Rotating scalar field wormhole
Tonatiuh MatosCIAR Cosmology and Gravity Program, Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, CanadaDarío NúñezInstituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apdo. 70-543, CU, 04510 México, D.F., Mexico
2006en
ABI
Abstract
We derive an exact solution to the Einstein's equations with a stress-energy tensor corresponding to an opposite-sign scalar field, and show that such a solution describes the internal region of a rotating wormhole. We also derive an static wormhole asymptotically flat solution and match them on both regions, thus obtaining an analytic solution for the complete space-time. We explore some of the features of these solutions.
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