Abstract
Ray-tracing of polarized neutrons faces a challenge when the neutron propagates through an inhomogeneous magnetic field. This affects simulations of novel instruments using encoding of energy or angle into the neutron spin. We here present a new implementation of propagation of polarized neutrons within the McStas simulation package and show that it outperforms the de-facto standard method implemented in the NISP package by Seeger and Daemen. We include simulation of a simplified model of a spin-echo instrument, including a simple virtual experiment.
Originalsprog | Engelsk |
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Tidsskrift | Journal of Neutron Research |
Vol/bind | 17 |
Udgave nummer | 1 |
Sider (fra-til) | 27-34 |
ISSN | 1023-8166 |
DOI | |
Status | Udgivet - 1 jan. 2014 |