The GALAXIES inelastic hard X-ray scattering end-station at Synchrotron SOLEIL

被引:27
作者
Ablett, J. M. [1 ]
Prieur, D. [1 ]
Ceolin, D. [1 ]
Lassalle-Kaiser, B. [1 ]
Lebert, B. [1 ,2 ]
Sauvage, M. [1 ]
Moreno, Th. [1 ]
Bac, S. [1 ]
Baledent, V. [3 ]
Ovono, A. [4 ]
Morand, M. [2 ]
Gelebart, F. [2 ]
Shukla, A. [2 ]
Rueff, J. -P. [1 ,5 ]
机构
[1] Synchrotron SOLEIL, BP 48, F-91192 Gif Sur Yvette, France
[2] Sorbonne Univ, CNRS, Inst Mineral Phys Mat & Cosmochim, MNHN,UMR 7590,IRD,UMR 206, 4 Pl Jussieu, F-75005 Paris, France
[3] Lab Phys Solides, F-91400 Orsay, France
[4] Ecole Natl Super Ingn Limoges, Limoges, France
[5] Sorbonne Univ, CNRS, LCPMR, F-75005 Paris, France
关键词
GALAXIES beamline; Synchrotron SOLEIL; inelastic hard X-ray scattering; beamlines; QUARTER-WAVE PLATES; PHOTOELECTRON-SPECTROSCOPY; PHASE PLATE; RESOLUTION; SPECTROMETER; BEAMLINE; RIXS; ANALYZER; FLUORESCENCE; TRANSITION;
D O I
10.1107/S160057751801559X
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
GALAXIES is an in-vacuum undulator hard X-ray micro-focused beamline dedicated to the study of the electronic structure of materials with high energy resolution using both photoelectron spectroscopy and inelastic X-ray scattering and under both non-resonant (NR-IXS) and resonant (RIXS) conditions. Due to the penetrating power of hard X-rays and the `photon-in/photon-out' technique, the sample environment is not a limitation. Materials under extreme conditions, for example in diamond anvil cells or catalysis chambers, thus constitute a major research direction. Here, the design and performance of the inelastic X-ray scattering end-station that operates in the energy range from approximate to 4keV up to 12keV is reported, and its capabilities are highlighted using a selection of data taken from recently performed experiments. The ability to scan `on the fly' the incident and scattered/emitted X-ray energies, and the sample position enables fast data collection and high experimental throughput. A diamond X-ray transmission phase retarder, which can be used to generate circularly polarized light, will also be discussed in the light of the recent RIXS-MCD approach.
引用
收藏
页码:263 / 271
页数:9
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