Well, it is definitely *not* "totally irrelevant to talk about pressure" when doing simulations in the NVT (canonical) or NVE (microcanonical) ensembles. Pressure, like temperature, volume, energy, numbers of particles, etc, is a thermodynamic property which is *always* defined for *any* system in equilibrium. These parameters characterize the thermodynamic state, regardless of the ensemble that you choose to describe the system in terms of statistical mechanics. And the microscopic counterparts of these thermodynamic parameters are defined in such a way that their ensemble average must necessarily equal the thermodynamic value, regardless of ensemble (although their fluctuations are ensemble-dependent, becoming asymptotically identical only for macroscopic systems).

In particular, the virial-based "instantaneous pressure" (call it P') computed in simulations has its ensemble average equal to the thermodynamic pressure P (check any good book on molecular simulation). But, as others already pointed out, this P' is well-known to show extremelly large fluctuations, meaning that its average computed from the simulation has usually a very large statistical spread. In other words, although the ensemble average of P' is strictly equal to P, its simulation average is a random variable that often shows large deviations from P (especially for short simulations). To get an idea of what is an acceptable error for the average of P', you may look at its distribution histogram in the NPT simulation.

As for the equilibration of the system, the only thing that matters is which termodynamic state you are aiming at and what is the best way to get there. For example, if you choose NVT but happen to start with a volume which is a bit too large (eg, because the parameterized model acquires a higher density than the true experimental value that you assumed when setting the box size), you may get into trouble because the system may then want to separate into two phases but, being unable to do so in a small simulation box, ends up in a weird metastable state (eg, if you take an amount of water into a syringe, seal the tip, and then further pull the piston, you will get an "empty" region that is actually filled with water vapor, because having only liquid water filling that volume at that temperature is not thermodynamically stable). So, it is usually a good idea equilibrate in NPT, because the system finds its proper density at some temperature and pressure, whose regions of interest you usually know for the system you are studying. Once a "good" volume is found for some relevant P and T values, you can do the same for the energy: use NVT and let the system find a "good" energy for that T value, moving then to NVE. So, if for some reason you really want to do a simulation in the NVE ensemble, the suggested sequential procedure NPT > NVT > NVE sounds reasonable to me. Actually, I have a simpler suggestion: just run an NPT simulation, look at the 2D distribution histogram of V and E values, choose one representative snapshot that is in the central region of that distribution, and use that snapshot to run NVE. In any case, unless you have some experimental indication of the material density (N/V) *and* of the energy density (E/V) of your system, which would be extremelly unusual, you will have to follow some kind of approach similar to this. Of course, we may also ask why you think you need an NVE simulation, but that is an entirely different question...

Best,
Antonio


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On Wed, 5 Nov 2014, Johnny Lu wrote:

Well... I finally have to accept that I really need NVE. Some forum posts
suggested to run NPT, then NVT, and finally NVE.

For ideal gas law, if we fix the number of molecules and the temperature,
then fixing the volume at different value means changing the pressure.
So, I guess pressure is still meaningful, if I have to decide the correct
volume to run the NVT simulation.

For a large number of ideal gas molecules, averages of all thermodynamic
variables should be defined, regardless of which three of them is fixed or
which ensemble do I choose to represent the state.
For a small number of molecules, the distribution of the thermodynamic
variables should still have a definition (so, the average and the
distribution of pressure is still meaningful).

For a protein simulation, it still has a partition function, and equation
of state.

I mainly want to know how much error in pressure (deviation from 1 bar) is
acceptable.

On Wed, Nov 5, 2014 at 2:35 PM, Téletchéa Stéphane <
[email protected]> wrote:

Le 04/11/2014 18:00, Johnny Lu a écrit :

 Hi.

If my NVT simulation of a protein in 30k molecules of water has a pressure
of 11 bar (error 0.5 bar from g_energy), will the dynamics (not
distribution of conformations) change enough that the mechanism inferred
from this simulation be significantly more unreliable than the mechanism
inferred from a 1 bar simulation? (Will the reviewers cut my paper into
ribbons?)

Thanks again.


Hi,

Considering only your "NVT" parameters for your simulation,
I would consider it totally irrelevant to talk about "pressure" where your
constrain the volume.
This value or any other one has not really a meaning in this situation,
and I seen
many variations in the pressure value in this microcanonical ensemble
without paying too much
attention on it.

In an "NPT" simulation, then you should be able to find back a normal 1
bar simulation I think.

Do you have any reason to do first an NPT simulation, and "then" an NVT
one?
I would personally let the system equilibrate in NVT, then swith to the
more natural NPT,
provided actual code and force fields are now good enough in this ensemble.

Best,

Stéphane

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