote = {Well-polarized positive surface muons are a tool to measure the magnetic properties of materials since the precession rate of the spin can be determined from the observation of the positron directions when the muons decay. For a dc beam an ideal µSR flux for surface µ+ should be about 40 kHz/mm2. In this report we show how this flux could be achieved in a beam line using the AGS complex at BNL for a source of protons. We also determined that an orbit feedback system with a pair of thin silicon position monitors and kickers would miss the desired flux by at least an order of magnitude, even with perfect time resolution and no multiple scattering.},
doi = {10.2172/1210188},
url = {https://www.osti.gov/biblio/1210188}, journal = {},
number = ,
volume = ,
place = {United States},
year = {Tue Jul 28 00:00:00 EDT 2015},
month = {Tue Jul 28 00:00:00 EDT 2015}
}