SMS Γ=1.339

Detail

In this case, the supermassive star is seeded with a poloidal dipole-like magnetic field that extends from the interior into the exterior. The stellar model with gas perturbation is described by a polytropic equation of state (EOS) with $\Gamma=1.339$. This EOS is most appropriate for stars with mass $M \sim 10^5 M_\odot$.