0000000001135559

AUTHOR

Alexei A. Starobinsky

showing 2 related works from this author

f(R) constant-roll inflation

2017

The previously introduced class of two-parametric phenomenological inflationary models in General Relativity in which the slow-roll assumption is replaced by the more general, constant-roll condition is generalized to the case of $f(R)$ gravity. A simple constant-roll condition is defined in the original Jordan frame, and exact expressions for a scalaron potential in the Einstein frame, for a function $f(R)$ (in the parametric form) and for inflationary dynamics are obtained. The region of the model parameters permitted by the latest observational constraints on the scalar spectral index and the tensor-to-scalar ratio of primordial metric perturbations generated during inflation is determin…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General relativityScalar (mathematics)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. RadioactivityEinstein010306 general physicsParametric equationEngineering (miscellaneous)Mathematical physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsFunction (mathematics)High Energy Physics - Theory (hep-th)Metric (mathematics)symbolslcsh:QC770-798Constant (mathematics)Astrophysics - Cosmology and Nongalactic AstrophysicsEuropean Physical Journal C: Particles and Fields
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Constant-roll inflation: confrontation with recent observational data

2017

The previously proposed class of phenomenological inflationary models in which the assumption of inflaton slow-roll is replaced by the more general, constant-roll condition is compared with the most recent cosmological observational data, mainly the Planck ones. Models in this two-parametric class which remain viable appear to be close to the slow-roll ones, and their inflaton potentials are close to (but still different from) that of the natural inflation model. Permitted regions for the two model parameters are presented.

High Energy Physics - TheoryClass (set theory)Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Physics and AstronomyModel parametersGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesPlanck010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsInflatonHigh Energy Physics - Theory (hep-th)symbolsObservational studyConstant (mathematics)Astrophysics - Cosmology and Nongalactic Astrophysics
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