Derivation · draft
Slow-Roll Inflation from a Scalar Field
D-343
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Threads fields · energy · symmetry · chance
Depends on The Friedmann Equations from Einstein's Equations, scalar-field-stress-energy, Particle Horizon, Horizon and Flatness Problems
Statement
A scalar field with dominant potential energy drives quasi-exponential expansion under the slow-roll conditions, solving the horizon and flatness problems.
Depends on
The Friedmann Equations from Einstein's Equations, scalar-field-stress-energy, Particle Horizon, Horizon and Flatness Problems
Used by
PU-308/L24