Objective The physical conditions in relativistic jets generated in vicinity of black holes or neutron stars may not be directly accessible to current observations, the reason being that the detected radiation originates from a non-thermal population of relativistic particles which may represent only a part of a more complex system (including a thermal component carying most of the mass of a jet). This project applies state-of-the-art numerical techniques as well as carefully developed analytic models to link the phy sical state of the jet to the radiation associated with the gamma ray bursts (GRBs) and active galactic nuclei (AGN). Fields of science natural sciencesphysical sciencesastronomystellar astronomyneutron starsnatural sciencesphysical sciencesastronomyastrophysicsblack holesnatural sciencesphysical sciencesastronomyobservational astronomyx-ray astronomynatural sciencesphysical sciencesastronomyplanetary sciencescelestial mechanicsengineering and technologyelectrical engineering, electronic engineering, information engineeringelectronic engineeringcomputer hardwaresupercomputers Keywords non-thermal radiation processes numerical hydrodynamics Programme(s) FP6-MOBILITY - Human resources and Mobility in the specific programme for research, technological development and demonstration "Structuring the European Research Area" under the Sixth Framework Programme 2002-2006 Topic(s) MOBILITY-2.3 - Marie Curie Incoming International Fellowships (IIF) Call for proposal FP6-2004-MOBILITY-7 See other projects for this call Funding Scheme EIF - Marie Curie actions-Intra-European Fellowships Coordinator UNIVERSITAT DE VALÈNCIA. ESTUDI GENERAL Address Avda. blasco ibañez, 13. Valencia Spain See on map Links Website Opens in new window EU contribution € 0,00
