Deear mister Ben,
     
    I don't know if your mail is serious, however I find your system very 
interesting.  Personally we think you mail might be joke, however I will do 
besst I can do helping you. My professor had once similar good idea. We are 
currently implementing relativistic equations of motion (lorentz 
transformations) for gromacs 5.0. 
    One could actually very interestingly study absortion of protein on black 
whole surface and calculate free energies.  
    On other next interesting thing,  my professor also expect that photo 
driven processes in protein as studied here:
     
    G. Groenhof, L.V. Schaefer, M. Boggio-Pasqua, H. Grubmueller and M.A. Robb.
    Arginine52 controls the photoisomerization process in photoactive yellow 
protein.
    Journal of Americal Chemical Society, 130 (2008), 3250-3251.
     
    Will be affected by presence of blackhole. Soon or later such kind event 
might become realistic and China should be the first to work on it. 
     
    However there is now experimental data to paramatrize such systems, 
especialy not under newtonian law.  A difficult with black holes is to 
intepretate experiments results, as there are  no distinction between blackhole 
of mater or anti-matter.
     
     
    First one thing:
     
    For proper solvent, currently me and my professor applied for grant for 
start working on the 'silent ether' forcefield, if interested you can contact 
us off list.  Although many people claim silent ether is not a realistic model, 
we will only use it as an emperical solvator to avoid complicated fysical 
effects.
     
    Second one next thing:
     
    For box to minimize the ammount of silent ether I think the best choice can 
be found here:
    Henk Bekker, Jur P. van den Berg, TSJERK A. WASSENAAR: Constructing a 
Near-Minimal-Volume Computational Box for Molecular Dynamics Simulations with 
Periodic Boundary Conditions. International Conference on Computational Science 
2003: 70-79
     
    Thrid one more next thing:
     
    For force field of black holes you should consider chose poper density, 
mass and  Schwarz-schild radius.
    But make sure mass stays in withinTolman-Oppenheimer-Volkoff limit.
     
    Fourth one final last thing:
     
   >Could two black wholes see each other if box too small?
     
    Shuch problem only occurs when using PME (threating "no hair" theorem). 
    For pressure virial law should still hold, with minor relativistic 
corrections.
     
    Other important next thing after last thing:
     
    Don't remove angular momentum each step,  as they form together with its 
mass an important classification for black hole. The silent ether added will 
prevent flying ice cube problems.
     
    For temperature be carefull to use older gromacs version (3.3), as the 
underestimate the proper temperature ensemble in system !!!!!!
     
    Good luck,
     
    greetings
     
    Jiang,
     
     
     
    roger han wrote:
   > Dear mister gromacs
   >
   > My professor interested in black wholes. How can I put a particle in a box 
and set mass to infinity? Which solvent is best choice and could there be 
problems with pressure? I'm also not sure about periodic boundaries. Could two 
black wholes see each other if box too small?
   >
   > Many thanks
   >
   > Ben
     
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