Experiments and instruments

A series of short movies showing how neutron experiments are prepared or performed. Some of these movies have an historical interest since they captured important moments in the life of the ILL.

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Films and animations

IN20 - Hydrogen dynamics in the picosecond range

G. Mpourmpakis et al., Nano Lett., 7 (7), 1893 -1897, 2007. 10.1021/nl070530u

Hydrogen is thought to be the fuel of the future since it is abundant and non-polluting. One promising material for the storage of hydrogen is nanoscrolls (a special form of carbon nanotubes). However we still have to dominate the storage/release process and thus we must understand better how hydrogen molecules or atoms bind to carbon atoms.

Such a study is very difficult for four main reasons:

  1. the binding energies are extremely weak, in the range of the micro eV (μeV) i.e. the picosecond time scale. This is beyond the capabilities of today's measuring techniques except for neutron spin echo (SE) spectrometry.
  2. the measurements require both neutron triple axis spectrometry (TAS) which provides the energy analysis, and neutron spin echo (SE), which provides the high resolution. This combination of techniques is called TASSE and only two TASSE neutron spectrometers exist worldwide.
  3. the sample is hydrogen but normal hydrogen (orthohydrogen) is a strong incoherent neutron scatterer which produces a strong background making measurements almost impossible. We must therefore replace orthohydrogen by parahydrogen which makes sample preparation more difficult.
  4. the mount of adsorbed hydrogen in the sample is small compared to the amount of carbon so the very high neutron flux of the ILL reactor is really necessary.

Altogether this means that the ILL instrument IN20-TASSE is certainly the best and only one capable of carrying out such measurements.

The movie below shows the very first steps of the experiment 6-02-407 (3 to 18 nov. 2008). It was very successful and one of the results is that, below 10K, the parahydrogen line halfwidth remains roughly constant at 3 mev and the energy of this line is also constant.

Click HERE to download the 320x240 MPEG-4 movie (file size: 6.7 kb, duration: 3'09)

Click HERE to download the 768x576 MPEG-4 movie (file size: 35.6 Mb, duration: 3'09)

©2008, Institut Laue-Langevin, Grenoble, France

Proposers

  BERMEJO Francisco Javier

Dept. Elect., Univ. Pais Vasco, BILBAO

  CABRILLO Carlos

Inst. Estructura de la Materia, CSIC, Madrid,Spain

  CHICO GOMEZ Leonor

Univ. de Castilla-La Mancha, Toledo, Spain

  FERNANDEZ PEREA Ricardo

Inst. ESTRUCT MAT, CSIC, Madrid, Spain

  FERNANDEZ-ALONSO Felix

ISIS RAL, Didcot, UK

  JIMENEZ-RUIZ Monica

ILL, Grenoble, France

  LEON Vincent

Université Montpellier, France

  SABOUNGI Marie-Louise

CNRS/CRMD-Centre Rech. Matière Divisée, Orléan, France

Local contacts
    CUELLO Gabriel Julio     ILL, GRENOBLE
    ENDERLE Mechthild     ILL, GRENOBLE
    FARHI Emmanuel     ILL, GRENOBLE
    GONZALEZ Miguel Angel     ILL, GRENOBLE

 

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Last update: A.Filhol, 12 Nov 2008.