Inflation in the five-dimensional universe with an orbifold extra dimension
Takeshi Nihei (KEK)

TL;DR
This paper constructs new inflationary solutions in a five-dimensional universe with an orbifold extra dimension, exploring effects of bulk and boundary cosmological constants on the inflationary dynamics.
Contribution
It provides explicit inflationary solutions in a simple five-dimensional orbifold model, including cases with non-zero bulk cosmological constant, extending previous work.
Findings
Solutions with static extra dimension and non-trivial background metric.
Inflation driven by bulk and boundary cosmological constants.
New solutions for non-zero bulk cosmological constant.
Abstract
New inflationary solutions to the Einstein equation are explicitly constructed in a simple five-dimensional model with an orbifold extra dimension . We consider inflation caused by cosmological constants for the five-dimensional bulk and the four-dimensional boundaries. In our solutions the extra dimension is static, and the background metric has a non-trivial configuration in the extra dimension. In addition to the solution for a vanishing bulk cosmological constant, which has already been discussed, we obtain solutions for a non-zero one.
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