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On the equivalence between Starobinsky and Higgs inflationary models in gravity and supergravity
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On the equivalence between Starobinsky and Higgs inflationary models in gravity and supergravity
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Starobinsky inflation and Higgs inflation in gravity, and their equivalence based on the common inflationary potential are extended to supergravity in the proper framework, where the Starobinsky and Higgs descriptions of inflation arise in two different gauges of the same supergravity model.
Forward citations
Cited by 5 Pith papers
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Higgs boson mass and thermal wino dark matter from Starobinsky supergravity with the MSSM
Starobinsky supergravity coupled to the MSSM links the CMB inflationary scale to the Higgs boson mass (~125 GeV) and predicts thermal wino dark matter at ~3 TeV, testable at future colliders and direct detection experiments.
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Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion
A minimal two-field radiative completion of Starobinsky inflation remains observably indistinguishable from the original model on the studied attractor-connected slow-roll branch.
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Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion
In this two-field completion, trajectories connected to the Starobinsky solution keep entropy modes suppressed so that curvature and tensor perturbations remain effectively single-field Starobinsky-like.
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Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion
Nearby trajectories in a minimal two-field scalar-tensor completion of Starobinsky inflation relax to an attractor where entropy sourcing is negligible, so observables remain effectively Starobinsky-like.
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On Legacy of Starobinsky Inflation
A memorial review of the Starobinsky inflation model that proposes a deformation for primordial black hole production and discusses superstring quantum corrections plus universal reheating.
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