Uniqueness of Self-Similar Asymptotically Friedmann-Robertson-Walker   Spacetime in Brans-Dicke theory
  We investigate spherically symmetric self-similar solutions in Brans-Dicke theory. Assuming a perfect fluid with the equation of state $p=(\gamma-1)\mu (1 \le \gamma<2)$, we show that there are no non-trivial solutions which approach asymptotically to the flat Friedmann-Robertson-Walker spacetime if the energy density is positive. This result suggests that primordial black holes in Brans-Dicke theory cannot grow at the same rate as the size of the cosmological particle horizon. 
Hideki Maeda, Jun-ichirou Koga and Kei-ichi Maeda