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arxiv: 2107.05926 · v3 · pith:5PPMCQ4Hnew · submitted 2021-07-13 · 🌀 gr-qc · astro-ph.CO· hep-th

k-Gauss-Bonnet inflation

classification 🌀 gr-qc astro-ph.COhep-th
keywords fieldinflationmodelscalargauss-bonnetabsenceadmitallowed
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We propose a novel {\it k}-Gauss-Bonnet inflationary model, in which a kinetic term of scalar field is allowed to non-minimally couple to the Gauss-Bonnet topological invariant in the absence of a potential of scalar field. As a result, this model is shown to admit an isotropic power-law inflation provided that the scalar field is phantom. Furthermore, stability analysis based on the dynamical system method is performed to indicate that this inflation solution is indeed stable and attractive. More interestingly, a gradient instability in tensor perturbations is shown to disappear in this model.

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  1. Beyond $f(\phi)\mathcal{G}$: Gauss--Bonnet inflation with $\mu(\phi,X)$

    astro-ph.CO 2026-04 unverdicted novelty 6.0

    A phase-space gating function μ(φ,X) localizes Gauss-Bonnet contributions to a finite e-fold window in inflation while preserving ghost and gradient stability for scalar and tensor modes.