Florian Simperl | Searcharxiv

arXiv2025

Identifying Electronic Doorway States in the Secondary Electron Emission from Layered Materials

We investigate the secondary low-energy electron emission induced by inelastic electron scattering from graphene and layered materials thereof. By applying a coincidence detection of the primary scattered and the emitted secondary electron we unravel pronounced resonance features otherwise overshadowed by the largely structureless secondary electron energy distribution. Supported by density functional theory calculations we show that these structures are the signature of prominent Feshbach resonances above the vacuum threshold which originate from interlayer states acting as a doorway state for electron emission. Remarkably, some of these doorway states open up only for samples with more than five layers.

cond-mat.mes-hall↗

arXiv2023

Energy Dissipation of Fast Electrons in Polymethylmetacrylate (PMMA): Towards a Universal Curve for Electron Beam Attenuation in Solids for Energies between ~0 eV and 100 keV

Wolfgang S.M. Werner, Florian Simperl, Felix Bloedorn, Julian Brunner, Johannes Kero, Alessandra Bellissimo and Olga Ridzel Spectroscopy of correlated electron pairs was employed to investigate the energy dissipation process as well as the transport and the emission of low energy electrons on a polymethylmetracylate (PMMA) surface, providing secondary electron (SE) spectra causally related to the energy loss of the primary electron. Two groups of electrons are identified in the cascade of slow electrons, corresponding to different stages in the energy dissipation process. For both groups, the characteristic lengths for attenuation due to collective excitations and momentum relaxation are quantified and are found to be distinctly different: l1=(12.0+/-2) Angstroem and l2=(61.5+/-11) Angstroem. The results strongly contradict the commonly employed model of exponential attenuation with the electron inelastic mean free path (IMFP) as characteristic length, but essentially agree with a theory used for decades in astrophysics and neutron transport, albeit with characteristic lengths expressed in units of Angstroems rather than lightyears.

cond-mat.mtrl-sci↗