Neha Patil (Editor)

Real gas

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Real gas

Real gases are non-hypothetical gases whose molecules occupy space and have interactions; consequently, they adhere to gas laws. To understand the behaviour of real gases, the following must be taken into account:

Contents

  • compressibility effects;
  • variable specific heat capacity;
  • van der Waals forces;
  • non-equilibrium thermodynamic effects;
  • issues with molecular dissociation and elementary reactions with variable composition

    • For most applications, such a detailed analysis is unnecessary, and the ideal gas approximation can be used with reasonable accuracy. On the other hand, real-gas models have to be used near the condensation point of gases, near critical points, at very high pressures, to explain the Joule–Thomson effect and in other less usual cases. The deviation from ideality can be described by the compressibility factor Z.

    Van der Waals model

    Real gases are often modeled by taking into account their molar weight and molar volume

    R T = ( p + a V m 2 ) ( V m − b )

    or alternatively:

    p = R T V m − b − a V m 2

    Where p is the pressure, T is the temperature, R the ideal gas constant, and Vm the molar volume. a and b are parameters that are determined empirically for each gas, but are sometimes estimated from their critical temperature (Tc) and critical pressure (pc) using these relations:

    a = 27 R 2 T c 2 64 p c b = R T c 8 p c

    With the reduced properties   p r = p p c   ,   V r = V m V m,c   ,   T r = T T c the equation can be written in the reduced form:

    p r = 8 3 T r V r − 1 3 − 3 V r 2

    Redlich–Kwong model

    The Redlich–Kwong equation is another two-parameter equation that is used to model real gases. It is almost always more accurate than the van der Waals equation, and often more accurate than some equations with more than two parameters. The equation is

    R T = ( p + a T V m ( V m + b ) ) ( V m − b )

    or alternatively:

    p = R T V m − b − a T V m ( V m + b )

    where a and b two empirical parameters that are not the same parameters as in the van der Waals equation. These parameters can be determined:

    a = 0.42748 R 2 T c 5 / 2 p c b = 0.08664 R T c p c

    Using   p r = p p c   ,   V r = V m V m,c   ,   T r = T T c the equation of state can be written in the reduced form:

    p r = 3 T r V r − b ′ − 1 b ′ T r V r ( V r + b ′ ) with b ′ = 2 3 − 1 ≈ 0.26

    Berthelot and modified Berthelot model

    The Berthelot equation (named after D. Berthelot) is very rarely used,

    p = R T V m − b − a T V m 2

    but the modified version is somewhat more accurate

    p = R T V m [ 1 + 9 p / p c 128 T / T c ( 1 − 6 ( T / T c ) 2 ) ]

    Dieterici model

    This model (named after C. Dieterici) fell out of usage in recent years

    p = R T V m − b ⋅ exp ⁡ ( − a V m R T )

    with parameters a,b and exp ⁡ ( − a V m R T ) = e − a V m R T = 1 − a V m R T + …

    Clausius model

    The Clausius equation (named after Rudolf Clausius) is a very simple three-parameter equation used to model gases.

    R T = ( p + a T ( V m + c ) 2 ) ( V m − b )

    or alternatively:

    p = R T V m − b − a T ( V m + c ) 2

    where

    a = 27 R 2 T c 3 64 p c

    b = V c − R T c 4 p c

    c = 3 R T c 8 p c − V c

    where Vc is critical volume.

    Virial model

    The Virial equation derives from a perturbative treatment of statistical mechanics.

    p V m = R T [ 1 + B ( T ) V m + C ( T ) V m 2 + D ( T ) V m 3 + . . . ]

    or alternatively

    p V m = R T [ 1 + B ′ ( T ) p + C ′ ( T ) p 2 + D ′ ( T ) p 3 . . . ]

    where A, B, C, A′, B′, and C′ are temperature dependent constants.

    Peng–Robinson model

    Peng–Robinson equation of state (named after D.-Y. Peng and D. B. Robinson) has the interesting property being useful in modeling some liquids as well as real gases.

    p = R T V m − b − a ( T ) V m ( V m + b ) + b ( V m − b )

    Wohl model

    The Wohl equation (named after A. Wohl) is formulated in terms of critical values, making it useful when real gas constants are not available, but it cannot be used for high densities, as for example the critical isotherm shows a drastic decrease of pressure when the volume is contracted beyond the critical volume.

    p = R T V m − b − a T V m ( V m − b ) + c T 2 V m 3

    or: ( p − c T 2 V m 3 ) ( V m − b ) = R T − a T V m

    or alternatively:

    R T = ( p + a T V m ( V m − b ) − c T 2 V m 3 ) ( V m − b )

    where

    a = 6 p c T c V m,c 2

    b = V m,c 4   with   V m,c = 4 15 R T c p c

    c = 4 p c T c 2 V m,c 3 , where   V m,c   ,   p c   ,   T c   are (respectively) the molar volume, the pressure and the temperature at the critical point.


    And with the reduced properties   p r = p p c   ,   V r = V m V m,c   ,   T r = T T c one can write the first equation in the reduced form:

    p r = 15 4 T r V r − 1 4 − 6 T r V r ( V r − 1 4 ) + 4 T r 2 V r 3

    This equation is based on five experimentally determined constants. It is expressed as

    p = R T v 2 ( 1 − c v T 3 ) ( v + B ) − A v 2

    where

    A = A 0 ( 1 − a v ) B = B 0 ( 1 − b v )

    This equation is known to be reasonably accurate for densities up to about 0.8 ρcr, where ρcr is the density of the substance at its critical point. The constants appearing in the above equation are available in following table when p is in kPa, v is in m 3 k mol , T is in K and R=8.314 kPa ⋅ m 3 k mol ⋅ K

    Benedict–Webb–Rubin model

    The BWR equation, sometimes referred to as the BWRS equation,

    p = R T d + d 2 ( R T ( B + b d ) − ( A + a d − a α d 4 ) − 1 T 2 [ C − c d ( 1 + γ d 2 ) exp ⁡ ( − γ d 2 ) ] )

    where d is the molar density and where a, b, c, A, B, C, α, and γ are empirical constants. Note that the γ constant is a derivative of constant α and therefore almost identical to 1.

    References

    Real gas Wikipedia
    (Text) CC BY-SA