“School of Physic”
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| Paper IPM / Physic / 7732 |
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| Abstract: | |||||||
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Using the Ehlers transformation along with the
gravitoelectromagnetic approach to stationary spacetimes we
start from the Morgan-Morgan disk spacetime(without radial pressure) as
the seed metric and find its corresponding stationary
spacetime. As expected from the Ehlers transformation the
stationary spacetime obtained suffers from a NUT-type singularity
and the new parameter introduced in the stationary case could be
interpreted as the gravitomagnetic monopole charge (or the NUT
factor). Some of the properties of this spacetime including its particle velocity distribution, gravitational redshift, stability and energy conditions are discussed.
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