Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8165842 | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment | 2018 | 7 Pages |
Abstract
A brilliance measurement was conducted on July 21, 2014 at the ICON beamline at SINQ as a benchmark before any potential changes are made to the liquid deuterium cold neutron source in a future extended shutdown period. The peak brilliance of the deuterium cold source at SINQ has been measured to be 3.3±0.15Ã1011 n cmâ2 sâ1 mAâ1 Ã
â1 steradâ1 at 1.8 Ã
, and the total brilliance (energy-integrated) has been measured to be 9.1±0.77Ã1011 n cmâ2 sâ1 mAâ1 steradâ1 for wavelengths above 0.7 Ã
via a time-of-flight measurement at the ICON beamline. Using a detailed MCNP model, the peak brilliance has been calculated to be 3.1±0.14Ã1011 n cmâ2 sâ1 mAâ1 Ã
â1 steradâ1 at 1.65 Ã
, and the total brilliance (energy-integrated) has been calculated to be 9.2±1.2Ã1011 n cmâ2 sâ1 mAâ1 steradâ1 for wavelengths above 0.7 Ã
. The peak brilliance value and wavelength position disagree only slightly between the measurement and model (7% difference in value, 8% difference in wavelength position), and the total brilliance agrees within the uncertainty bounds. The close agreement validates the models and benchmarks the state of the cold source.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Instrumentation
Authors
Ryan M. Bergmann, Masako Yamada, Uwe Filges, Tibor Reiss, Vadim Talanov, Michael Wohlmuther,