Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published August 7, 2023 | Published
Journal Article Open

Using electron energy-loss spectroscopy to measure nanoscale electronic and vibrational dynamics in a TEM

  • 1. ROR icon California Institute of Technology

Abstract

Electron energy-loss spectroscopy (EELS) can measure similar information to x-ray, UV–Vis, and IR spectroscopies but with atomic resolution and increased scattering cross-sections. Recent advances in electron monochromators have expanded EELS capabilities from chemical identification to the realms of synchrotron-level core-loss measurements and to low-loss, 10–100 meV excitations, such as phonons, excitons, and valence structures. EELS measurements are easily correlated with electron diffraction and atomic-scale real-space imaging in a transmission electron microscope (TEM) to provide detailed local pictures of quasiparticle and bonding states. This perspective provides an overview of existing high-resolution EELS (HR-EELS) capabilities while also motivating the powerful next step in the field—ultrafast EELS in a TEM. Ultrafast EELS aims to combine atomic-level, element-specific, and correlated temporal measurements to better understand spatially specific excited-state phenomena. Ultrafast EELS measurements also add to the abilities of steady-state HR-EELS by being able to image the electromagnetic field and use electrons to excite photon-forbidden and momentum-specific transitions. We discuss the technical challenges ultrafast HR-EELS currently faces, as well as how integration with in situ and cryo measurements could expand the technique to new systems of interest, especially molecular and biological samples.

Copyright and License

© 2023 Author(s). Published under an exclusive license by AIP Publishing.

Acknowledgement

This research was supported as part of the Ensembles of Photosynthetic Nanoreactors, an Energy Frontiers Research Center funded by the U.S. Department of Energy, Office of Science under Award No. DE-SC0023431. Y.-J.K. is further supported by the Liquid Sunlight Alliance (the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Fuels from Sunlight Hub under Award No. DE-SC0021266). L.D.P. is supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE‐1745301. W.L. acknowledges further support from the Korea Foundation for Advanced Studies.

Contributions

Ye-Jin Kim: Conceptualization (equal); Visualization (equal); Writing – original draft (lead); Writing – review & editing (lead). Levi D. Palmer: Conceptualization (equal); Visualization (lead); Writing – original draft (equal); Writing – review & editing (equal). Wonseok Lee: Conceptualization (equal); Visualization (equal); Writing – original draft (equal); Writing – review & editing (equal). Nicholas J. Heller: Conceptualization (equal); Visualization (supporting); Writing – original draft (supporting). Scott K. Cushing: Conceptualization (lead); Funding acquisition (lead); Writing – original draft (equal); Writing – review & editing (equal).

Data Availability

The data that support the findings of this study are available from the corresponding author upon reasonable request.

Conflict of Interest

The authors have no conflicts to disclose.

Files

050901_1_5.0147356.pdf
Files (16.3 MB)
Name Size Download all
md5:03e253c0f3504b66f70662de01ab1a7d
16.3 MB Preview Download

Additional details

Created:
October 27, 2023
Modified:
August 7, 2024