Sunyaev-Zel'dovich anisotropy due to Primordial black holes
  We investigate the Sunyaev-Zel'dovich (SZ) effect caused by primordial black
holes (PBHs) on the cosmic microwave background (CMB) temperature fluctuations.
The gas accreting on a PBH heats up by the release of the gravitational energy.
As a result, the heated gas in the vicinity of the PBH emits the UV and X-ray
photons. These photons can ionize and heat the intergalactic medium (IGM)
around the PBH. Assuming the simple model of these emitting photons, we compute
the profiles of the IGM ionization fraction and temperature around a PBH. Using
these profiles, we evaluate the Compton $y$-parameter created by the IGM gas
around a PBH. Finally, we estimate the CMB temperature angular power spectrum
due to the PBH SZ effect in our model. We show that the SZ temperature
anisotropy due to the PBHs has the flat angular power spectrum on small scale,
$l\leq2000$ and could dominate the primordial temperature spectrum on smaller
scales than the Silk scale. This flat spectrum extends to the scale of the
ionized region by the PBH emission. We also discuss the impact of the
small-scale CMB measurement on the PBH abundance based on our results.
