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...
Kaydedildi:
| Yazar: | |
|---|---|
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
MDPI AG
2020-05-01
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| Seri Bilgileri: | Galaxies |
| Konular: | |
| Online Erişim: | https://www.mdpi.com/2075-4434/8/2/45 |
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