Gas dynamics in strong gravitational fields

Details Gas dynamics in strong gravitational fields Gas dynamics in strong gravitational fields

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982gregr..14..399h&link_type=abstract

General Relativity and Gravitation, vol. 14, Apr. 1982, p. 399-410.

Astronomy and Astrophysics

Astronomy

1

Axisymmetric Flow, Black Holes (Astronomy), Gas Dynamics, Gravitational Fields, Relativity, Field Theory (Physics), Hydrodynamic Equations, Ideal Fluids, Oblique Shock Waves, Shock Wave Interaction

Scientific paper

The steady and axially symmetric flow of a perfect fluid is studied in the context of general relativistic gas dynamics. It is assumed that the flow occurs in the background field of a rotating black hole (or any compact object). The hydrodynamic equations are referred to a locally nonrotating frame and their characteristics are found. The equations describing oblique shock waves are also obtained.

Affiliated with

Also associated with

No associations

Rating

Gas dynamics in strong gravitational fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gas dynamics in strong gravitational fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gas dynamics in strong gravitational fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-841759