Inflation and dark energy from f(R) gravity
Artymowski, Michal · Lalak, Zygmunt
Original · EN
The standard Starobinsky inflation has been extended to the R + αRⁿ - βR²⁻ⁿ model to obtain a stable minimum of the Einstein frame scalar potential of the auxiliary field. As a result we have obtained obtain a scalar potential with non-zero value of residual vacuum energy, which may be a source of Dark Energy. Our results can be easily consistent with PLANCK or BICEP2 data for appropriate choices of the value of n.
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