Cosmological constant, inflation and no-cloning theorem
  From the viewpoint of no-cloning theorem we postulate a relation between the current accelerated expansion of our universe and the inflationary expansion in the very early universe. It implies that the fate of our universe should be in a state with accelerated expansion. Quantitatively we find that the no-cloning theorem leads to a lower bound on the cosmological constant which is compatible with observations. 
Qing-Guo Huang and Feng-Li Lin
hep-th astro-ph.CO gr-qc hep-ph quant-ph