Relativistic transport theory
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Publication:2522877
DOI10.1016/0003-4916(66)90207-7zbMath0142.23902OpenAlexW4381948007MaRDI QIDQ2522877
Publication date: 1966
Published in: Annals of Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/0003-4916(66)90207-7
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Cites Work
- On the differential geometry of tangent bundles of Riemannian manifolds. II
- Supernovae, neutrinos, and neutron stars
- Harmonic fields in Riemannian manifolds (Generalized potential theory)
- Internal State of a Gravitating Gas
- Neutrino Theory of Stellar Collapse
- ‘Newtonian’ Time in General Relativity
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
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