Abstract

In the simplest inflationary model V=12m2ϕ2V=\frac12 m^2ϕ^2, we provide a prediction accurate up to 1%1\% for the spectral index nsn_s and the tensor-to-scalar ratio rr assuming instantaneous reheating and a standard thermal history: ns=0.9668±0.0003n_s = 0.9668\pm0.0003 and r=0.131±0.001r=0.131\pm 0.001. This represents the simplest and most informative point in the (ns,r)(n_s,r) plane. The result is independent of the details of reheating (or preheating) provided the conversion to radiation is sufficiently fast. A slower reheating or a modified post-inflationary evolution push towards smaller nsn_s (and larger rr), so that our prediction corresponds to the maximum nsn_s (and minimum rr) for the quadratic potential. We also derive similar results for a general V∝ϕpV \propto ϕ^p potential.

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