Initial (dotted) and final (solid) midplane Bernoulli parameters, Be, of two GRMHD accretion simulations. The Bernoulli parameter is measured in units of rest mass energy. The energetically unbound flow (blue) is the A0.0BtN10 model of McKinney et al. (2012). The energetically bound flow (black) is the ADAF/SANE model of Narayan et al. (2012). The unbound simulation reached t = 96   796M and the bound simulation reached t = 200   000M. In both cases, the final Be appears to depend on the initial Be.