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Paper detail

The metric of general rotating spacetimes

We propose the metric for general rotating spacetimes. These spacetimes are stationary, axially symmetric and spatially asymptotically flat. They can be the spacetimes outside of rotating black holes or rotating celestial bodies such as the Sun and the Earth. The metric functions are expanded in power series of distance and the angle variable is included in the expansion coefficients.

preprint2022arXivOpen access
Changjun Gao
astro-ph.HEgr-qcastro-ph.SR
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Changjun Gao

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