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DC Field | Value | Language |
---|---|---|
dc.contributor.author | NITYANANDA, RAJARAM | en_US |
dc.contributor.author | Konar, Sushan | en_US |
dc.date.accessioned | 2020-10-26T06:38:37Z | - |
dc.date.available | 2020-10-26T06:38:37Z | - |
dc.date.issued | 2015-01 | en_US |
dc.identifier.citation | Physical Review D, 91(2). | en_US |
dc.identifier.issn | 1550-7998 | en_US |
dc.identifier.issn | 1550-2368 | en_US |
dc.identifier.uri | http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5296 | - |
dc.identifier.uri | https://doi.org/10.1103/PhysRevD.91.028301 | en_US |
dc.description.abstract | The supermassive white dwarf models proposed by Das and Mukhopadhyaya [Phys. Rev. D 86, 042001 (2012)], based on modifying the equation of state by a superstrong magnetic field in the center, are very far from equilibrium because of the neglect of Lorentz forces, as has recently been shown by Nityananda and Konar [Phys. Rev. D 89, 103017 (2014]. | en_US |
dc.language.iso | en | en_US |
dc.publisher | American Physical Society | en_US |
dc.subject | Physics | en_US |
dc.subject | 2015 | en_US |
dc.title | Comment on "Strongly magnetized cold degenerate electron gas: Mass-radius relation of the magnetized white dwarf" | en_US |
dc.type | Article | en_US |
dc.contributor.department | Dept. of Physics | en_US |
dc.identifier.sourcetitle | Physical Review D | en_US |
dc.publication.originofpublisher | Foreign | en_US |
Appears in Collections: | JOURNAL ARTICLES |
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