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Anomalous Hall Effect due to Magnetic Fluctuations in a Ferromagnetic Weyl Semimetal
Physik-Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland, Winterthurerstrasse 190; Department of Physics and Astronomy, Uppsala University, Box 516, SE-75120 Uppsala, Sweden, Box 516.
Department of Physics, Southern University of Science and Technology (SUSTech), Shenzhen 518055, China.
Laboratory for Multiscale Materials Experiments, PSI Center for Neutron and Muon Sciences, Forschungsstrasse 111, 5232 Villigen PSI, Switzerland, Forschungsstrasse 111.
Physik-Institut, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland, Winterthurerstrasse 190.
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2025 (Engelska)Ingår i: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 134, nr 12, artikel-id 126602Artikel i tidskrift (Refereegranskat) Published
Abstract [en]

The anomalous Hall effect (AHE) has emerged as a key indicator of time-reversal symmetry breaking (TRSB) and topological features in electronic band structures. Absent of a magnetic field, the AHE requires spontaneous TRSB but has proven hard to probe due to averaging over domains. The anomalous component of the Hall effect is thus frequently derived from extrapolating the magnetic field dependence of the Hall response. We show that discerning whether the AHE is an intrinsic property of the field-free system becomes intricate in the presence of strong magnetic fluctuations. As a study case, we use the Weyl semimetal PrAlGe, where TRSB can be toggled via a ferromagnetic transition, providing a transparent view of the AHE's topological origin. Through a combination of thermodynamic, transport, and muon spin relaxation measurements, we contrast the behavior below the ferromagnetic transition temperature to that of strong magnetic fluctuations above. Our results on PrAlGe provide general insights into the interpretation of anomalous Hall signals in systems where TRSB is debated, such as families of kagome metals or certain transition metal dichalcogenides.

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American Physical Society (APS) , 2025. Vol. 134, nr 12, artikel-id 126602
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URN: urn:nbn:se:kth:diva-362258DOI: 10.1103/PhysRevLett.134.126602ISI: 001458956800001PubMedID: 40215520Scopus ID: 2-s2.0-105001293334OAI: oai:DiVA.org:kth-362258DiVA, id: diva2:1951052
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QC 20250415

Tillgänglig från: 2025-04-09 Skapad: 2025-04-09 Senast uppdaterad: 2025-04-15Bibliografiskt granskad

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Sassa, Yasmine

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