Comments on "Strongly magnetized cold degenerate electron gas: Mass-radius relation of the magnetized white dwarf"
arXiv:1405.4719 · doi:10.1103/PhysRevD.91.028301
Abstract
The super-massive white dwarf models proposed by Das & Mukhopadhyaya [Phys. Rev. D 86 042001 (2012)], 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, as has recently been shown by Nityananda & Konar [arXiv:1306.1625].
arXiv commentComment on Das & Mukhopadhyay, Phys. Rev. D 86, 042001 (2012); brief summary of Nityananda & Konar, arXiv:1306.1625
References in corpus (9)
- New mass limit for white dwarfs: super-Chandrasekhar type Ia supernova as a new standard candle
- Strongly magnetized cold electron degenerate gas: Mass-radius relation of the magnetized white dwarf
- Stability of super-Chandrasekhar magnetic white dwarfs
- A possible evolutionary scenario of highly magnetized super-Chandrasekhar white dwarfs: progenitors of peculiar type Ia supernovae
- Dynamical instability of white dwarfs and breaking of spherical symmetry under the presence of extreme magnetic fields
- Violation of Chandrasekhar Mass Limit: The Exciting Potential of Strongly Magnetized White Dwarfs
- Mass-radius relation of strongly magnetized white dwarfs: nearly independent of Landau quantization
- Revisiting some physics issues related to the new mass limit for magnetized white dwarfs
- Strong constraints on magnetized white dwarfs surpassing the Chandrasekhar mass limit
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