Neutron Ray-Tracing Simulations of a New Supermirror Guide for the Osiris Spectrometer

被引:2
|
作者
Perrichon, A. [1 ,2 ]
Fernandez-Alonso, F. [2 ,3 ]
Wolff, M. [1 ]
Karlsson, M. [4 ]
Demmel, F. [2 ]
机构
[1] Uppsala Univ, Dept Phys & Astron, S-75237 Uppsala, Sweden
[2] Rutherford Appleton Lab, ISIS Facil, Didcot OX11 0QX, Oxon, England
[3] UCL, Dept Phys & Astron, London WC1E 6BT, England
[4] Chalmers Univ Technol, Dept Chem & Chem Engn, S-41296 Gothenburg, Sweden
来源
JOURNAL OF SURFACE INVESTIGATION | 2020年 / 14卷 / SUPPL 1期
基金
英国科学技术设施理事会; 瑞典研究理事会;
关键词
neutron spectrometer; Monte Carlo simulations; OSIRIS; quasielastic neutron scattering; PERFORMANCE;
D O I
10.1134/S1027451020070381
中图分类号
O469 [凝聚态物理学];
学科分类号
070205 ;
摘要
A new supermirror guide has been proposed to replace the current neutron guide of the indirect time-of-flight near-backscattering spectrometer OSIRIS at the ISIS facility. Here we present an extensive Monte Carlo simulation study for the design and optimisation of a new guide system. Among the several guide geometry assessed, a curved guide with elliptical defocusing and focusing sections is shown to perform best. The estimated gain in intensity is a factor of 5-6 at the sample position with a homogeneous distribution of the divergence. The elliptic geometry results in a smaller beam spot and smaller samples will particularly benefit from this upgrade. The proposed guide replacement will ensure that the OSIRIS spectrometer will remain competitive in the years to come.
引用
收藏
页码:S169 / S174
页数:6
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