Exploring Gauge-Higgs Inflation with Extra Dimensions: Abstract and Introduction

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Delve into the mysteries of inflation with 5D U(1) gauge theory in a warped spacetime, exploring its implications for early universe dynamics.

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Inflation can solve both the flatness problem and the horizon problem at the same time and also explain temperature fluctuations of the cosmic microwave background (CMB) It is almost certain that inflation occurred in the early universe. In our model, fields involved in inflation obey a different type of boundary condition from that of the visible particles. A surviving Wilson line phase can play a specific role for physics beyond the standard model.