PIONEER, a high-resolution single-crystal polarized neutron diffractometer

Yaohua Liu, Huibo Cao, Stephan Rosenkranz, Matthew Frost, Thomas Huegle, Jiao Y.Y. Lin, Peter Torres, Alexandru Stoica, Bryan C. Chakoumakos

Research output: Contribution to journalArticlepeer-review

12 Scopus citations

Abstract

PIONEER is a high Q-resolution, single-crystal, polarized neutron diffractometer at the Second Target Station (STS), Oak Ridge National Laboratory. It will provide the unprecedented capability of measuring tiny crystals (0.001 mm3, i.e., x-ray diffraction size), ultra-thin films (10 nm thickness), and weak structural and magnetic transitions. PIONEER benefits from the increased peak brightness of STS cold-neutron sources and uses advanced Montel mirrors that are able to deliver a focused beam with a high brilliance transfer, a homogeneous profile, and a low background. Monte Carlo simulations suggest that the optimized instrument has a high theoretical peak brilliance of 2.9 × 1012 n cm-2 sr-1 Å-1 s-1 at 2.5 Å at the sample position, within a 5 × 5 mm2 region and a ±0.3° divergence range. The moderator-to-sample distance is 60 m, providing a nominal wavelength band of 4.3 Å with a wavelength resolution better than 0.2% in the wavelength range of 1.0-6.0 Å. PIONEER is capable of characterizing large-scale periodic structures up to 200 Å. With a sample-to-detector distance of 0.8 m, PIONEER accommodates various sample environments, including low/high temperature, high pressure, and high magnetic/electric field. A large cylindrical detector array (4.0 sr) with a radial collimator is planned to suppress the background scattering from sample environments. Bottom detector banks provide an additional 0.4 sr coverage or can be removed if needed to accommodate special sample environments. We present virtual experimental results to demonstrate the scientific performance of PIONEER in measuring tiny samples.

Original languageEnglish
Article number073901
JournalReview of Scientific Instruments
Volume93
Issue number7
DOIs
StatePublished - Jul 1 2022

Funding

We sincerely thank the external science advisory board, Robert Birgeneau, Robert Cava, Martin Greven, Bo Iversen, Steven May, Ni Ni, Patrick Woodward, Stephen Wilson, Shan Wu, and Joe Zhou for identifying the scientific cases and defining the scientific requirements for PIONEER. We thank Koji Kaneko, Takashi Ohhara, and Ryoji Kiyanagi for discussion on SENJU at J-PARC; Werner Schweika and Fabrèges Xavier for discussion on MAGiC at ESS; Artur Glavic for discussion on ESTIA at ESS; Christina Hoffmann, Xiaoping Wang, and Feng Ye for discussion on TOPAZ and CORELLI at the SNS; and Bianca Haberl for discussion on DACs. This research used the resources of the Spallation Neutron Source Second Target Station Project at Oak Ridge National Laboratory (ORNL). ORNL is managed by UT-Battelle LLC for DOE’s Office of Science, the single largest supporter of basic research in the physical sciences in the United States. The work at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division.

FundersFunder number
U.S. Department of Energy
Office of Science
Basic Energy Sciences
Argonne National Laboratory
Division of Materials Sciences and Engineering

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