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dc.contributor.authorLauter, Valeria
dc.contributor.authorWang, Kang
dc.contributor.authorMewes, Tim
dc.contributor.authorGlavic, Artur
dc.contributor.authorToperverg, Boris
dc.contributor.authorAhmadi, Mahshid
dc.contributor.authorAssaf, Badih
dc.contributor.authorHu, Bin
dc.contributor.authorLi, Mingda
dc.contributor.authorLiu, Xinyu
dc.contributor.authorLiu, Yaohua
dc.contributor.authorMoodera, Jagadeesh
dc.contributor.authorRokhinson, Leonid
dc.contributor.authorSingh, Deepak
dc.contributor.authorSun, Nian
dc.date.accessioned2023-01-20T18:13:24Z
dc.date.available2023-01-20T18:13:24Z
dc.date.issued2022
dc.identifier.urihttps://hdl.handle.net/1721.1/147615
dc.description.abstract<jats:p> M-STAR is a next generation polarized neutron reflectometer with advanced capabilities. A new focusing guide concept is optimized for samples with dimensions down to a millimeter range. A proposed hybrid pulse-skipping chopper will enable experiments at constant geometry at one incident angle in a broad range of wavevector transfer Q up to 0.3 A<jats:sup>−1</jats:sup> for specular, off-specular, and GISANS measurements. M-STAR will empower nanoscience and spintronics studies routinely on small samples (∼2 × 2 mm<jats:sup>2</jats:sup>) and of atomic-scale thickness using versatile experimental conditions of magnetic and/or electric fields, light, and temperature applied in situ to novel complex device-like nanosystems with multiple buried interfaces. M-STAR will enable improved grazing incidence diffraction measurements, as a surface-sensitive depth-resolved probe of, e.g., the out-of-plane component of atomic magnetic moments in ferromagnetic, antiferromagnetic, and more complex structures as well as in-plane atomic-scale structures inaccessible with contemporary diffractometry and reflectometry. New horizons will be opened by the development of an option to probe near-surface dynamics with inelastic grazing incidence scattering in the time-of-flight mode. These novel options in combination with ideally matched parameters of the second target station will place M-STAR in the world’s leading position for high resolution polarized reflectometry. </jats:p>en_US
dc.language.isoen
dc.publisherAIP Publishingen_US
dc.relation.isversionof10.1063/5.0093622en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceAmerican Institute of Physics (AIP)en_US
dc.titleM-STAR: Magnetism second target advanced reflectometer at the Spallation Neutron Sourceen_US
dc.typeArticleen_US
dc.identifier.citationLauter, Valeria, Wang, Kang, Mewes, Tim, Glavic, Artur, Toperverg, Boris et al. 2022. "M-STAR: Magnetism second target advanced reflectometer at the Spallation Neutron Source." Review of Scientific Instruments, 93 (10).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_US
dc.relation.journalReview of Scientific Instrumentsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2023-01-20T18:08:35Z
dspace.orderedauthorsLauter, V; Wang, K; Mewes, T; Glavic, A; Toperverg, B; Ahmadi, M; Assaf, B; Hu, B; Li, M; Liu, X; Liu, Y; Moodera, J; Rokhinson, L; Singh, D; Sun, Nen_US
dspace.date.submission2023-01-20T18:08:42Z
mit.journal.volume93en_US
mit.journal.issue10en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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