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Population III stars are believed to be rapidly-rotating sources with a massrange of hundreds to thousand of solar masses. Masses larger than 260 M$_\odot$are expected to collapse resulting in central rotating Kerr black holes withlarge rotation parameter a. Due to particle-antiparticle asymmetry is small, weuse the neutrino effective potential up to order $1/M_W^4$ in a magnetizedplasma at the base of the ejecta to constrain the rotation parameter by meansof neutrino oscillations. Additionally, we investigate the implications in themagnetic field, temperature and electron asymmetry.

Neutrino Oscillation as a constraint in the dynamics of Pop III Gamma Ray Bursts