Faster chiral versus collinear magnetic order recovery after optical excitation revealed by femtosecond XUV scattering

dc.contributor.authorKerber, Nico
dc.contributor.authorKsenzov, Dmitriy
dc.contributor.authorFreimuth, Frank
dc.contributor.authorCapotondi, Flavio
dc.contributor.authorPedersoli, Emanuele
dc.contributor.authorLopez-Quintas, Ignacio
dc.contributor.authorSeng, Boris
dc.contributor.authorCramer, Joel
dc.contributor.authorLitzius, Kai
dc.contributor.authorLacour, Daniel
dc.contributor.authorZabel, Hartmut
dc.contributor.authorMokrousov, Yuriy
dc.contributor.authorKläui, Mathias
dc.contributor.authorGutt, Christian
dc.date.accessioned2021-01-15T11:14:26Z
dc.date.available2021-01-15T11:14:26Z
dc.date.issued2020
dc.description.abstractWhile chiral spin structures stabilized by Dzyaloshinskii-Moriya interaction (DMI) are candidates as novel information carriers, their dynamics on the fs-ps timescale is little known. Since with the bulk Heisenberg exchange and the interfacial DMI two distinct exchange mechanisms are at play, the ultrafast dynamics of the chiral order needs to be ascertained and compared to the dynamics of the conventional collinear order. Using an XUV free-electron laser we determine the fs-ps temporal evolution of the chiral order in domain walls in a magnetic thin film sample by an IR pump - X-ray magnetic scattering probe experiment. Upon demagnetization we observe that the dichroic (CL-CR) signal connected with the chiral order correlator m(z)m(x) in the domain walls recovers significantly faster than the (CL+CR) sum signal representing the average collinear domain magnetization m(z)(2)+m(x)(2). We explore possible explanations based on spin structure dynamics and reduced transversal magnetization fluctuations inside the domain walls and find that the latter can explain the experimental data leading to different dynamics for collinear magnetic order and chiral magnetic order. Chiral spin structures have great promise for future information processing applications, however little is known about their ultrafast dynamics. In this experimental study, the authors use femtosecond temporal evolution to observe the fast recovery of chiral magnetic order.en_GB
dc.identifier.doihttp://doi.org/10.25358/openscience-5559
dc.identifier.urihttps://openscience.ub.uni-mainz.de/handle/20.500.12030/5563
dc.language.isoeng
dc.rightsCC-BY-4.0
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject.ddc530 Physikde_DE
dc.subject.ddc530 Physicsen_GB
dc.titleFaster chiral versus collinear magnetic order recovery after optical excitation revealed by femtosecond XUV scatteringen_GB
dc.typeZeitschriftenaufsatzde_DE
jgu.journal.titleNature communications
jgu.journal.volume11
jgu.organisation.departmentFB 08 Physik, Mathematik u. Informatikde_DE
jgu.organisation.nameJohannes Gutenberg-Universität Mainzde_DE
jgu.organisation.number7940
jgu.organisation.placeMainz
jgu.organisation.rorhttps://ror.org/023b0x485
jgu.pages.alternative6304
jgu.publisher.doi10.1038/s41467-020-19613-z
jgu.publisher.issn2041-1723
jgu.publisher.nameNature Publishing Group UK
jgu.publisher.placeLondon
jgu.publisher.urihttps://doi.org/10.1038/s41467-020-19613-z
jgu.publisher.year2020
jgu.rights.accessrightsopenAccessen_GB
jgu.subject.ddccode530
jgu.type.contenttypeScientific articleen_GB
jgu.type.dinitypeArticleen_GB
jgu.type.resourceTexten_GB
jgu.type.versionPublished versionen_GB

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
kerber_nico-faster_chiral_-20210115100755843.pdf
Size:
1.79 MB
Format:
Adobe Portable Document Format
Description:

License bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
license.txt
Size:
3.57 KB
Format:
Item-specific license agreed upon to submission
Description: