Focusing Telescopes in Nuclear Astrophysics

Scientific Requirements and Prospects.- Prospects in space-based gamma-ray astronomy.- Annihilation of positrons in the Galaxy.- Prospects and requirements for measurements of extragalactic ?-ray lines.- Non-thermal cosmic backgrounds and prospects for future high-energy observations of blazars.- Rolling down from the 30 keV peak: Modelling the hard X-ray and ?-ray backgrounds.- Focusing supernova gamma rays.- Nucleosynthesis in nova explosions: Prospects for its observation with focusing telescopes.- Puzzles and potential for gamma-ray line observations of solar flare ion acceleration.- Gamma-ray Optics.- The INTEGRAL - HESS/MAGIC connection: A new class of cosmic high energy accelerators from keV to TeV.- Replicated nickel optics for the hard-x-ray region.- Small d-spacing WC/SiC multilayers for future hard X-ray telescope designs.- Design aspects of grazing angle multilayer mirrors for soft ?-rays.- Progress toward light weight high angular resolution multilayer coated optics.- InFOC?S hard X-ray imaging telescope.- Development of the HEFT and NuSTAR focusing telescopes.- The SIMBOL-X hard X-ray mission.- Laue diffraction lenses for astrophysics: Theoretical concepts.- Laue diffraction lenses for astrophysics: From theory to experiments.- Mosaic and gradient SiGe single crystals for gamma ray Laue lenses.- Copper mosaic crystals for Laue lenses.- High diffraction efficiency, broadband, diffraction crystals for use in crystal diffraction lenses.- An "ESA-affordable" Laue-lens.- Optical properties of Laue lenses for hard X-rays ( 60 keV).- Development of a new photon diffraction imaging system for diagnostic nuclear medicine.- HAXTEL: A Laue lens telescope development project for a deep exploration of the hard X-ray sky (60 keV).- CLAIRE: First light for a gamma-ray lens.- MAX, a Laue diffraction lens for nuclear astrophysics.- The gamma ray lens - an ESA technology reference study.- Gamma ray Fresnel lenses - why not?.- Development of ground-testable phase fresnel

Peter von Ballmoos est né en 1956 à Zürich. Après des études de physique à l'Ecole Polytechnique Fédérale de Zürich, un doctorat à l'Université Technique de Munich, et des post-docs outre Atlantique, il a été élu professeur d'astrophysique à l'Université de Toulouse en 1991.Au sein du Centre d'Etudes Spatiales des Rayonnements de Toulouse, il mène des recherches en astrophysique nucléaire - en particulier l'instrumentation, l'observation et l'interprétation des raies gamma nucléaires. L'observation des raies gamma nucléaires est une des clés aux questions fondamentales sur la structure et l'évolution de l'Univers, et particulièrement sur les cycles de vie de la matière et du comportement de la matière dans des conditions extrêmes. Peter von Ballmoos est co-responsable du projet Spectromètre INTEGRAL de l'ESA et responsable des projets "lentille gamma" du CNES (CLAIRE, MAX).