Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5296
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dc.contributor.authorNITYANANDA, RAJARAMen_US
dc.contributor.authorKonar, Sushanen_US
dc.date.accessioned2020-10-26T06:38:37Z-
dc.date.available2020-10-26T06:38:37Z-
dc.date.issued2015-01en_US
dc.identifier.citationPhysical Review D, 91(2).en_US
dc.identifier.issn1550-7998en_US
dc.identifier.issn1550-2368en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5296-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.91.028301en_US
dc.description.abstractThe 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.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectPhysicsen_US
dc.subject2015en_US
dc.titleComment on "Strongly magnetized cold degenerate electron gas: Mass-radius relation of the magnetized white dwarf"en_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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