Geodesic Structure of the Accelerated Stephani Universe
For the spherically symmetric Stephani cosmological model with an accelerated expansion, we investigate the main scenarios of the test particle and photon motion. We show that a comoving observer sees an appropriate picture. In the case of purely radial motion, the radial velocity decreases slightly...
Main Authors: | Irina Bormotova, Elena Kopteva, Zdeněk Stuchlík |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-06-01
|
Series: | Symmetry |
Subjects: | |
Online Access: | https://www.mdpi.com/2073-8994/13/6/1001 |
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