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dc.creatorJovanović, Vladimir P.
dc.creatorRaffy, H.
dc.creatorLi, Z. Z.
dc.creatorRemenyi, G.
dc.creatorMonceau, P.
dc.date.accessioned2022-04-05T15:34:39Z
dc.date.available2022-04-05T15:34:39Z
dc.date.issued2021
dc.identifier.issn2469-9950
dc.identifier.urihttp://rimsi.imsi.bg.ac.rs/handle/123456789/1442
dc.description.abstractWe studied the in-plane angular magnetoresistance (AMR), in the normal state, of underdoped superconducting Sr1-xLaxCuO2, which has the simplest crystal structure among cuprates. The measurements of two underdoped thin films with different dopings were performed in intense magnetic field H (up to 22 T). The longitudinal magnetoresistance at temperature T is negative and scales with HIT. For both samples, the AMR is anisotropic and shows an unexpected dependence on H intensity. While at the low magnetic field, one observes essentially twofold AMR oscillations for the more doped sample, fourfold ones start to grow under the high magnetic field, resulting in the coexistence of the two. For the less doped film at the low magnetic field, both twofold and fourfold AMR components exist. With the increase of the magnetic field, the fourfold component survives a pi/4 phase shift, during which its amplitude vanishes, at a magnetic field such as 16 T lt H-c lt 17 T. As a result, at the high magnetic field above H-c, the angular dependence of the in-plane magnetoresistance turns out to be the same for both samples. We tentatively ascribe the above features to the presence of antiferromagnetism in the CuO2 planes of underdoped Sr1-xLaxCuO2.en
dc.publisherAmer Physical Soc, College Pk
dc.relationinfo:eu-repo/grantAgreement/MESTD/inst-2020/200053/RS//
dc.rightsrestrictedAccess
dc.sourcePhysical Review B
dc.subjectsuperconductors
dc.subjectelectron-doped cuprate
dc.subjectepitaxial thin films
dc.subjectmagnetotransport
dc.subjecthigh magnetic fields
dc.titleHigh magnetic-field evolution of the in-plane angular magnetoresistance of electron-doped Sr1-xLaxCuO2 in the normal stateen
dc.typearticle
dc.rights.licenseARR
dc.citation.issue1
dc.citation.other103(1): -
dc.citation.rankM21~
dc.citation.volume103
dc.identifier.doi10.1103/PhysRevB.103.014520
dc.identifier.scopus2-s2.0-85100140623
dc.identifier.wos000612136200005
dc.type.versionpublishedVersion


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