How to tell the shape of a wormhole by its quasinormal modes
Here we shall show how to reconstruct the shape function of a spherically symmetric traversable Lorenzian wormhole near its throat if one knows high frequency quasinormal modes of the wormhole. The wormhole spacetime is given by the Morris–Thorne ansatz. The solution to the inverse problem via fitti...
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| Format: | Article |
| Language: | English |
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Elsevier
2018-09-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S037026931830563X |