A Solution to the Main Cosmological Problems
May, 19853 pages
Published in:
- Phys.Lett.B 171 (1986) 363-365
- Published: 1986
Report number:
- Print-85-0485 (RIYADH)
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Abstract: (Elsevier)
A model of the universe with an additional term Λ ( x ) g μν in the energy-momentum tensor is motivated and presented. The model is completely determined by the assumption that the energy density ofthe universe equals its critical value. It has k = 1 geometry, is free of the initial singularity and does not possess a horizon, entropy or monopole problem.- COSMOLOGICAL MODEL
- COSMOLOGICAL CONSTANT
- ASTROPHYSICS: CRITICAL PHENOMENA
- TENSOR: ENERGY-MOMENTUM
- ENTROPY
- POSTULATED PARTICLE: MAGNETIC MONOPOLE
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