Search results for "Friedmann equations"

showing 2 items of 2 documents

Quantum corrections to inflation: the importance of RG-running and choosing the optimal RG-scale

2017

We demonstrate the importance of correctly implementing RG running and choosing the RG scale when calculating quantum corrections to inflaton dynamics. We show that such corrections are negligible for single-field inflation, in the sense of not altering the viable region in the ${n}_{s}\ensuremath{-}r$ plane, when imposing Planck constraints on ${A}_{s}$. Surprisingly, this also applies, in a nontrivial way, for an inflaton coupled to additional spectator degrees of freedom. The result relies on choosing the renormalization scale (pseudo-)optimally, thereby avoiding unphysical large logarithmic corrections to the Friedmann equations and large running of the couplings. We find that the viabl…

Physics beyond the Standard ModelScalar (mathematics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesClassical limitRenormalizationsymbols.namesakeGeneral Relativity and Quantum Cosmologyquantum correctionsHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanics0103 physical sciences010306 general physicsQuantumMathematical physicsPhysicsta114010308 nuclear & particles physicsFriedmann equationsInflatonRenormalization groupinflatonHigh Energy Physics - Phenomenologysymbols
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A model for the very early universe

2008

A model with N species of massless fermions interacting via (microscopic) gravitational torsion in de Sitter spacetime is investigated in the limit N->infinity. The U_V(N)*U_A(N) flavor symmetry is broken dynamically irrespective of the (positive) value of the induced four-fermion coupling. This model is equivalent to a theory with free but massive fermions fluctuating about the chiral condensate. When the fermions are integrated out in a way demonstrated long ago by Candelas and Raine, the associated gap equation together with the Friedmann equation predict that the Hubble parameter vanishes. Introducing a matter sector (subject to a finite gauge symmetry) as a source for subsequent cos…

High Energy Physics - TheoryChiral anomalyPhysicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeFriedmann equationsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermionMassless particleHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)De Sitter universesymbolsAxionGauge symmetryHubble's lawMathematical physicsJournal of High Energy Physics
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