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étude de la diffraction en géométrie de Laue : application à l'astrophysique nucléaire

Abstract : The gamma-ray lens is a new type of instrument for high energy astrophysic, ranging from about 100 keV to 1.3 MeV. Its goals are the gamma-ray lines and the precise localisation of the gamma source owing to its unprecedent angular resolution (roughly 60 arc secondes) and its good energy resolution (DE/E " 1%). The aim of the CLAIRE project is to execute the first balloon flight of the lens to observe the Crab nebula.
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https://tel.archives-ouvertes.fr/tel-00003544
Contributor : Philippe Laporte <>
Submitted on : Monday, October 13, 2003 - 1:32:15 PM
Last modification on : Thursday, October 15, 2020 - 4:07:37 AM
Long-term archiving on: : Friday, April 2, 2010 - 7:38:01 PM

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  • HAL Id : tel-00003544, version 1

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Philippe Laporte. étude de la diffraction en géométrie de Laue : application à l'astrophysique nucléaire. Astrophysique [astro-ph]. Université Paul Sabatier - Toulouse III, 2000. Français. ⟨tel-00003544⟩

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