Spectroscopic probe of ultrafast magnetization dynamics in the extreme ultraviolet spectral range
Johanna Richter, Somnath Jana, Robert Behrends, Carl S. Davies, Dieter W. Engel, Martin Hennecke, Daniel Schick, Clemens von Korff Schmising, Stefan Eisebitt
TL;DR
This work addresses the need for a simple, intensity-based XUV probe of ultrafast magnetization in systems with out-of-plane anisotropy grown on opaque substrates. It introduces two geometries, L-MOKE and P-MOKE, that leverage Kerr-induced polarization changes together with strong Brewster-angle reflectance anisotropy, allowing analyzer-free measurements with linearly polarized XUV light. Through HHG-based XUV sources, simulations using the udkm1Dsim toolkit, and time-resolved pump-probe experiments on FeNi and Pt/GdCo/Pt structures, the authors map energy- and polarization-dependent magneto-optical signals and demonstrate sizable, linear responses up to about 10% asymmetry. The methods reveal distinct ultrafast demagnetization dynamics, including element-specific delays, and offer a versatile platform for imaging nanoscale magnetic textures on opaque substrates, with broad implications for ultrafast spintronics and magnetic microscopy.
Abstract
The development of spectroscopic techniques in the extreme ultraviolet (XUV) spectral range has significantly advanced the understanding of ultrafast interactions in magnetic systems triggered by optical excitation. In this work, we introduce a previously missing geometry that facilitates the observation of the ultrafast magnetization dynamics of magnetic systems with an out-of-plane magnetization grown on XUV opaque substrates. This approach to probing ultrafast magnetization dynamics combines the magneto-optical Kerr effect with the strong dependence of a sample's reflectance near its Brewster angle. It therefore works with linearly polarized light and does not require any additional polarizing optics. We provide a comprehensive analysis of the technique by presenting both simulations and experimental data as a function of the energy and the polarization of the XUV probe radiation as well as of the delay time after optical excitation.
