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- W1964871330 startingPage "3746" @default.
- W1964871330 abstract "A method is investigated which enables exact solutions to be found for k=0 Friedmann cosmological models with a perfect fluid satisfying the equation of states p=(ensuremath{gamma}-1)ensuremath{rho}, where ensuremath{gamma} is constant and 0ensuremath{le}ensuremath{gamma}ensuremath{le}2, in scalar-tensor gravity theories with an arbitrary form for the gravitational coupling function ensuremath{omega}(ensuremath{varphi}), which defines the theory. A number of explicit solutions are investigated for p=0 universes and inflationary universes, including those for theories in which ensuremath{omega}(ensuremath{varphi}) has a power-law dependence on the scalar field ensuremath{varphi}. When p=-ensuremath{rho} new varieties of inflation arise in which a(t)ensuremath{propto}${mathit{t}}^{mathit{n}}$exp(${mathit{H}}_{0}$${mathit{t}}^{mathit{m}}$)." @default.
- W1964871330 created "2016-06-24" @default.
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- W1964871330 date "1994-09-15" @default.
- W1964871330 modified "2023-10-10" @default.
- W1964871330 title "Perfect fluid scalar-tensor cosmologies" @default.
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- W1964871330 doi "https://doi.org/10.1103/physrevd.50.3746" @default.
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