TY - JOUR
T1 - Diffraction efficiency of a small-period astronomical x-ray reflection grating fabricated using thermally activated selective topography equilibration
AU - McCurdy, Ross C.
AU - Miles, Drew M.
AU - McCoy, Jake A.
AU - Grisé, Fabien
AU - McEntaffer, Randall L.
N1 - Funding Information:
The authors would like to thank Chad Eichfeld and Michael Labella for their assistance with grating fabrication and Eric Gullikson for his support at ALS. This research used resources of the Nanofabrication Laboratory and the Materials Characterization Laboratory at the Materials Research Institute at The Pennsylvania State University, as well as the Advanced Light Source, which is a DOE Office of Science User Facility under contract no. DE-AC02-05CH11231. This work is supported by NASA under Grants Nos. 80NSSC18K0282, NNX17AD19G, and NASA Space Technology Research Fellowships. The authors have no relevant financial interests in the manuscript and no other potential conflicts of interest to disclose.
Publisher Copyright:
© 2020 Society of Photo-Optical Instrumentation Engineers (SPIE).
PY - 2020/10/1
Y1 - 2020/10/1
N2 - We have fabricated a blazed x-ray reflection grating with a period of 160 nm using thermally activated selective topography equilibration (TASTE) and electron-beam (ebeam) physical vapor evaporation. TASTE makes use of grayscale ebeam lithography to create three-dimensional (3-D) structures in resist, which can then be thermally reflown into a desired profile. A blazed grating profile can be fabricated by selectively reflowing a periodic staircase structure into a wedge. This was done for the first time at a grating period of 160 nm, 2.5 times smaller than previous x-ray gratings fabricated using TASTE. The grating was patterned over a 10 mm by 60 mm area in a 147-nm-Thick layer of poly(methyl methacrylate) resist and coated with 5 nm of chromium and 15 nm of gold using ebeam evaporation. The diffraction efficiency of the grating was measured using beamline 6.3.2 at Lawrence Berkeley National Laboratory's Advanced Light Source. The results show a total absolute diffraction efficiency â‰340 % at lower energies, with maximum single-order diffraction efficiency ranging from 20% to 40%. The total diffraction efficiency was â‰330 % across the measured bandpass of 180 to 1300 eV.
AB - We have fabricated a blazed x-ray reflection grating with a period of 160 nm using thermally activated selective topography equilibration (TASTE) and electron-beam (ebeam) physical vapor evaporation. TASTE makes use of grayscale ebeam lithography to create three-dimensional (3-D) structures in resist, which can then be thermally reflown into a desired profile. A blazed grating profile can be fabricated by selectively reflowing a periodic staircase structure into a wedge. This was done for the first time at a grating period of 160 nm, 2.5 times smaller than previous x-ray gratings fabricated using TASTE. The grating was patterned over a 10 mm by 60 mm area in a 147-nm-Thick layer of poly(methyl methacrylate) resist and coated with 5 nm of chromium and 15 nm of gold using ebeam evaporation. The diffraction efficiency of the grating was measured using beamline 6.3.2 at Lawrence Berkeley National Laboratory's Advanced Light Source. The results show a total absolute diffraction efficiency â‰340 % at lower energies, with maximum single-order diffraction efficiency ranging from 20% to 40%. The total diffraction efficiency was â‰330 % across the measured bandpass of 180 to 1300 eV.
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U2 - 10.1117/1.JATIS.6.4.045003
DO - 10.1117/1.JATIS.6.4.045003
M3 - Article
AN - SCOPUS:85098721264
SN - 2329-4124
VL - 6
JO - Journal of Astronomical Telescopes, Instruments, and Systems
JF - Journal of Astronomical Telescopes, Instruments, and Systems
IS - 4
M1 - 045003
ER -