Equation of state

Encyclopedia : E : EQ : EQU : Equation of state

---

In physics and thermodynamics, an equation of state is a constitutive equation describing the state of matter under a given set of physical conditions. It provides a mathematical relationship between two or more state functions associated with the matter, such as its temperature, pressure, volume, or internal energy. Equations of state are useful in describing the properties of fluids, mixtures of fluids, solids, and even the interior of stars.

The most prominent use of an equation of state is to predict the state of gases and liquids. One of the simplest equations of state for this purpose is the ideal gas law, which is roughly accurate for gases at low pressures and high temperatures. However, this equation becomes increasingly inaccurate at higher pressures and lower temperatures, and fails to predict condensation from a gas to a liquid. Therefore, a number of much more accurate equations of state have been developed for gases and liquids. At present, there is no single equation of state that accurately predicts the properties of all substances under all conditions.

In addition to predicting the behavior of gases and liquids, there are also equations of state for predicting the volume of solids, including the transition of solids from one crystalline state to another. There are equations that model the interior of stars, including neutron stars. A related concept is the perfect fluid equation of state used in cosmology.

Examples of equations of state

In the following equations the variables are defined as follows, any consistent set of units can be used although SI units are preferred:

P = pressure

V = volume

n = number of moles of a substance

V_m = V/n = molar volume, the volume of 1 mole of gas or liquid

T = temperature (K)

R = ideal gas constant (8.314472 J/(mol·K))

Classical ideal gas law

The classical ideal gas law may be written:

[PV = nRT\,]

The ideal gas law may also be expressed as follows

[ P=\rho (\gamma-1) e\,]

where [\rho] is the density, [\gamma] the adiabatic index, and e the internal energy. This form is purely in terms of intensive quantities and is useful when simulating the Euler equations because it expresses the relationship between internal energy and other forms of energy (such as kinetic), thus allowing simulations to obey the First Law.

Van der Waals equation of state

The Van der Waals equation of state may be written:

[\left(P + \frac\right)\left(V_m-b\right) = RT], note that V_m is molar volume.

Where a, b and R are constants that depend on the specific material. They can be calculated from the critical properties as:

[a = 3P_c V_c^2]

[b = \frac]

Proposed in 1873, the van der Waals equation of state was one of the first to perform markedly better than the ideal gas law. In this landmark equation a is called the attraction parameter and b the repulsion parameter or the effective molecular volume. While the equation is definitely superior to the ideal gas law and does predict the formation of a liquid phase, the agreement with experimental data is limited for conditions where the liquid forms. While the van der Waals equation is commonly referenced in text-books and papers for historical reasons, it is now obsolete. Other modern equations of only slightly greater complexity are much more accurate.

Van der Waals equation may be considered as the ideal gas law, "improved" due to two independent reasons:

1. Molecules are thought as particles with volume, not material points. Thus V cannot be too little, less than some constant. So we get (V - b) instead of V.
2. While ideal gas molecules do not interact, we consider molecules attracting others within a distance of several molecules' radii. It makes no effect inside material, but surface molecules attract to inside. We see this as diminishing of pressure on the outer shell (which is used in the ideal gas law), so we write (P + something) instead of P. To evaluate this 'something', let's examine addition force acting on an element of gas surface. While force acting on each surface molecule is ~[\rho], the force acting on the whole element is ~[\rho^2]~[\frac]

The virial equation of state

[\frac = 1 + \frac + \frac + \frac + \dots]

[B = -V_c \,]

[C = \frac]

Although usually not the most convenient equation of state, the virial equation is important because it can be derived directly from statistical mechanics. If appropriate assumptions are made about the mathematical form of intermolecular forces, theoretical expressions can be developed for each of the coefficients. In this case B corresponds to interactions between pairs of molecules, C to triplets, and so on. Accuracy can be increased by codidering higher order terms

Redlich-Kwong equation of state

[P = \frac - \fracV_m\left(V_m+b\right)}]

[a = \frac}]

[b = \frac]

R = ideal gas constant (8.31451 J/(mol·K))

Introduced in 1949 the Redlich-Kwong equation of state was a considerable improvement over other equations of the time. It is still of interest primarily due to its relatively simple form. While superior to the van der Waals equation of state, it performs poorly with respect to the liquid phase and thus cannot be used for accurately calculating vapor-liquid equilibria. However, it can be used in conjunction with separate liquid-phase correlations for this purpose.

The Redlich-Kwong equation is adequate for calculation of gas phase properties when the ratio of the pressure to the critical pressure (reduced pressure) is less than about one-half of the ratio of the temperature to the critical temperature (reduced temperature).

The Soave equation of state

[P = \frac - \frac]

R = ideal gas constant (8.31451 J/(mol·K))

[a = \frac]

[b = \frac]

[\alpha = \left(1 + \left(0.48508 + 1.55171\omega - 0.15613\omega^2\right) \left(1-T_r^\right)\right)^2]

[T_r = \frac]

Where ω is the acentric factor for the species.

for hydrogen:

[\alpha = 1.202 \exp\left(-0.30288T_r\right)]

In 1972 Soave replaced the a/√(T) term of the Redlich-Kwong equation with a function α(T,ω) involving the temperature and the acentric factor. The α function was devised to fit the vapor pressure data of hydrocarbons and the equation does fairly well for these materials.

The Peng-Robinson equation of state

[P=\frac - \frac]

R = ideal gas constant (8.31451 J/(mol·K))

[a = \frac]

[b = \frac]

[\alpha = \left(1 + \left(0.37464 + 1.54226\omega - 0.26992\omega^2\right) \left(1-T_r^\right)\right)^2]

[T_r = \frac]

Where ω is the acentric factor for the species.

