Oscillating Cosmological Force Modifies Newtonian Dynamics
In the Newtonian limit of general relativity a force acting on a test mass in a central gravitational field is conventionally defined by the attractive Newtonian gravity (inverse square) term plus a small repulsive cosmological force, which is proportional to the slow acceleration of the universe ex...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-05-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/8/2/45 |