Orbits of fluid elements accreting onto a black hole

Details Orbits of fluid elements accreting onto a black hole Orbits of fluid elements accreting onto a black hole

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197..283l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 2, p. 283-288.

Physics

Fluid Dynamics

Accretion Disks, Black Holes (Astronomy), Fluid Flow, Space-Time Functions, Fluid Dynamics, Orbit Calculation, Particle Motion

Scientific paper

The internal pressure can delay the accretion process of fluid flow onto a black hole by an order of magnitude compared with the particle case. The motion of accreting fluid elements inside rms (the marginally stable circular orbit of particles) is not free fall as previously suggested in the standard model of accretion disks. The contribution to the observable output of radiation from fluids in the region inside rms needs to be re-examined.

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