Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion
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arXiv
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| Format: | Preprint |
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2026
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| _version_ | 1866911737855344640 |
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| author | Latosh, Boris |
| author_facet | Latosh, Boris |
| contents | We study a minimal two-field scalar-tensor completion of Starobinsky inflation motivated by the one-loop effective action of scalar-tensor gravity. The model admits an exact Starobinsky branch, but the relevant question is whether nearby trajectories generate observable multifield effects. We show that a non-trivial class of initial conditions relaxes to an attractor-connected slow-roll branch continuously connected to the Starobinsky solution. We then solve the coupled adiabatic and entropy perturbation equations numerically. On the branch studied here, the entropy mode remains sufficiently suppressed that its sourcing of the curvature perturbation is negligible, while the tensor sector is unchanged. The inflationary observables therefore remain effectively Starobinsky-like, providing a robustness test of Starobinsky inflation against a minimal radiative scalar-tensor deformation. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2604_15931 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion Latosh, Boris General Relativity and Quantum Cosmology High Energy Physics - Theory We study a minimal two-field scalar-tensor completion of Starobinsky inflation motivated by the one-loop effective action of scalar-tensor gravity. The model admits an exact Starobinsky branch, but the relevant question is whether nearby trajectories generate observable multifield effects. We show that a non-trivial class of initial conditions relaxes to an attractor-connected slow-roll branch continuously connected to the Starobinsky solution. We then solve the coupled adiabatic and entropy perturbation equations numerically. On the branch studied here, the entropy mode remains sufficiently suppressed that its sourcing of the curvature perturbation is negligible, while the tensor sector is unchanged. The inflationary observables therefore remain effectively Starobinsky-like, providing a robustness test of Starobinsky inflation against a minimal radiative scalar-tensor deformation. |
| title | Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2604.15931 |