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Paper detail

Lense-Thirring Precession in Plebański-Demiański spacetimes

An exact expression of Lense-Thirring precession rate is derived for non-extremal and extremal Plebański-Demiański spacetimes. This formula is used to find the exact Lense-Thirring precession rate in various axisymmetric spacetimes, like: Kerr, Kerr-Newman, Kerr-de Sitter etc. We also show, if the Kerr parameter vanishes in Plebański-Demiański(PD) spacetime, the Lense-Thirring precession does not vanish due to the existence of NUT charge. To derive the LT precession rate in extremal Plebański-Demiański we first derive the general extremal condition for PD spacetimes. This general result could be applied to get the extremal limit in any stationary and axisymmetric spacetimes.

preprint2013arXivOpen access
Chandrachur ChakrabortyPartha Pratim Pradhan
astro-ph.HEgr-qc
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Chandrachur ChakrabortyPartha Pratim Pradhan

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