Abstract
A model of gravitationally anticollapsing objects, white holes, is constructed on the basis of the Kerr metric in the limit of small rotation with a corresponding interior metric. The extended space-time manifold is considered and the spectral shift of radiation from the point of view of a remote observer is calculated for different parameters of such white holes.
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Gurin, V.S. Slowly rotating white holes. Pramana - J Phys 38, 249–256 (1992). https://doi.org/10.1007/BF02875371
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DOI: https://doi.org/10.1007/BF02875371