Strong constraints on magnetized white dwarfs surpassing the Chandrasekhar mass limit

TL;DR

This paper demonstrates that white dwarf models claiming masses above the Chandrasekhar limit due to strong magnetic fields are physically unviable because Lorentz forces prevent such equilibrium configurations.

Contribution

It provides a detailed analysis showing that magnetic fields exceeding certain bounds cannot support super-Chandrasekhar white dwarf models, challenging recent proposals based on modified equations of state.

Findings

Super-strong magnetic fields are incompatible with white dwarf equilibrium.

Lorentz forces significantly limit the magnetic field strength in white dwarfs.

Super-Chandrasekhar white dwarf models are unphysical when Lorentz forces are considered.

Abstract

We show that recently proposed white dwarf models with masses well in excess of the Chandrasekhar limit, based on modifying the equation of state by a super-strong magnetic field in the centre, are very far from equilibrium because of the neglect of Lorentz forces. An upper bound on the central magnetic fields, from a spherically averaged hydrostatic equation, is much smaller than the values assumed. Robust estimates of the Lorentz forces are also made without assuming spherical averaging. These again bear out the results obtained from a spherically averaged model. In our assessment, these estimates rule out the possibility that magnetic tension could change the situation in favor of larger magnetic fields. We conclude that such super-Chandrasekhar models are unphysical and exploration of their astrophysical consequences is premature. Erratum : We correct certain numerical estimates made in our paper. This correction however does not alter the conclusion that when Lorentz forces are taken into account the super-massive white dwarf models, obtained simply by modifying the equation of state in presence of a super-strong magnetic field in the centre, fail to be in equilibrium.