Bright Light for Ultrafast Snapshots of Materials

Estimated reading time: 4 minutes

If you want to understand how novel phases emerge in correlated materials, including high-temperature superconductivity and nanoscale electronic order, you can obtain completely new viewpoints by taking ‘snapshots’ of underlying rapid electronic interactions. One way to do this is by delivering pulses of extremely short-wavelength UV light to a material and deriving information based on the energy and direction of travel of the emitted electrons. However, generating pulsed extreme-UV (XUV) light with the required properties for such applications is difficult to achieve.

Now, researchers at the U.S. Department of Energy (DOE)’s Lawrence Berkeley National Laboratory (Berkeley Lab) have developed a way of producing an efficient, high-repetition-rate XUV source for use in obtaining rapid, sharp images of electronic structure.

“Like taking a photo on a bright day as opposed to dim twilight, if you have a bright laser source, you can cut down the measurement noise and take excellent data because you have a lot of photons to work with” says Robert Kaindl, a condensed matter physicist with Berkeley Lab’s Materials Sciences Division, who led the work. “But there’s a catch: for experiments such as photoemission the light has to be distributed across as many pulses as possible, to avoid unwanted blurring of the measured spectra.”

Angle-resolved photoemission spectroscopy, or ARPES, is a key technique that makes use of the photoelectric effect for studying condensed matter materials. By analyzing the emitted electrons, it provides direct information about a material’s electronic structure in energy and momentum space. But standard detectors used for static measurements are about ten trillion times slower than the timescale on which electrons interact with each other. To access such microscopic timescales requires a different measurement technique based on extremely short pulses of light, on the order of 10 to 100 femtoseconds (1 fs is 10-15 s).

Importantly, the photon energy of light also needs to overcome the work function of the material – with shorter wavelengths allowing for a more comprehensive view of electronic structure across energy and momentum. Thus, time-resolved ARPES requires overcoming two challenges: generating short-wavelength XUV light, and pulsing it at rapid intervals with a small number of photons per pulse, to minimize blurring from electron-electron interactions that occur after photoemission.

“It’s very difficult to generate XUV light in the first place. This is made possible by a process called high-harmonic generation, where you expose atoms to extremely strong laser fields with peak intensities of 100 Terawatts or more,” explains He Wang, who developed the source as a postdoctoral researcher at Berkeley Lab while working with Kaindl. “An electron can then tunnel out of the atom and return having picked up a lot of energy that, subsequently, it can lose by emitting an XUV photon. An important result of our work is that we achieve very efficient high-harmonic conversion into the XUV, despite operating at high repetition rates where the driving laser power has to be divided among many pulses.”

The scheme first converts infrared pulses from an amplified femtosecond laser into the UV, then gains back orders-of-magnitude in efficiency through subsequent high-harmonic conversion. At the high rate of 50,000 pulses/second, the correspondingly weak UV-driving pulses have to be focused tightly into the thin column of Krypton gas where high-harmonic generation occurs. However, this intermediate step yields a more than hundred-fold boost of XUV conversion efficiency, compared to driving the process directly with the infrared laser. 

The Berkeley Lab study demonstrated an exceptionally bright XUV source flux, with the strongest harmonic line occurring at a wavelength of 56 nm (photon energy ~22 eV) and exceeding 1013 photons/second. By accompanying these experiments with numerical calculations, Wang and Kaindl explained the observed efficiency boost through a combination of favorable electron dynamics in the intense UV laser field, together with a near-optimal coherent buildup of XUV light across the gas. In addition to flux enhancement, the setup also delivers other benefits.

“High-harmonic sources generate a series of lines with different XUV wavelengths, a show-stopper for applications like ARPES where spectra from different lines will get entangled,” says Kaindl. “In contrast, our scheme isolates a single XUV harmonic using only thin metal filters, resulting in a very compact beamline.”

The harmonic has an energy width of 72 meV, corresponding to only 0.3 % of the photon energy.

“That is extremely narrow for high harmonics, and allows us to take sharp images of the electronic structure in materials,” Wang says.

With this bright, high repetition-rate XUV source, researchers now have the opportunity to gain new insights into the physics of correlated materials by tracking their rapid, fundamental interactions across large swaths of energy and momentum space. Beyond that, these femtosecond XUV pulses represent a powerful tool for other applications such as short-wavelength metrology, coincidence and time-of-flight spectroscopy of molecules, and nanoscale imaging.

Kaindl and Wang are corresponding authors of a paper titled ‘Bright high-repetition-rate source of narrowband extreme-ultraviolet harmonics beyond 22eV” describing this research in the journal Nature Communications. Co-authoring the paper are Yiming Xu, Stefan Ulonska, Joseph Robinson and Predrag Ranitovic.

This research was funded by the DOE Office of Science.

About Lawrence Berkeley National Laboratory

Lawrence Berkeley National Laboratory addresses the world’s most urgent scientific challenges by advancing sustainable energy, protecting human health, creating new materials, and revealing the origin and fate of the universe. Founded in 1931, Berkeley Lab’s scientific expertise has been recognized with 13 Nobel prizes. The University of California manages Berkeley Lab for the U.S. Department of Energy’s Office of Science. For more, visit www.lbl.gov.

About DOE

DOE’s Office of Science is the single largest supporter of basic research in the physical sciences in the United States, and is working to address some of the most pressing challenges of our time. For more information, please visit the Office of Science website at science.energy.gov/.