General Relativistic Gravitational Collapse of Rotating Star with Magnetic Fields ---The Formalism and the Initial Value Equations---

Details General Relativistic Gravitational Collapse of Rotating Star with Magnetic Fields ---The Formalism and the Initial Value Equations--- General Relativistic Gravitational Collapse of Rotating Star with Magnetic Fields ---The Formalism and the Initial Value Equations---

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pthph..68..567m&link_type=abstract

Progress of Theoretical Physics, Vol. 68, No. 2, pp. 567-579

Physics

2

Scientific paper

Magnetic fields, as well as a rotation, play an essential role in a number of astrophysical situation. We present the formalism for treating dynamically the general relativistic phenomena with magnetic fields, e.g., the gravitational collapse of a magnetized star, when assuming an axial symmetry and magnetohydrodynamics approximation. Next, we give the method of setting up initial values and show some numerical examples.

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