Our system is currently under heavy load due to increased usage. We're actively working on upgrades to improve performance. Thank you for your patience.
2016
DOI: 10.1103/physrevb.93.104403
|View full text |Cite
|
Sign up to set email alerts
|

Thickness dependence of exchange coupling in (111)-oriented perovskite oxide superlattices

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

3
20
0

Year Published

2017
2017
2023
2023

Publication Types

Select...
9

Relationship

2
7

Authors

Journals

citations
Cited by 18 publications
(23 citation statements)
references
References 54 publications
(63 reference statements)
3
20
0
Order By: Relevance
“…With the TEY measurements, the Mn-XA/XMCD signal emanates primarily from the portion of the LSMO sublayer in proximity to the top LSMO/LSCO interface, and the signal could not be detected above the noise floor for the m > 12 SLs. For the m ⩽ 12 SLs, the interface-sensitive Mn-XA spectra resembles that of the LSCMO film and differs from LSMO [40][41][42][43][44]. However, as with the Co-XMCD spectra, the spectral shape of the Mn-XMCD curves remains unchanged, indicating that the magnetically active Mn 3+ /Mn 4+ ions remain largely as in the thick LSMO film though they are broken up by a higher concentration of Mn 4+ ions.…”
Section: Maximum Of Dρ(t) Dtmentioning
confidence: 95%
“…With the TEY measurements, the Mn-XA/XMCD signal emanates primarily from the portion of the LSMO sublayer in proximity to the top LSMO/LSCO interface, and the signal could not be detected above the noise floor for the m > 12 SLs. For the m ⩽ 12 SLs, the interface-sensitive Mn-XA spectra resembles that of the LSCMO film and differs from LSMO [40][41][42][43][44]. However, as with the Co-XMCD spectra, the spectral shape of the Mn-XMCD curves remains unchanged, indicating that the magnetically active Mn 3+ /Mn 4+ ions remain largely as in the thick LSMO film though they are broken up by a higher concentration of Mn 4+ ions.…”
Section: Maximum Of Dρ(t) Dtmentioning
confidence: 95%
“…Interfacial and confinement effects in heterostructures grown along the perovskite-(111) orientation are much less studied. 24,29,33,34 Interestingly, in a thin film with a thickness of two monolayers (MLs) of LNO grown along this orientation, the Ni atoms form a buckled honeycomb lattice; such a heterostructure was predicted to host novel topological phases which are yet to be found experimentally. [35][36][37][38] The recent realization of high quality heterostructures that combine LNO with thin insulating ferromagnetic LaMnO 3 (LMO) layers along the (111) direction and exhibit unexpected phenomena is an example of the novel physics found in this type of heterostructures.…”
Section: © 2017 Author(s) All Article Content Except Where Otherwismentioning
confidence: 99%
“…With the TEY measurements, the Mn-XA/XMCD signal emanates primarily from the portion of the LSMO sublayer in proximity to the top LSMO/LSCO interface, and the signal could not be detected above the noise floor for the m > 12 SLs. For the m ⩽ 12 SLs, the interface-sensitive Mn-XA spectra resembles that of the LSCMO film and differs from LSMO [40][41][42][43][44]. However, as with the Co-XMCD spectra, the spectral shape of the Mn-XMCD curves remains unchanged, indicating that the magnetically active Mn 3+ /Mn 4+ ions remain largely as in the thick LSMO film though they are broken up by a higher concentration of Mn 4+ ions.…”
Section: Maximum Of Dρ(t) Dtmentioning
confidence: 89%