CoCoNuT: General relativistic hydrodynamics code with dynamical space-time evolution

Details CoCoNuT: General relativistic hydrodynamics code with dynamical space-time evolution CoCoNuT: General relativistic hydrodynamics code with dynamical space-time evolution

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ascl.soft02012d&link_type=abstract

Astrophysics Source Code Library, record ascl:1202.012

Astronomy and Astrophysics

Astrophysics

Scientific paper

CoCoNuT is a general relativistic hydrodynamics code with dynamical space-time evolution. The main aim of this numerical code is the study of several astrophysical scenarios in which general relativity can play an important role, namely the collapse of rapidly rotating stellar cores and the evolution of isolated neutron stars. The code has two flavors: CoCoA, the axisymmetric (2D) magnetized version, and CoCoNuT, the 3D non-magnetized version.

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