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Laue diffraction lenses for astrophysics: Theoretical concepts
Authors:Hubert Halloin  Pierre Bastie
Affiliation:(1) CESR, 9, avenuedu Colonel Roche, 31028 Toulouse, France;(2) Present address: APC, 11, Place Marcelin Berthelot, 75231 Paris Cedex 05, France;(3) Laboratoire de Spectrométric Physique, BP 87 38402 st., Martin d’Hères Cedex, France;(4) ILL, BP 156, 38402 Grenoble Cedex 9, France
Abstract:Beyond the present technologies, Laue diffraction lenses are very promising tools in the field of gamma-ray astrophysics. The theoretical concepts of this kind of instruments are based on the Laue diffraction in crystals, discovered almost 100 years ago. Though they are commonly used in crystallography, their application to γ-ray focusing in astrophysics requires some specific developments, e.g. in terms of energy and imaging responses. The present article describes the physics of X-ray diffraction in crystals. In the context of the Darwin model of mosaic crystals, some peculiar aspects, relevant to the astrophysical observation, are discussed. The evaluation and optimization of diffraction efficiency are discussed, especially with rigards to the crystal’s mosaicity and thickness, its spatial extent and deviations to the “ideally imperfect” Darwin model. PACS 95.55.Ka, 61.50.Ah, 61.10.−i, 41.50.+h
Keywords:Focusing optics  Gamma-ray astrophysics  Crystal diffraction
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