The simplest model that can produce inflation is a massive noninteracting scalar particle with potential V = m(2)phi(2)/2. However, phi(2) 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 R-2 term, the phi(2) potential can be consistent with the observed bound on r while retaining the successful prediction for the scalar spectral index, n(s). Here we show that the Palatini phi R-2(2) inflation model can also solve the super-Planckian inflaton problem of phi(2) 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 alpha greater than or similar to 10(12), where a is the coefficient of the R-2 term, the inflaton in the Einstein frame, sigma, remains sub-Planckian throughout inflation. In addition, if alpha greater than or similar to 10(20), 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 alpha greater than or similar to 10(32), then the predictions are unaffected by Planck-suppressed potential corrections in general. The value of r is generally small, with r less than or similar to 10(-5) for alpha greater than or similar to 10(12). We calculate the maximum possible reheating temperature, T-Rmax, corresponding to instantaneous reheating, for the different regimes of alpha. We find that for alpha less than or similar to 10(32), T-Rmax, is approximately 10(10)( )GeV, with larger values of T-Rmax for smaller alpha. For the case of instantaneous reheating, we show that n(s) is in agreement with the 2018 Planck results to within 1-sigma, with the exception of the alpha similar or equal to 10(32) case, which is close to the 2-sigma 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 n(s). 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 phi R-2(2) 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.
