CoCoNuT: General relativistic hydrodynamics code with dynami

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

Post by owlice » Sun Feb 19, 2012 6:41 pm

[c]CoCoNuT: General relativistic hydrodynamics code with dynamical space-time evolution[/c][/b]
Abstract: 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.

Credit: Dimmelmeier, Harald; Novak, Jérôme; Cerdá-Durán, Pablo

Site: https://www.uv.es/coconut/
http://adsabs.harvard.edu/abs/2012ApJ...756...84M

Bibcode: 2012ascl.soft02012D

ID: ascl:1202.012
Last edited by Ada Coda on Sun Apr 08, 2018 8:38 pm, edited 1 time in total.
Reason: Updated code entry.
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