Observational Constraints on Interacting Dark Matter Model Without Dark
  Energy
  The interacting dark matter (IDM) scenario allows for the acceleration of the
Universe without Dark Energy. We constrain the IDM model by using the newly
revised observational data including $H(z)$ data and Union2 SNe Ia via the
Markov chain Monte Carlo method. When mimicking the $\Lambda$CDM model, we
obtain a more stringent upper limit to the effective annihilation term at
$\kappa C_1\approx 10^{-3.4}\rm{Gyr}^{-1}$, and a tighter lower limit to the
relevant mass of Dark Matter particles at $M_x\approx 10^{-8.6}\rm{Gev}$. When
mimicking the $w$CDM model, we find that the effective equation of state of IDM
is consistent with the concordance $\Lambda$CDM model and appears to be most
consistent with the effective phantom model with a constant EoS for which
$w<-1$.
