Relativistic Radiation Hydrodynamics of Spherical Accretion

Details Relativistic Radiation Hydrodynamics of Spherical Accretion Relativistic Radiation Hydrodynamics of Spherical Accretion

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jkas...34..305p&link_type=abstract

Journal of the Korean Astronomical Society, vol. 34, no. 4, pp. 305-307

Physics

4

Accretion, Black Hole Physics, Radiative Transfer

Scientific paper

Radiation hydrodynamics in high velocity or high optical-depth flow should be treated under rigorous relativistic formalism. Relativistic radiation hydrodynamic moment equations are summarized, and its application to the near-critical accretion onto neutron star is discussed. The relativistic effects can dominate the dynamics of the flow even when the gravity is weak and the velocity is small. First order equations fail to describe the intricate relativistic effects correctly.

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