Pressure

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Pressure (p) is the force per unit area applied on a surface, in a direction perpendicular to that surface, i.e. the scalar part of the stress tensor under equilibrium/hydrostatic conditions.

Thermodynamics[edit]

In thermodynamics the pressure is given by

p=−∂A∂V|T,N=kBT∂lnQ∂V|T,N

where A is the Helmholtz energy function, V is the volume, kB is the Boltzmann constant, T is the temperature and Q(N,V,T) is the canonical ensemble partition function.

Units[edit]

The SI units for pressure are Pascals (Pa), 1 Pa being 1 N/m2, or 1 J/m3. Other frequently encountered units are bars and millibars (mbar); 1 mbar = 100 Pa = 1 hPa, 1 hectopascal. 1 bar is 105 Pa by definition. This is very close to the standard atmosphere (atm), approximately equal to typical air pressure at earth mean sea level: atm, standard atmosphere = 101325 Pa = 101.325 kPa = 1013.25 hPa = 1.01325 bar

Stress[edit]

The stress is given by

F=σijA

where F is the force, A is the area, and σij is the stress tensor, given by

σij≡[σxτxyτxzτyxσyτyzτzxτzyσz]

where where σx, σy, and σz are normal stresses, and τxy, τxz, τyx, τyz, τzx, and τzy are shear stresess.

Virial pressure[edit]

The virial pressure is commonly used to obtain the pressure from a general simulation. It is particularly well suited to molecular dynamics, since forces are evaluated and readily available. For pair interactions, one has (Eq. 2 in [1]):

p=kBTNV+1Vd∑i<jfijrij¯,

where p is the pressure, T is the temperature, V is the volume and kB is the Boltzmann constant. In this equation one can recognize an ideal gas contribution, and a second term due to the virial. The overline is an average, which would be a time average in molecular dynamics, or an ensemble average in Monte Carlo; d is the dimension of the system (3 in the "real" world). fij is the force on particle i exerted by particle j, and rij is the vector going from i to j: rij=rj−ri.

This relationship is readily obtained by writing the partition function in "reduced coordinates", i.e. x*=x/L, etc, then considering a "blow-up" of the system by changing the value of L. This would apply to a simple cubic system, but the same ideas can also be applied to obtain expressions for the stress tensor and the surface tension, and are also used in constant-pressure Monte Carlo.

If the interaction is central, the force is given by

fij=−rijrijf(rij),

where f(r) the force corresponding to the intermolecular potential Φ(r):

−∂Φ(r)/∂r.

For example, for the Lennard-Jones potential, f(r)=24ϵ(2(σ/r)12−(σ/r)6)/r. Hence, the expression reduces to

p=kBTNV+1Vd∑i<jf(rij)rij¯.

Notice that most realistic potentials are attractive at long ranges; hence the first correction to the ideal pressure will be a negative contribution: the second virial coefficient. On the other hand, contributions from purely repulsive potentials, such as hard spheres, are always positive.

Pressure equation[edit]

For particles acting through two-body central forces alone one may use the thermodynamic relation

p=−∂A∂V|T

Using this relation, along with the Helmholtz energy function and the canonical partition function, one arrives at the so-called pressure equation (also known as the virial equation):

p*=βpρ=pVNkBT=1−β23πρ∫0∞(dΦ(r)drr)g(r)r2dr

where β:=1/kBT, Φ(r) is a central potential and g(r) is the pair distribution function.

See also[edit]

References[edit]

Related reading