X-Ray Magnetic Circular Dichroism in Altermagnetic α-MnTe.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
26 Apr 2024
Historique:
received: 08 05 2023
revised: 01 02 2024
accepted: 20 03 2024
medline: 10 5 2024
pubmed: 10 5 2024
entrez: 10 5 2024
Statut: ppublish

Résumé

Altermagnetism is a recently identified magnetic symmetry class combining characteristics of conventional collinear ferromagnets and antiferromagnets, that were regarded as mutually exclusive, and enabling phenomena and functionalities unparalleled in either of the two traditional elementary magnetic classes. In this work we use symmetry, ab initio theory, and experiments to explore x-ray magnetic circular dichroism (XMCD) in the altermagnetic class. As a representative material for our XMCD study we choose α-MnTe with compensated antiparallel magnetic order in which an anomalous Hall effect has been already demonstrated. We predict and experimentally confirm a characteristic XMCD line shape for compensated moments lying in a plane perpendicular to the light propagation vector. Our results highlight the distinct phenomenology in altermagnets of this time-reversal symmetry breaking response, and its potential utility for element-specific spectroscopy and microscopy.

Identifiants

pubmed: 38728732
doi: 10.1103/PhysRevLett.132.176701
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

176701

Auteurs

A Hariki (A)

Department of Physics and Electronics, Graduate School of Engineering, Osaka Metropolitan University, 1-1 Gakuen-cho, Nakaku, Sakai, Osaka 599-8531, Japan.

A Dal Din (A)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.

O J Amin (OJ)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.

T Yamaguchi (T)

Department of Physics and Electronics, Graduate School of Engineering, Osaka Metropolitan University, 1-1 Gakuen-cho, Nakaku, Sakai, Osaka 599-8531, Japan.

A Badura (A)

Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6 Czech Republic.

D Kriegner (D)

Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6 Czech Republic.

K W Edmonds (KW)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.

R P Campion (RP)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.

P Wadley (P)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.

D Backes (D)

Diamond Light Source, Chilton OX11 0DE, United Kingdom.

L S I Veiga (LSI)

Diamond Light Source, Chilton OX11 0DE, United Kingdom.

S S Dhesi (SS)

Diamond Light Source, Chilton OX11 0DE, United Kingdom.

G Springholz (G)

Institute of Semiconductor and Solid State Physics, Johannes Kepler University Linz, Altenbergerstraße 69, 4040 Linz, Austria.

L Šmejkal (L)

Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6 Czech Republic.
Institut für Physik, Johannes Gutenberg Universität Mainz, D-55099 Mainz, Germany.

K Výborný (K)

Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6 Czech Republic.

T Jungwirth (T)

School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom.
Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6 Czech Republic.

J Kuneš (J)

Institute for Solid State Physics, TU Wien, 1040 Vienna, Austria.
Department of Condensed Matter Physics, Faculty of Science, Masaryk University, Kotlářská 2, 611 37 Brno, Czechia.

Classifications MeSH