Author/Authors :
Bloom، J. S. نويسنده , , Kulkarni، S. R. نويسنده , , Galama، T. J. نويسنده , , Castro، S. نويسنده , , Harrison، F. A. نويسنده , , Holtzman، J. A. نويسنده , , Djorgovski، S. G. نويسنده ,
Abstract :
We assemble the equations of general relativistic magnetohydrodynamics (MHD) in 3 + 1 form. These consist of the complete coupled set of Maxwellʹs equations for the electromagnetic field, Einsteinʹs equations for the gravitational field, and the equations of relativistic MHD for a perfectly conducting ideal gas. The adopted form of the equations is suitable for evolving numerically a relativistic MHD fluid in a dynamical spacetime characterized by a strong gravitational field.
Keywords :
gamma rays , bursts , high-redshift , galaxies
