prikaz prve stranice dokumenta Nodal-line driven anomalous susceptibility in ZrSiS
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Scientific paper - Letter
Nodal-line driven anomalous susceptibility in ZrSiS
Physical Review B: Condensed matter and materials physics, 105 (2022), 24; L241115. https://doi.org/10.1103/PhysRevB.105.L241115
Gudac, Bruno; Kriener, Markus; Sharlai, Yuriy V.; Bosnar, Mihovil; Orbanić, Filip; Mikitik, Grigorii P.; Kimura, Akio; Kokanović, Ivan; Novak, Mario

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Gudac, B., Kriener, M., Sharlai, Y. V., Bosnar, M., Orbanić, F., Mikitik, G. P. ... Novak, M. (2022). Nodal-line driven anomalous susceptibility in ZrSiS. Physical Review B: Condensed matter and materials physics, 105. (24). doi: 10.1103/PhysRevB.105.L241115

Gudac, Bruno, et al. "Nodal-line driven anomalous susceptibility in ZrSiS." Physical Review B: Condensed matter and materials physics, vol. 105, no. 24, 2022. https://doi.org/10.1103/PhysRevB.105.L241115

Gudac, Bruno, Markus Kriener, Yuriy V. Sharlai, Mihovil Bosnar, Filip Orbanić, Grigorii P. Mikitik, Akio Kimura, Ivan Kokanović and Mario Novak. "Nodal-line driven anomalous susceptibility in ZrSiS." Physical Review B: Condensed matter and materials physics 105, no. 24 (2022). https://doi.org/10.1103/PhysRevB.105.L241115

Gudac, B., et al. (2022) 'Nodal-line driven anomalous susceptibility in ZrSiS', Physical Review B: Condensed matter and materials physics, 105(24). doi: 10.1103/PhysRevB.105.L241115

Gudac B, Kriener M, Sharlai YV, Bosnar M, Orbanić F, Mikitik GP, and sur.. Nodal-line driven anomalous susceptibility in ZrSiS. Physical Review B: Condensed matter and materials physics [Internet]. 2022 June [cited 2024 November 05];105(24). doi: 10.1103/PhysRevB.105.L241115

B. Gudac, et al., "Nodal-line driven anomalous susceptibility in ZrSiS", Physical Review B: Condensed matter and materials physics, vol. 105, no. 24, June 2022. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:530356. [Accessed: 05 November 2024]

Metadata
Title (english)Nodal-line driven anomalous susceptibility in ZrSiS
AuthorBruno Gudac
AuthorMarkus Kriener
AuthorYuriy V. Sharlai
AuthorMihovil Bosnar
AuthorFilip Orbanić
AuthorGrigorii P. Mikitik
AuthorAkio Kimura
AuthorIvan Kokanović
AuthorMario Novak
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
We demonstrate a unique approach to test the signature of the nodal-line physics by thermodynamic methods. By measuring magnetic susceptibility in ZrSiS we found an intriguing temperature-driven crossover from dia- to paramagnetic behavior. We show that the anomalous behavior represents a real thermodynamic signature of the underlying nodal-line physics through the means of chemical pressure (isovalent substitution of Zr for Hf), quantum oscillations, and theoretical modeling. The anomalous part of the susceptibility is orbital by nature, and it arises due to the vicinity of the Fermi level to a degeneracy point created by the crossing of two nodal lines. Furthermore, an unexpected Lifshitz topological transition at the degeneracy point is revealed by tuning the Fermi level. The present findings in ZrSiS give an attractive starting point for various nodal-line physics-related phenomena to be tested by thermodynamic methods in other related materials.
Keywords (english)
Languageenglish
Publication typeScientific paper - Letter
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titlePhysical Review B: Condensed matter and materials physics
Numberingvol. 105, no. 24, L241115
p-ISSN2469-9950
e-ISSN2469-9969
DOIhttps://doi.org/10.1103/PhysRevB.105.L241115
URN:NBNurn:nbn:hr:217:530356
Publication2022-06
Document URLhttps://journals.aps.org/prb/abstract/10.1103/PhysRevB.105.L241115
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2022 American Physical Society. Received 21 March 2022. Revised 31 May 2022. Accepted 1 June 2022. Published 29 June 2022.
Created on2024-08-21 10:20:25