Journal article Evaluation of Ho 100 x y Er x Ce y magnetic refrigerants using advanced multisample neutron transmission spectroscopy
ORCID SAMURAI ; ORCID SAMURAI ;
Simon Rosenqvist Larsen (author) (Search by this author)
; ORCID SAMURAI ;
Kosuke Hiroi (author) (Search by this author)
;
Takenao Shinohara (author) (Search by this author)
; ORCID SAMURAI
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Citation
Hiroaki Mamiya, Noriki Terada, Simon Rosenqvist Larsen, Naohito Tsujii, Kosuke Hiroi, Takenao Shinohara, Hossein Sepehri-Amin. Evaluation of Ho 100 x y Er x Ce y magnetic refrigerants using advanced multisample neutron transmission spectroscopy. Physical Review Research. 2025, 7 (1), 013233. https://doi.org/10.1103/physrevresearch.7.013233

Description:

(abstract)

This article presents a novel multisample neutron transmission spectroscopy method, specifically developed to analyze the spin configurations of Ho100-x-yErxCey across 25 different compositions. Conventional neutron diffractometry is precise but inefficient for evaluating the extensive range of these alloys required for advanced hydrogen liquefaction technologies, prompting the development of our novel technique. We demonstrate that this new spectroscopic technique is not only crucial for high throughput evaluation of the magnetic refrigerants but also serves as a valuable tool for big data-driven research into new magnetic materials.

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Keyword: Neutron Bragg edge analysis, Magnetcaloric effect, Heavy rare earth alloys, Simultaneous high throughput measurement

Date published: 2025-03-03

Publisher: American Physical Society (APS)

Journal:

  • Physical Review Research (ISSN: 26431564) vol. 7 issue. 1 013233

Funding:

  • Ministry of Education, Culture, Sports, Science and Technology 24NM5119
  • Japan Society for the Promotion of Science 19H04400
  • Japan Science and Technology Corporation JPMJMI18A3

Manuscript type: Publisher's version (Version of record)

MDR DOI:

First published URL: https://doi.org/10.1103/physrevresearch.7.013233

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Updated at: 2025-05-09 16:30:35 +0900

Published on MDR: 2025-05-09 16:21:37 +0900

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