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When ϵV is constant: In such a case, graceful exit can only occur if Q decreases

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astro-ph.CO 1

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2025 1

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Behaviour of $\alpha$-attractors in Warm Inflation

astro-ph.CO · 2025-06-10 · reject · novelty 5.0

In strongly dissipative warm inflation, T, E, and polynomial alpha-attractor models lose the cold-inflation attractor convergence in the n_s-r plane.

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  • Behaviour of $\alpha$-attractors in Warm Inflation astro-ph.CO · 2025-06-10 · reject · none · ref 4

    In strongly dissipative warm inflation, T, E, and polynomial alpha-attractor models lose the cold-inflation attractor convergence in the n_s-r plane.