April 22 - 26, 2024
Seattle, Washington
May 7 - 9, 2024 (Virtual)

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2024 MRS Spring Meeting
QT01.11.02

Terahertz Emission Spectroscopy to Probe Ultrafast Spin to Charge Conversion at Perovskite/Ferromagnet Interfaces

When and Where

Apr 26, 2024
3:00pm - 3:15pm
Room 420, Level 4, Summit

Presenter(s)

Co-Author(s)

Yifan Dong1,Matthew Hautzinger1,Andrew Comstock2,Aeron McConnell2,Dali Sun2,Matthew Beard1

National Renewable Energy Laboratory1,North Carolina State University2

Abstract

Yifan Dong1,Matthew Hautzinger1,Andrew Comstock2,Aeron McConnell2,Dali Sun2,Matthew Beard1

National Renewable Energy Laboratory1,North Carolina State University2
Understanding spin-to-charge conversion (SCC) allows efficient control and manipulation of the spin degree of freedom, which can pave the way for next generation spintronic devices. Unlike conventional transport-based measurements, terahertz (THz) emission spectroscopy offers great advantages including the capability of measuring transient charge currents with sub-picosecond time resolution. Using THz emission spectroscopy, we observed the ultrafast spin current injection at the interface between a ferromagnetic (FM) material and a chiral two-dimensional (2D) perovskite via inverse Rashba-Edelstein effect. In summary, we observed strong magnetic field- and polarization-dependence in both phase and intensity of the emitted THz signal, implying the great tunability in these chiral 2D perovskites for spintronic application. These results present a promising way to control charge and spin interconversion at perovskite/ferromagnetic interfaces and future spintronics devices. The unique asymmetry in THz emission due to SCC at chiral 2D perovskite/FM (i.e. (R-MBA)<sub>2</sub>PbI<sub>4</sub>/NiFe and (S-MBA)<sub>2</sub>PbI<sub>4</sub>) interface distinguishes them from three-dimensional perovskite materials which only exhibiit symmetric THz emission. In this talk, I will discuss the measured THz emission signals including both the forward and backward THz emission (reflected at the air/substrate interface). The forward emission signal exhibits a π-phase shift when the in-plane magnetic field flips its sign, whereas the backward signal exhibits no phase shift at all. In addition, I will also discuss the asymmetry in THz emission intensity. Specifically, the THz emission intensity of the forward emission signal decreases by almost two-fold when the in-plane magnetic field reverses, while the backward emission signal increases by two-fold when the field direction reverses. Such asymmetry in THz emission can be explained with an in-plane momentum shift of the Rashba bands induced by the ultrafast laser pump.

Keywords

magnetoresistance (transport) | spectroscopy

Symposium Organizers

Ajay Ram Srimath Kandada, Wake Forest University
Nicolò Maccaferri, Umeå University
Chiara Trovatello, Columbia University
Ursula Wurstbauer, Technical University of Munich

Symposium Support

Bronze
LIGHT CONVERSION

Session Chairs

Veronica Policht
Chiara Trovatello

In this Session