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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

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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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, br. 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 i Mario Novak. "Nodal-line driven anomalous susceptibility in ZrSiS." Physical Review B: Condensed matter and materials physics 105, br. 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, i sur.. Nodal-line driven anomalous susceptibility in ZrSiS. Physical Review B: Condensed matter and materials physics [Internet]. 06.2022. [pristupljeno 05.11.2024.];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, br. 24, Lipanj 2022. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:530356. [Citirano: 05.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:530356
Podaci o radu
Naslov (engleski)Nodal-line driven anomalous susceptibility in ZrSiS
AutorBruno Gudac
AutorMarkus Kriener
AutorYuriy V. Sharlai
AutorMihovil Bosnar
AutorFilip Orbanić
AutorGrigorii P. Mikitik
AutorAkio Kimura
AutorIvan Kokanović
AutorMario Novak
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Pismo
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysical Review B: Condensed matter and materials physics
Brojčani podacivol. 105, br. 24, L241115
p-ISSN2469-9950
e-ISSN2469-9969
DOIhttps://doi.org/10.1103/PhysRevB.105.L241115
URN:NBNurn:nbn:hr:217:530356
Datum objave publikacije2022-06
URL dokumentahttps://journals.aps.org/prb/abstract/10.1103/PhysRevB.105.L241115
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2022 American Physical Society. Received 21 March 2022. Revised 31 May 2022. Accepted 1 June 2022. Published 29 June 2022.
Datum i vrijeme pohrane2024-08-21 10:20:25