C-field Cosmology with Variable G in the Flat Friedmann Robertson Walker Model

Details C-field Cosmology with Variable G in the Flat Friedmann Robertson Walker Model C-field Cosmology with Variable G in the Flat Friedmann Robertson Walker Model

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007chphl..24.3290r&link_type=abstract

Chinese Physics Letters, Volume 24, Issue 11, pp. 3290-3292 (2007).

Physics

3

Scientific paper

The C-field cosmological model based on the Hoyle Narlikar theory with variable gravitational constant G is investigated. To obtain the deterministic value of dot C = dC/dt we present certain constant values for integration constants. The creation field is proportional to time. G and ρ (density) decrease with time and the universe represents an expanding universe. The creation field increases as time increases. We find C = (1/(2πf))1/2t where f>0. Thus dot C = 1 when f = 1/(2π)>0.

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