Magnetic Fields in GRB Progenitors

Details Magnetic Fields in GRB Progenitors Magnetic Fields in GRB Progenitors

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1799m&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

The Newtonian condition for the equilibrium of a star endowed with a uniform magnetic field is studied as an initial datum for a magnetic field coupled to a Schwarzschild black hole. Such a magnetic field is equivalent to an "effective" field in a flat space-time according to a distant observer. The effective field is studied and it's found that it reaches a maximum value and then it vanishes at the event horizon of the star. Assuming as initial condition the maximum value of the magnetic field of a self-gravitating system established the maximum magnetic field, coupled to a body of mass M, as measured by a distant observer is estimated.

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