%0 Journal Article %1 PhysRevB.103.224429 %A Ortiz Hernändez, N. %A Salman, Z. %A Prokscha, T. %A Suter, A. %A Mardegan, J. R. L. %A Moser, S. %A Zakharova, A. %A Piamonteze, C. %A Staub, U. %D 2021 %I American Physical Society %J Phys. Rev. B %K a %N 22 %P 224429 %R 10.1103/PhysRevB.103.224429 %T Magnetic order of tetragonal CuO ultrathin films %U https://link.aps.org/doi/10.1103/PhysRevB.103.224429 %V 103 %X We present a detailed low-energy muon spin rotation and x-ray magnetic circular dichroism (XMCD) investigation of the magnetic structure in ultrathin tetragonal (T)-CuO films. The measured muon-spin polarization decay indicates an antiferromagnetic (AFM) order with a transition temperature higher than 200 K. The XMCD signal obtained around the CuL2,3 edges indicates the presence of pinned Cu2+ moments that are parallel to the sample surface, and additionally, isotropic paramagnetic moments. The pinning of some of the Cu moments is caused by an AFM ordering consisting of moments that lie most likely in plane of the film. Moreover, pinned moments show a larger orbital magnetic moment contribution with an approximate ratio of morb/mspin=1.5, indicating that these spins are located at sites with reduced symmetry. Some fractions of the pinned moments remain pinned from an AFM background even at 360 K, indicating that TN>360K. We propose a simple model that explains these experimental findings, showing that the magnetic order of the T-CuO ultrathin films differs from the theoretical predictions.

@article{PhysRevB.103.224429, abstract = {We present a detailed low-energy muon spin rotation and x-ray magnetic circular dichroism (XMCD) investigation of the magnetic structure in ultrathin tetragonal (T)-CuO films. The measured muon-spin polarization decay indicates an antiferromagnetic (AFM) order with a transition temperature higher than 200 K. The XMCD signal obtained around the CuL2,3 edges indicates the presence of pinned Cu2+ moments that are parallel to the sample surface, and additionally, isotropic paramagnetic moments. The pinning of some of the Cu moments is caused by an AFM ordering consisting of moments that lie most likely in plane of the film. Moreover, pinned moments show a larger orbital magnetic moment contribution with an approximate ratio of morb/mspin=1.5, indicating that these spins are located at sites with reduced symmetry. Some fractions of the pinned moments remain pinned from an AFM background even at 360 K, indicating that TN>360K. We propose a simple model that explains these experimental findings, showing that the magnetic order of the T-CuO ultrathin films differs from the theoretical predictions.}, added-at = {2023-04-06T15:31:37.000+0200}, author = {Ortiz Hernändez, N. and Salman, Z. and Prokscha, T. and Suter, A. and Mardegan, J. R. L. and Moser, S. and Zakharova, A. and Piamonteze, C. and Staub, U.}, biburl = {https://www.bibsonomy.org/bibtex/2c49c943ec1aefef7e95ea5a6385ebc68/ctqmat}, day = 22, description = {Magnetic order of tetragonal CuO ultrathin films}, doi = {10.1103/PhysRevB.103.224429}, interhash = {c9d740c0c2f51ce50e91ed6147ca16c6}, intrahash = {c49c943ec1aefef7e95ea5a6385ebc68}, journal = {Phys. Rev. B}, keywords = {a}, month = {06}, number = 22, numpages = {11}, pages = 224429, publisher = {American Physical Society}, timestamp = {2023-04-06T15:31:37.000+0200}, title = {Magnetic order of tetragonal CuO ultrathin films}, url = {https://link.aps.org/doi/10.1103/PhysRevB.103.224429}, volume = 103, year = 2021 }