6533b860fe1ef96bd12c3a2c
RESEARCH PRODUCT
Do current data prefer a nonminimally coupled inflaton?
Lotfi BoubekeurElena GiusarmaHéctor RamírezOlga Menasubject
PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFOS: Physical sciencesFísicaSigmaAstrophysics::Cosmology and Extragalactic AstrophysicsInflaton01 natural sciencesSpectral lineGeneral Relativity and Quantum Cosmologysymbols.namesake13. Climate action0103 physical sciencessymbolsPlanck010306 general physicsLagrangianAstrophysics - Cosmology and Nongalactic AstrophysicsScalar curvaturedescription
We examine the impact of a non-minimal coupling of the inflaton to the Ricci scalar, $\frac12 \xi R\phi^2$, on the inflationary predictions. Such a non-minimal coupling is expected to be present in the inflaton Lagrangian on fairly general grounds. As a case study, we focus on the simplest inflationary model governed by the potential $V\propto \phi^2$, using the latest combined 2015 analysis of Planck and BICEP2/Keck Array. We find that the presence of a coupling $\xi$ is favoured at a significance of $99\%$ CL, assuming that nature has chosen the potential $V\propto \phi^2$ to generate the primordial perturbations and a number of e-foldings $N=60$. Within the context of the same scenario, we find that the value of $\xi$ is different from zero at the $2\sigma$ level. When considering the cross-correlation polarization spectra from BICEP2/Keck Array and Planck, a value of $r=0.038_{-0.030}^{+0.039}$ is predicted in this particular non-minimally coupled scenario. Future cosmological observations may therefore test these values of $r$ and verify or falsify the non-minimally coupled model explored here.
year | journal | country | edition | language |
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2015-02-18 | Physical Review D |