Low-energy probes of small CMB amplitude in models of radiative Higgs
  mechanism
  The small CMB amplitude $A_s \simeq 10^{-9}$ (or, small temperature
fluctuation $\delta T/T \simeq 10^{-5}$) typically requires an unnaturally
small effective coupling of an inflaton $\lambda_\phi \sim 10^{-14}$. In
successful models, there usually is extra suppression of the amplitude, e.g. by
large-field inflaton with non-minimal coupling $\xi$, so that $\lambda_\phi$
can be much larger. But $\lambda_\phi$ and $\xi$ cannot be $\sim {\cal O}(1)$
simultaneously; the naturalness burden is shared between them. We show that the
absence of new physics signals at TeV scale may prefer a more natural size of
$\xi \lesssim {\cal O}(1-100)$ with $\lambda_\phi \lesssim {\cal
O}(10^{-4}-10^{-8})$, constraining larger $\xi$ with larger $\lambda_\phi$ more
strongly. This intriguing connection between low- and high-energy physics is
made in the scenarios with $U(1)_X$ where inflaton's renormalization running
also induces Coleman-Weinberg mechanism for the electroweak symmetry breaking.
We particularly work out the prospects of LHC 13 and 100 TeV $pp$ colliders for
probing the parameter space of the small CMB amplitude.
