Objective
The goal of the project is the development of a multipurpose, scalable, parallel, high- performance 3D code, evolving both relativistic gravitational fields and hydrodynam- ics, for the study of relativistic astrophysics and gravitational wave astronomy. The code will be obtained by coupling the existing NCSA/AEI efficient vacuum general relativity code to Valencia's group relativistic hydrodynamic code. This project will be one of the first to solve simultaneously both sides of Einstein field equations. For this purpose, it will take advantage of the latest developments in numerical relativity and computational science. This project represents a major step forward to model the evolution of matter in a dynamical 3D spacetime, thereby allowing the study of all components of relativistic astrophysics, including highly dynamic gravitational fields, strong gravitational waves, relativistic fluid motion, and shocks.
Fields of science (EuroSciVoc)
CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques.
CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques.
- natural sciencesphysical sciencesrelativistic mechanics
- natural sciencesphysical sciencesastronomyobservational astronomygravitational waves
- natural sciencescomputer and information sciencescomputational science
- natural sciencesphysical sciencesastronomyastrophysics
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Call for proposal
Data not availableFunding Scheme
RGI - Research grants (individual fellowships)Coordinator
14476 GOLM
Germany