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arXiv · 0802.1148

Comments on "Charged particle dynamics in the field of slowly rotating compact star"

Mubasher Jamil·Asghar Qadir
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Abstract

B.M. Mirza \cite{1} presented a solution of coupled Einstein-Maxwell equations for a slowly rotating neutron star; however his derivations had some errors and implicit assumptions that rendered the solution invalid. We point out the errors and present a mathematically consistent solution. The resulting solution is also physically consistent as it remains finite in the no rotation limit, whereas Mirza's solution diverges for zero rotation.

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Mubasher Jamil, Asghar Qadir. 2008-10-28. Comments on "Charged particle dynamics in the field of slowly rotating compact star". https://doi.org/10.1393/ncb%2Fi2007-10385-7

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