Corpus ID: 54004661

Relativistic Dissipative Accretion Flow onto Black Hole

@article{Saida2009RelativisticDA,
  title={Relativistic Dissipative Accretion Flow onto Black Hole},
  author={Hiromi Saida and Rohta Takahashi and Hiroki Nagakura},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2009}
}
Dissipations, e.g. heat flow and bulk and shear viscosities, cause the transport of energy, momentum and angular momentum, which is the essence of accretion of matters onto celestial objects. Dissipations are usually described by the Fourier and Navier-Stokes laws ("classic laws" of dissipations). However the classic laws result in an infinitely fast propagation of dissipations. In relativistic formulation, the classic laws of dissipations violate the causality, and hence no relativistic theory… Expand
1 Citations
A fast numerical scheme for causal relativistic hydrodynamics with dissipation
TLDR
A stable and fast numerical scheme for relativistic dissipative hydrodynamics based on Israel–Stewart theory is developed, and Riemann solver can be used for obtaining numerical flux for the inviscid step. Expand

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