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

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

2008-02-08

arxiv.org/abs/0802.1148v2

Nuovo Cim.B122:599-602,2007

Astronomy and Astrophysics

Astrophysics

4 pages; paper presented at the "first Italian Pakistan workshop on relativistic astrophysics" June 20-22, 2007

Scientific paper

10.1393/ncb/i2007-10385-7

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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