Minimum amount of inflation to solve the flatness and horizon problems

Physics

Scientific paper

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Origin And Formation Of The Universe, Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

In this note we show that for natural initial conditions at the Planck
time the horizon problem requires only twice as much inflation for its
solution as does the flatness problem. We further argue that with these
initial conditions the Universe is open rather than closed, and was
dominated by gravitational curvature at the onset of inflation.

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