AVS 71 Session LS-ThP: Light Sources Enabled Science Mini-Symposium Poster Session

The National Science Foundation (NSF) National eXtreme Ultrafast Science Facility (NeXUS) is a new open access user facility that provides access to extreme light to researchers around the world. The facility contains a mix of optical and analytical capabilities that allow for the study of chemical and material properties on the time scale of femtoseconds to attoseconds and on the length scale of angstroms. A customized high power, high repetition rate (800 W @ 100 kHz) Yb-doped fiber laser and pulse compression scheme from Active Fiber Systems GmbH is used to produce extreme ultraviolet light (XUV) through high harmonic generation. The XUV light is conditioned through three beamlines, which provide tailored light to a variety of end stations, three of which support materials analysis: X-ray absorption/reflection spectroscopy (XAS/XRS), Angle Resolved Photoemission Spectroscopy (ARPES), and Scanning Tunneling Microscopy (STM).

The combination of an ultrafast XUV beamline with more traditional condensed matter characterization tools, such as ARPES and STM, provides expanded capabilities for user experiments. ARPES is a surface sensitive technique that typically uses a helium discharge lamp to eject photoelectrons, and measurement of their energy and momenta allows for the study of electronic structure in reciprocal space. The addition of a beamline capable of providing light in an optical-pump XUV-probe arrangement allows the NeXUS ARPES to probe charge and carrier dynamics with sub-picosecond time resolution.

STM is a surface characterization technique used to study physical and electronic structure, with angstrom scale spatial resolution, by measuring the tunneling current across a nanoscale junction between the sample and an atomically sharp metal tip. At NeXUS, Thetailored light provided by the beamline addresses two long-standing weaknesses of STM measurements: poor time resolution (> ~1 µs), and lack of elemental specificity. The beamline allows for optical-pump probe measurements, which combine ~100 fs time resolution with angstrom scale spatial resolution of the STM. Additionally, XUV light can be tuned across an atomic core edge, resulting in a spike in photocurrent that is collected by the STM tip, yielding a spatially resolved elemental map of a surface.

This poster will present the preliminary results and progress during the commissioning and inaugural user experiments at NeXUS.