Statistics – Computation
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.125..305c&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 125, no. 2, Aug. 1986, p. 305-309.
Statistics
Computation
3
Computational Astrophysics, Cosmology, Isotropism, Polytropic Processes, Two Fluid Models
Scientific paper
The process of re-escalation of the scalar field φ as φR3 ≡ ψ, the energy density ρ as ρR3 ≡ ɛ, and the pressure p as pR3 ≡ P, lends itself to obtain a reduced equation that represents, for a wide variety of equations of state, the cosmological evolution of an homogeneous and isotropic, flat Universe. A particular solution to this equation is presented.
Chauvet Pablo
Klapp Jaime
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