Spiral Inflation with Coleman-Weinberg Potential
classification
✦ hep-ph
astro-ph.CO
keywords
scaleinflationcoleman-weinbergmathcalpotentialspiralsymmetry-breakingallowed
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We apply the idea of spiral inflation to Coleman-Weinberg potential, and show that inflation matching well observations is allowed for a symmetry-breaking scale ranging from an intermediate scale to GUT scale even if the quartic coupling $\lambda$ is of $\mathcal{O}(0.1)$. The tensor-to-scalar ratio can be of $\mathcal{O}(0.01)$ in case of GUT scale symmetry-breaking.
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