Comment on "Strong constraints on magnetized white dwarfs surpassing the Chandrasekhar mass limit"
Upasana Das, Banibrata Mukhopadhyay

TL;DR
This paper critically examines previous claims about the magnetic field limits of super-Chandrasekhar white dwarfs, identifying errors that support their stability and challenging earlier conclusions.
Contribution
It provides a corrected analysis of magnetic field bounds in super-Chandrasekhar white dwarfs, refuting prior erroneous calculations and supporting their potential stability.
Findings
Previous bounds on magnetic fields were incorrect
Corrected calculations support stability of super-Chandrasekhar white dwarfs
Identified numerical errors in prior work
Abstract
We show that the upper bound for the central magnetic field of a super-Chandrasekhar white dwarf calculated by Nityananda and Konar [Phys. Rev. D 89, 103017 (2014)] is completely erroneous. This in turn strengthens the argument in favor of the stability of the recently proposed magnetized super-Chandrasekhar white dwarfs. We also point out several other numerical errors in their work. Overall we conclude, based on our calculations, that the arguments put forth by Nityananda and Konar are fallacious and misleading.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Stellar, planetary, and galactic studies
