General relativistic treatment of magnetofluid disk around compact objects. II - Steady-state solutions

Details General relativistic treatment of magnetofluid disk around compact objects. II - Steady-state solutions General relativistic treatment of magnetofluid disk around compact objects. II - Steady-state solutions

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.141..251p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 141, no. 2, Feb. 1988, p. 251-256.

Astronomy and Astrophysics

Astrophysics

Accretion Disks, Gyromagnetism, Magnetohydrodynamic Flow, Schwarzschild Metric, Lorentz Force, Magnetic Field Configurations, Relativity, Space-Time Functions

Scientific paper

Solutions of magnetofluid accretion disk with negligible self-gravitation have been obtained in the background of the Schwarzschild spacetime for differential as well as rigid rotation. The constraint equations for the magnetic field components have also been derived. It is shown that the magnetic field plays an important role in confining the fluid flow.

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