Ideal Gas Material
Constitutive Laws
This MPM material models either an ideal gas or a non-ideal van der Waals gas. Note the MPM is not in ideal method for odeling gas dynamics. The main use of this material type is when combine gas material points interact with other material types. TO optimize such modeling, the gas pressure can be is tracked by one of two methods:
- Actual Pressure: Set reference pressure to [math]\displaystyle{ P_0 }[/math] and track total pressure, [math]\displaystyle{ P }[/math], on the each particle from gas laws.
- Gauge Pressure: Omitting reference pressure material property, P0, tells the calculation track a gauge pressure, [math]\displaystyle{ p = P - P_0 }[/math] where [math]\displaystyle{ P_0 }[/math] is the gauge pressure set to 1 atmosphere (= 0.101325 MPa), on each particle. In other words 1 atmosphere pressure is a new baseline that correspond to zero gauge pressure on the particle.
The "Actual Pressure" works best when modeling just an ideal gas. The "Gauge Pressure" method appears to work better when gas particles are interacting with other materials (all of which have zero stress under starting conditions).
Ideal Gas Law
The ideal gas law is:
[math]\displaystyle{ PV = nRT }[/math]
where P is pressure, V is volume, n is number of moles, R is the gas constant, and T is absolute temperture. By making use of a reference state, this equation is recast in a more convenient form for modeling as a hyperelastic material in MPM code. The resulting constitutive laws for pressure and gauge pressure are:
[math]\displaystyle{ P = P_0 {T\over T_0} {1\over J} \quad{\rm and}\quad p = P_0 \left({T\over T_0} {1\over J}-1\right) }[/math]
where J is determinant of the deformation tensor (J = V/V0). P0, T0, and V0 (the initial particle value) define a gas reference state. Note that P0 is always 1 atmosphere when using gauge pressure.
The pressure is stored in the normal stresses or σxx =σyy = σzz = -P (or -p). All shear stresses are zero. This material is equivalent to a hyperelastic material with strain energy function of
[math]\displaystyle{ P = -\frac{dW(J)}{dJ} \quad {\rm or}\quad W(J) = -P_0{T\over T_0} \ln J }[/math]
This energy function is equivalent to the energy per unit initial volume for isothermal compression or expansion of an ideal gas.
Non-Ideal van der Waals Gas
The van der Waals gas law is
[math]\displaystyle{ \left(P + {an^2\over V^2}\right)\left({V\over n}-b\right) = RT }[/math]
where a and b are van der Waals gas properties. Using reference state calculations to eliminate n, actual and gauge pressure constitutive laws can be written as:
[math]\displaystyle{ P = P_0'{T\over T_0}\left({1\over J-b'}\right) - {a'\over J^2} \quad{\rm and}\quad p = P_0'{T\over T_0}\left({1\over J-b'}\right) -\left(P_0 + {a'\over J^2}\right) }[/math]
where
[math]\displaystyle{ a' = \frac{a\rho_0^2}{M_g},\ b'=\frac{b\rho_0}{M_g},\ {\rm and}\ P_0'=(P_0+a')(1-b') }[/math]
Note that these laws revert to ideal gas law when [math]\displaystyle{ a'=b'=0 }[/math]. The constant [math]\displaystyle{ b' }[/math] can also be written as [math]\displaystyle{ b'=bn/V_0 }[/math] which is a dimension value that corresponds to fraction of the reference volume that is occupied by gas molecules (an ideal gas ignores volume of gas molecules).
Reference State
Gas material properties are set by defining a reference state with pressure, [math]\displaystyle{ P_0 }[/math], temperature, [math]\displaystyle{ T_0 }[/math], and initial particle volume, [math]\displaystyle{ V_0 }[/math]. When using gauge pressure method, [math]\displaystyle{ P_0 }[/math] is set to 1 atmosphere. The reference state is used eliminate number of moles in the gas law. For an ideal gas the analysis is easy:
[math]\displaystyle{ n = \frac{P_0V_0}{RT_0} }[/math]
Substitution into ideal gas law gives the constitutive laws used in code. The calculation is the same for a van der Waals gas but is more complicated (it needs to solve a cubic equation for [math]\displaystyle{ V_0/n }[/math]). The details are provided in the materials.pdf file in the technical notes with final laws given above
Dynamic mechanical modeling in MPM coding needs know the gas density in the initial particle configuration. It is given, in general, by
[math]\displaystyle{ \rho_0 = \frac{nM_g}{V_0} }[/math]
where [math]\displaystyle{ M_g }[/math] is molecular weight of the gas molecule. Using reference state calculations, this density for both ideal and van der Waals gas can be found from
[math]\displaystyle{ \rho_0 = {P_0' M_g\over R T_0} }[/math]
For example, air might have reference pressure of 1 atm = 0.101325 MPa, [math]\displaystyle{ M_g=28.97 }[/math] g/mol at room temperature T0=300K with R = 8.3144621 J/k/mol leading to [math]\displaystyle{ \rho_0=0.1176 }[/math] g/cm2. This calculation assumed an ideal gas (where [math]\displaystyle{ P_0'=P_0 }[/math]). Calculations for density of a van der Waals gas differ only slight from density found by ideal gas law calculations.
