6533b838fe1ef96bd12a508a

RESEARCH PRODUCT

Upper bound on the tensor-to-scalar ratio in GUT-scale supersymmetric hybrid inflation

Qaisar ShafiMatthew CivilettiConstantinos Pallis

subject

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)SuperpotentialScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryInflatonUpper and lower boundsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Cosmology and Nongalactic AstrophysicsMinimal Supersymmetric Standard ModelGauge symmetry

description

We explore the upper bound on the tensor-to-scalar ratio r in supersymmetric (F-term) hybrid inflation models with the gauge symmetry breaking scale set equal to the value 2.86⋅1016 GeV2.86⋅1016 GeV, as dictated by the unification of the MSSM gauge couplings. We employ a unique renormalizable superpotential and a quasi-canonical Kähler potential, and the scalar spectral index nsns is required to lie within the two-sigma interval from the central value found by the Planck satellite. In a sizable region of the parameter space the potential along the inflationary trajectory is a monotonically increasing function of the inflaton, and for this case, r≲2.9⋅10−4r≲2.9⋅10−4, while the spectral index running, View the MathML source|dns/dlnk|, can be as large as 0.01. Ignoring higher order terms which ensure the boundedness of the potential for large values of the inflaton, the upper bound on r is significantly larger, of order 0.01, for subplanckian values of the inflaton, and View the MathML source|dns/dlnk|≃0.006.

10.1016/j.physletb.2014.04.060http://repo.scoap3.org/api