University of Illinois at Urbana-Champaign
The star has the following general characteristics
The star is modeled as an infinite cylinder initially obeying the above equation of state for static polytropes. We present cases for which n is equal to 0.001, 3, and 5.
In all the calculations, the initial differential rotational profile has the form shown by
the equation above. This rotational profile obeys the necessary boundary
and initial conditions required for our calculations. R represents the radius of the star.
The radial component of the field is independent of time and has the form shown above. In all cases, there is no toroidal component of the magnetic field at t=0.