dc.contributor.author |
BHAT, BHAGYASHRI DEVARU |
en_US |
dc.date.accessioned |
2023-08-18T09:43:55Z |
|
dc.date.available |
2023-08-18T09:43:55Z |
|
dc.date.issued |
2023-10 |
en_US |
dc.identifier.citation |
Journal of Physics: Condensed Matter, 35(43). |
en_US |
dc.identifier.issn |
0953-8984 |
en_US |
dc.identifier.issn |
1361-648X |
en_US |
dc.identifier.uri |
https://doi.org/10.1088/1361-648X/ace8e4 |
en_US |
dc.identifier.uri |
http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/8141 |
|
dc.description.abstract |
Janus transition metal dichalcogenide monolayers have shown a lack of mirror symmetry perpendicular to the 2D plane. The breaking of out-of-plane symmetry, along with the spin–orbit coupling, induces Rashba spin-splitting (RSS) in these materials. In this work, RSS in Janus tin dichalcogenide monolayers are studied. In addition, the heterostructures (HSs) of Janus SnXY and WXY (X, Y = S, Se, Te; X ≠ Y) monolayers are discussed. A RSS energy of about 43 meV, more significant than the room temperature energy, is observed in the Janus SnSSe/WSSe HS. The consequences of vertical strain on the semiconducting HS are examined. Compressive vertical strain enhances and tensile strain reduces, the spin-splitting. For the compressive strain of 10.4%, Janus SnSSe/WSSe HS remains semiconductor with only Rashba bands surrounding near the Fermi level. Enhanced Rashba parameter of about 0.96 eV Å and splitting energy of about 72 meV are observed. These findings confirm that Janus SnSSe/WSSe HS is a productive Rashba material for spintronic device applications. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
IOP Publishing |
en_US |
dc.subject |
Rashba effect |
en_US |
dc.subject |
Spin-splitting |
en_US |
dc.subject |
Janus monolayers |
en_US |
dc.subject |
Spintronics |
en_US |
dc.subject |
Vertical strain |
en_US |
dc.subject |
Spin-orbit coupling |
en_US |
dc.subject |
2023-AUG-WEEK1 |
en_US |
dc.subject |
TOC-AUG-2023 |
en_US |
dc.subject |
2023 |
en_US |
dc.title |
Rashba spin-splitting in Janus SnXY/WXY (X, Y = S, Se, Te; X ≠ Y) heterostructures |
en_US |
dc.type |
Article |
en_US |
dc.contributor.department |
Dept. of Physics |
en_US |
dc.identifier.sourcetitle |
Journal of Physics: Condensed Matter |
en_US |
dc.publication.originofpublisher |
Foreign |
en_US |