AVS 65th International Symposium & Exhibition
    Novel Trends in Synchrotron and FEL-Based Analysis Focus Topic Wednesday Sessions
       Session SA+AS+MI-WeA

Invited Paper SA+AS+MI-WeA7
Development of Ambient Pressure HAXPES and other HAXPES Measurements at SPring-8 for Buried Interface

Wednesday, October 24, 2018, 4:20 pm, Room 202A

Session: Hard X-Ray Photoemission for Probing Buried Interfaces
Presenter: Yasumasa Takagi, Japan Synchrotron Radiation Research Institute (JASRI), Japan
Correspondent: Click to Email

A near ambient pressure photoelectron spectroscopy measurement that use with hard X-rays (AP-HAXPES) were conducted at the BL36XU of SPring-8. The AP-HAXPES system with a commercial differential pumping-type spectrometer (R4000 HiPP-2, Scienta Omicron Inc.) was installed in the beamline. The excitation light of 7.94 keV focused to a beam size of 20 μm x 20 μm on the sample surface was used. The standard aperture size at the top of the front cone in the spectrometer is a diameter of 300 μm. In this report, we replaced the front cone with our home-made one with an aperture diameter of 30 μm to increase the pressure limit in the AP- HAXPES measurement. Meanwhile, we have adapted the working distance of 60 μm in order not to perturb the gas environment at the sample surface.

We measured the XPS spectra of the Au(111) surface grown on a mica substrate under various gas pressures using the AP-HAXPES equipment. The intensity decay of the Au 4f spectra with an increasing gas pressure from 1 Pa to 100 kPa. Here we use “100 kPa” as the atmospheric pressure. The XPS measurement was not affected by the ambient gas at a pressure of 1 Pa. As the gas pressure increased, the signal intensity decreased because the photoelectrons were scattered by the ambient gas while passing through the sample to the detector. Although the signal intensity was very weak at the atmospheric pressure, the peaks of 4f5/2 and 4f7/2 can be detected. The signal-to-noise ratio can be improved by a prolonged acquisition time. The 4f7/2 and 4f5/2 peaks are clearly found in the spectrum at the atmospheric pressure in an acquisition time of 30 min. The Shirley background was subtracted from the spectrum, and the plots were fitted with a Voigt function. The curve fitting result shows that the energy difference between the 4f7/2 and 4f5/2 peaks is 3.7 eV and the intensity ratio 4f7/2:4f5/2 is almost 4:3. These values are in good agreement with the standard value of the Au 4f peaks. Thus, a photoelectron spectroscopy under atmospheric pressure was successfully obtained using an aperture of 30 μm.