On the correlation between the X-ray and gamma-ray emission in TeV
  blazars
  The observations of TeV blazars published recently show an unexpected
quadratic or even cubic correlation between the X-ray and gamma-ray emission. A
standard model of the synchrotron self-Compton emission of a compact source
inside a jet is not able to explain such a correlation. Therefore, we propose
an alternative scenario where the emission of at least two independent compact
components is observed at the same time.
  We compare two different models. The first model assumes the injection of
relativistic particles into a downstream region of a shock wave inside a jet
that creates the emitting source. The model precisely describes the evolution
of the particle energy spectrum inside the source and takes into account a
light-crossing time effect for the produced radiation. The second model assumes
an intrinsically constant emission of a homogeneous source that travels inside
the jet along a curved trajectory, where the activity is produced simply by
different values of the source's Doppler factor. To verify the two models we
use recentlu published observations of Mrk 421.
  Our simulations show that simultaneous radiation of at least two independent
sources, where the first source dominates the emission in the X-ray range and
the second source radiates strongly in the gamma-ray range, can explain the
observed correlations. However, the injection model provides inadequate results
because it gives different values for the correlation of the rise and decay of
a flare. This problem is negligible in the scenario that uses the Doppler
boosting effect. Therefore, this approach yields much better results.