Isothermal and Adiabatic Modes
When using isothermal mode, this material models isothermal compression and expansion, which implies all work results in heating or cooling. The amount of heat generated is tracked in the particle's heat energy. The problem may include heat input (in thermal boundary conditions), which may cause temperature rises. In other words, this mode only means the gas itself will not cause temperature changes. An ideal gas is characterized buy no change in internal energy unless there is external external heating. A van der Waals gas, however, can change internal energy with a term proportional to [math]\displaystyle{ a' }[/math].
To model adiabatic compression and expansion, activate adiabatic mode. This mode will convert work to heat resulting in heating during compression or cooling during expansion. You need to enter heat capacity and enter thermal conductivity. The current implementation uses a temperature independent conductivity (which may change in the future). The calculations model both ideal gases and van der Waals gases.
Stability
Ideal and van der Waals gas particles are fairly stable, but can be made unstable by certain boundary conditions on constraining walls. If stability problems arise, try different boundary conditions. They also do not work well for irreversibale processes such as free expansion into empty space (although can come close if using a very small CFL factor). This material model is intended to always be bounded by stable pressure conditions.
Material Properties
The ideal gas properties are set with
| Property | Description | Units | Default |
|---|---|---|---|
| P0 | Reference pressure at reference temperature and reference density. When entered, this property must be a positive value greater than zero and the calculation track actual pressure. If this property is omitted, the reference pressure is set to 1 atmosphere and the code tracks gauge pressure. | pressure units | Omitted |
| T0 | Reference temperature | K | none |
| rho | Density at reference conditions. | density units | none |
| vdwa | Enter the van der Waals a property (setting this property sets code to use van der Waals gas law). The units are (length units)6(pressure units)/mole2 | (see descriptio) | none |
| vdwb | Enter the van der Waals b property (setting this property sets code to use van der Waals gas law). The units are (length units)3/mole | (see description) | none |
| Cv | Instead of heat capacity, this parameter determines if the gas is monatomic or diatomic. Enter 1 (or any number smaller than 1) for monatomic or 2 (or any number larger than 2) for diatomic. The resulting heat capacity is described below | none | 1 |
| (other) | Properties common to all materials | varies | varies |
When using gas particles, the stress free temperature must always be set to a desired temperature in Kelvin.
Heat Capacity and Thermal Expansion Coefficient
The material definitions for gases do not enter heat capacity or thermal expansion coefficient. Instead these properties are calculated from gas thermodynamics. A general results for heat capacity is
[math]\displaystyle{ C_v=\frac{nR}{(\gamma-1)\rho_0 V_0} }[/math]
where [math]\displaystyle{ V_0/n }[/math] can be eliminated by reference state calculations and [math]\displaystyle{ \gamma=5/3 }[/math] for a monoatomic gas and [math]\displaystyle{ \gamma=7/5 }[/math] for a diatomic case. Thus, the material properties only need to indicate if the gas monoatomic or diatomic, and that is done with the Cv material property.
Similarly, the volumetric thermal expansion coefficient can be explicitly calculated as
[math]\displaystyle{ \alpha_V = \frac{1}{T}\frac{\left(P+\frac{a'}{J^2}\right)(J-b')}{\left(JP-\frac{a'}{J}+\frac{2a'b'}{J^2}\right)} }[/math]
The details are in the materials.pdf technical notes. For an ideal gas, this result simplifies to [math]\displaystyle{ \alpha_V=1/T }[/math].
History Variables
None
Examples
Note that you must always set the stress free temperature when use ideal gas law for sample particles.
Material "air","Air","IdealGas" P0 0.101325 T0 300 rho 0.001176 Cv 2 Done StressFreeTemp 300