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GALAXIES beamline

Research Contents / Beamlines / GALAXIES: IXS - HAXPES

The GALAXIES beamline is dedicated to inelastic x-ray scattering (IXS) and hard x-ray photoemission (HAXPES). These spectroscopic techniques are powerful probes to characterize the electronic properties of materials. The beamline is optimized to operate in the 2.3 et 12 keV energy range with high resolution and micro beam.

 
GALAXIES
Hard x rays induce a MUST ultrafast dissociation phenomenon.
 
 

Interaction of light with matter is multifarious. Light can be absorbed, emitted, reflected, scattered. It can warm and cool, destroy or heal. Light, or electromagnetic radiation, of various specific characteristics, is often used in research to get insights into the laws of nature, e.g. properties of matter, its structure, formation or degradation. The energy carried by the absorbed light may lead to matter ionization or its transfer to unstable transient excited states, which would then relax, releasing the excess energy (all at once or by portions in several steps) in many forms, e. g. emission of photons and/or electrons, which is often accompanied by structural deformations, such as changes in bond lengths, twisting and rotation of bond angles, isomerization or even bond breakages. [Full story]


 
 
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Beamline description

GALAXIES is an undulator beamline dedicated to hard x-ray spectroscopy. The main experimental techniques are:
- Inelastic x-ray scattering (IXS)
- Hard x-ray photoemission spectroscopy (HAXPES)
 
Technical data | Scientific opportinities | Staff | Partners

Beamline News

All the news from the GALAXIES beamline installation, commissioning.
 
Planning | Commissioning | Installation

Research News

All the scientific news on the beamline
 
Highlights | Workshops

User guide

Everything you need to know about the beamline use and performances
 
Overview | References

 Beamline scientific articles
 

Other News

- Superconductivity and nickelates

- Characterization of the electronic properties of a functionalized oxides interface

Good reasons for using hard X-ray photoemission spectroscopy

July 2011: First XAS spectra

April 2011: First monochromatic beam

July 2010: First beam

Delivery of the RIXS spectro

Start of construction

All beamline news


Preliminary Project

Beamline description 

 Download diagram
of the energy ranges

Poster

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