TY - JOUR

T1 - Sub-Planckian φ2 inflation in the Palatini formulation of gravity with an R2 term

AU - Lloyd-Stubbs, A.

AU - McDonald, J.

PY - 2020/6/16

Y1 - 2020/6/16

N2 - The simplest model that can produce inflation is a massive noninteracting scalar particle with potential V=m2φ2/2. However, φ2 chaotic inflation is inconsistent with the observed upper bound on the tensor-to-scalar ratio, r. Recently it has been shown that, in the context of the Palatini formalism of gravity with an R2 term, the φ2 potential can be consistent with the observed bound on r while retaining the successful prediction for the scalar spectral index, ns. Here we show that the Palatini φ2R2 inflation model can also solve the super-Planckian inflaton problem of φ2 chaotic inflation, and that the model can be consistent with Planck scale-suppressed potential corrections, as may arise from a complete quantum gravity theory. If α≳1012, where α is the coefficient of the R2 term, the inflaton in the Einstein frame, σ, remains sub-Planckian throughout inflation. In addition, if α≳1020, then the predictions of the model are unaffected by Planck-suppressed potential corrections in the case where there is a broken shift symmetry, and if α≳1032, then the predictions are unaffected by Planck-suppressed potential corrections in general. The value of r is generally small, with r≲10-5 for α≳1012. We calculate the maximum possible reheating temperature, TRmax, corresponding to instantaneous reheating, for the different regimes of α. We find that for α≈1032, TRmax is approximately 1010 GeV, with larger values of TRmax for smaller α. For the case of instantaneous reheating, we show that ns is in agreement with the 2018 Planck results to within 1-σ, with the exception of the α≈1032 case, which is close to the 2-σ lower bound. Following inflation, the inflaton condensate is likely to rapidly fragment, which makes it possible for reheating to occur via the Higgs portal due to inflaton annihilations within oscillons. This typically results in delayed reheating, which is disfavored by the observed value of ns. In contrast, reheating via inflaton decays to right-handed neutrinos can easily result in instantaneous reheating. We determine the scale of unitarity violation and show that, in general, unitarity is conserved during inflation, although the inflaton field is larger than the unitarity-violation scale. We conclude that the Palatini φ2R2 inflation model provides a completely consistent model of inflation which can be sub-Planckian and consistent with Planck scale-suppressed potential corrections, can reheat successfully, and conserves unitarity during inflation.

AB - The simplest model that can produce inflation is a massive noninteracting scalar particle with potential V=m2φ2/2. However, φ2 chaotic inflation is inconsistent with the observed upper bound on the tensor-to-scalar ratio, r. Recently it has been shown that, in the context of the Palatini formalism of gravity with an R2 term, the φ2 potential can be consistent with the observed bound on r while retaining the successful prediction for the scalar spectral index, ns. Here we show that the Palatini φ2R2 inflation model can also solve the super-Planckian inflaton problem of φ2 chaotic inflation, and that the model can be consistent with Planck scale-suppressed potential corrections, as may arise from a complete quantum gravity theory. If α≳1012, where α is the coefficient of the R2 term, the inflaton in the Einstein frame, σ, remains sub-Planckian throughout inflation. In addition, if α≳1020, then the predictions of the model are unaffected by Planck-suppressed potential corrections in the case where there is a broken shift symmetry, and if α≳1032, then the predictions are unaffected by Planck-suppressed potential corrections in general. The value of r is generally small, with r≲10-5 for α≳1012. We calculate the maximum possible reheating temperature, TRmax, corresponding to instantaneous reheating, for the different regimes of α. We find that for α≈1032, TRmax is approximately 1010 GeV, with larger values of TRmax for smaller α. For the case of instantaneous reheating, we show that ns is in agreement with the 2018 Planck results to within 1-σ, with the exception of the α≈1032 case, which is close to the 2-σ lower bound. Following inflation, the inflaton condensate is likely to rapidly fragment, which makes it possible for reheating to occur via the Higgs portal due to inflaton annihilations within oscillons. This typically results in delayed reheating, which is disfavored by the observed value of ns. In contrast, reheating via inflaton decays to right-handed neutrinos can easily result in instantaneous reheating. We determine the scale of unitarity violation and show that, in general, unitarity is conserved during inflation, although the inflaton field is larger than the unitarity-violation scale. We conclude that the Palatini φ2R2 inflation model provides a completely consistent model of inflation which can be sub-Planckian and consistent with Planck scale-suppressed potential corrections, can reheat successfully, and conserves unitarity during inflation.

U2 - 10.1103/PhysRevD.101.123515

DO - 10.1103/PhysRevD.101.123515

M3 - Journal article

VL - 101

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 12

M1 - 123515

ER -