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Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text]
The magnetic phase diagram of Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] as a function of hydrostatic pressure and temperature is investigated by means of high pressure muon spin rotation, relaxation and resonance ([Formula: see text] SR). The weak pressur...
Autores principales: | , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2022
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9585139/ https://www.ncbi.nlm.nih.gov/pubmed/36266305 http://dx.doi.org/10.1038/s41598-022-21699-y |
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author | Forslund, Ola Kenji Andreica, Daniel Sassa, Yasmine Imai, Masaki Michioka, Chishiro Yoshimura, Kazuyoshi Guguchia, Zurab Shermadini, Zurab Khasanov, Rustem Sugiyama, Jun Månsson, Martin |
author_facet | Forslund, Ola Kenji Andreica, Daniel Sassa, Yasmine Imai, Masaki Michioka, Chishiro Yoshimura, Kazuyoshi Guguchia, Zurab Shermadini, Zurab Khasanov, Rustem Sugiyama, Jun Månsson, Martin |
author_sort | Forslund, Ola Kenji |
collection | PubMed |
description | The magnetic phase diagram of Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] as a function of hydrostatic pressure and temperature is investigated by means of high pressure muon spin rotation, relaxation and resonance ([Formula: see text] SR). The weak pressure dependence for the [Formula: see text] compounds suggests that the rich phase diagram of Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] as a function of x at ambient pressure may not solely be attributed to chemical pressure effects. The [Formula: see text] compound on the other hand reveals a high pressure dependence, where the long range magnetic order is fully suppressed at [Formula: see text] kbar, which seem to be a first order transition. In addition, an intermediate phase consisting of magnetic domains is formed above [Formula: see text] kbar where they co-exist with a magnetically disordered state. These domains are likely to be ferromagnetic islands (FMI) and consist of an high- (FMI-[Formula: see text] ) and low-temperature (FMI-[Formula: see text] ) region, respectively, separated by a phase boundary at [Formula: see text] K. This kind of co-existence is unusual and is originating from a coupling between lattice and magnetic degrees of freedoms. |
format | Online Article Text |
id | pubmed-9585139 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-95851392022-10-22 Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] Forslund, Ola Kenji Andreica, Daniel Sassa, Yasmine Imai, Masaki Michioka, Chishiro Yoshimura, Kazuyoshi Guguchia, Zurab Shermadini, Zurab Khasanov, Rustem Sugiyama, Jun Månsson, Martin Sci Rep Article The magnetic phase diagram of Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] as a function of hydrostatic pressure and temperature is investigated by means of high pressure muon spin rotation, relaxation and resonance ([Formula: see text] SR). The weak pressure dependence for the [Formula: see text] compounds suggests that the rich phase diagram of Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] as a function of x at ambient pressure may not solely be attributed to chemical pressure effects. The [Formula: see text] compound on the other hand reveals a high pressure dependence, where the long range magnetic order is fully suppressed at [Formula: see text] kbar, which seem to be a first order transition. In addition, an intermediate phase consisting of magnetic domains is formed above [Formula: see text] kbar where they co-exist with a magnetically disordered state. These domains are likely to be ferromagnetic islands (FMI) and consist of an high- (FMI-[Formula: see text] ) and low-temperature (FMI-[Formula: see text] ) region, respectively, separated by a phase boundary at [Formula: see text] K. This kind of co-existence is unusual and is originating from a coupling between lattice and magnetic degrees of freedoms. Nature Publishing Group UK 2022-10-20 /pmc/articles/PMC9585139/ /pubmed/36266305 http://dx.doi.org/10.1038/s41598-022-21699-y Text en © The Author(s) 2022 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Forslund, Ola Kenji Andreica, Daniel Sassa, Yasmine Imai, Masaki Michioka, Chishiro Yoshimura, Kazuyoshi Guguchia, Zurab Shermadini, Zurab Khasanov, Rustem Sugiyama, Jun Månsson, Martin Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title | Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title_full | Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title_fullStr | Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title_full_unstemmed | Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title_short | Pressure driven magnetic order in Sr[Formula: see text] Ca[Formula: see text] Co[Formula: see text] P[Formula: see text] |
title_sort | pressure driven magnetic order in sr[formula: see text] ca[formula: see text] co[formula: see text] p[formula: see text] |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9585139/ https://www.ncbi.nlm.nih.gov/pubmed/36266305 http://dx.doi.org/10.1038/s41598-022-21699-y |
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