The Peng-Robinson equation was developed in 1976 in order to satisfy the following goals:

1. The parameters should be expressible in terms of the critical properties and the acentric factor.
2. The model should provide reasonable accuracy near the critical point, particularly for calculations of the Compressibility factor and liquid density.
3. The mixing rules should not employ more than a single binary interaction parameter, which should be independent of temperature pressure and composition.
4. The equation should be applicable to all calculations of all fluid properties in natural gas processes.

For the most part the Peng-Robinson equation exhibits performance similar to the Soave equation, although it is generally superior in predicting the liquid densities of many materials, especially nonpolar ones.

The BWRS equation of state

[P=\rho RT + \left(B_0 RT-A_0 - \frac + \frac - \frac\right) \rho^2 + \left(bRT-a-\frac\right) \rho^3 + \alpha\left(a+\frac\right) \rho^6 + \frac\left(1 + \gamma\rho^2\right)\exp\left(-\gamma\rho^2\right)]

ρ = the molar density

Values of the various parameters for 15 substances can be found in:

K.E. Starling, Fluid Properties for Light Petroleum Systems. Gulf Publishing Company (1973).

Elliott, Suresh, Donohue

The Elliott, Suresh, and Donohue (ESD) equation of state (EOS) was proposed in 1990. The equation seeks to correct a shortcoming in the Peng-Robinson EOS in that there was an inaccuracy in the van der Waals repulsive term. The EOS accounts for the effect of the shape of a non-polar molecule and can be extended to polymers with the addition of an extra term (not shown). The EOS itself was developed through modeling computer simulations and should capture the essential physics of the size, shape, and hydrogen bonding.

[\frac=Z=1+\frac-\frac]

Where:

c = a "`shape factor"'

[\eta=b\rho]

[q=1+1.90476(c-1)]

[Y=\exp(\frac)-1.0617]

Reference: Elliott & Lira, Introductory Chemical Engineering Thermodynamics, 1999, Prentice Hall.

Stiffened equation of state

When considering water under very high pressures (typical applications are underwater nuclear explosions, sonic shock lithotripsy, and sonoluminescence) the stiffened equation of state is often used:

[ p=\rho(\gamma-1)e-\gamma p^0 \,]

where [e] is the internal energy per unit mass, [\gamma] is an empirically determined constant typically taken to be about 6.1, and [p^0] is another constant, representing the molecular attraction between water molecules. The magnitude of the correction is about 2 gigapascals (20000 atmospheres).

The equation is stated in this form because the speed of sound in water is given by [c^2=\gamma(p+p^0)/\rho].

Thus water behaves as though it is an ideal gas that is already under about 20000 atmospheres (2 GPa) pressure, and explains why water is commonly assumed to be incompressible: when the external pressure changes from 1 atmosphere to 2 atmospheres (100 kPa to 200 kPa), the water behaves as an ideal gas would do when changing from 20001 to 20002 atmospheres (200.01 MPa to 201.02 MPa).

This equation mispredicts the specific heat capacity of water but few alternatives are available for severely nonisentropic processes such as strong shocks.

Ultrarelativistic equation of state

An ultrarelativistic fluid has equation of state

[p=c_s^2\mu]

where [p] is the pressure, [\mu] is the energy density, and [c_s] is a constant referred to as the sound speed.

Ideal Bose equation of state

The equation of state for an ideal Bose gas is

[PV_m=RT~\frac_(z)}\left(\frac\right)^\alpha]

where α is an exponent specific to the system (e.g. in the absence of a potential field, α=3/2), z is exp(μ/kT) where μ is the chemical potential, Li is the polylogarithm, ζ is the Riemann zeta function, and T_c is the critical temperature at which a Bose-Einstein condensate begins to form.

History

Boyle's Law was perhaps the first expression of an equation of state. In 1662 Robert Boyle, an Irishman, performed a series of experiments employing a J-shaped glass tube, which was sealed on one end. Mercury was added to the tube, trapping a fixed quantity of air in the short, sealed end of the tube. Then the volume of gas was carefully measured as additional mercury was added to the tube. The pressure of the gas could be determined by the difference between the mercury level in the short end of the tube and that in the long, open end. Through these experiments, Boyle noted that the gas volume varied inversely with the pressure. In mathematical form, this can be stated as:

PV = constant

The above relationship has also been attributed to Edme Mariotte and is sometimes referred to as Mariotte's law. However, Mariotte's work was not published until 1676.

Charles's law or

In 1787 the French physicist Jacques Charles found that oxygen, nitrogen, hydrogen, carbon dioxide, and air expand to the same extent over the same 80 kelvin interval. Later, in 1802, Joseph Louis Gay-Lussac published results of similar experiments, indicating a linear relationship between volume and temperature:

V₁/T₁ = V₂/T₂

The

In 1834 Émile Clapeyron combined Boyle's Law and Charles' law into the first statement of the ideal gas law. Initially the law was formulated as PV_m=R(T_C+267) (with temperature expressed in degrees Celsius). However, later work revealed that the number should actually be 273.2, and then the Celsius scale was defined with 0 °C = 273.15 K, giving:

PV_m=R(T_C+273.15)

See also

• Gas Laws

 

---

From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.

Search Titles

0

1

2

3

4

5

6

7

8

9

A

B

C

D

E

F

G

H

I

J

K

L

M

N

O

P

Q

R

S

T

U

V

W

X

Y

Z

?