加载中…
We demonstrate that there are no scale-invariant one-loop corrections to the superhorizon tensor perturbations from small-scale (potentially enhanced) scalar perturbations, irrespective of the details of inflationary background time evolution. For this purpose we derive a soft tensor effective field theory at leading order in the gradient expansion by integrating out small-scale scalar fluctuations in a general time-dependent background over the Schwinger-Keldysh contour, i.e., we perform loop calculations in the soft limit of external momentum. The absence of scale-invariant corrections originates from the diffeomorphism invariance of general relativity and is therefore unavoidable.

生成讲解博客的中文版本

生成AI智能校验的中文版本