A critical-density closed Universe in Brans-Dicke Theory
نویسندگان
چکیده
In a Brans-Dicke (BD) cosmological model, the energy density associated with some scalar field decreases as a −2 ( ωo+ 1 2 ωo+1 ) with the scale factor a(t) of the Universe, giving a matter with an Equation of state p = − 1 3 (
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