Thermodynamic Constraints on the Non-Baryonic Dark Matter Gas Composing Galactic Halos
To explain rotation curves of spiral galaxies through Newtonian orbital models, massive halos of non-baryonic dark matter (NBDM) are commonly invoked. The postulated properties are that NBDM interacts gravitationally with baryonic matter, yet negligibly interacts with photons. Since halos are large,...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-11-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/8/4/77 |