Author/Authors :
Prada، Francisco نويسنده , , Gunn، James E. نويسنده , , Lupton، Robert H. نويسنده , , IveziC، Zeljko نويسنده , , Schneider، Donald P. نويسنده , , Strauss، Michael A. نويسنده , , Helmi، Amina نويسنده , , Pentericci، Laura نويسنده , , Rockosi، Constance M. نويسنده , , Grebel، Eva K. نويسنده , , Harbeck، Daniel نويسنده , , Knapp، Gillian R. نويسنده , , Brinkmann، Jonathan 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 :
stars , Structure , surveys , photometric , Techniques , general , Galaxy , Halo , Population II
