Review of fluid properties
Pure fluids
Ideal cases
pV = nRT
pV = RT
The kinetic energy is stronger than the Van Der Waals forces
Andrew Curve (saturation curve)
Critical Point
Tcr
Subcooled Liquid
Saturated Liquid
2 phases
Saturated Liq + Vap
Vapor
Saturated Vapor
Isobar
Supercritical Fluids
Subcritical Fluids
Pcr
Review of fluid properties
Pure fluids
Ideal cases
pV = nRT
pV = RT
The kinetic energy is stronger than the Van Der Waals forces
Tcr
Saturated Liquid
Critical Point
Vapor
2 phases
Andrew Curve (saturation curve)
Subcooled Liquid
Isobar
Saturated Liq + Vap
Saturated Vapor
Supercritical Fluids
Pcr
Subcritical Fluids
Vapor phase
How to model the behavior of pure fluids, so how to calculate the dynamic properties? It depends where you are in the diagram:
T > 3Tcr, p < pcr ideal gas model pv = RT (Equation of State)
T < 3Tcr or p > pcr real gas (vapor) Z = v(p,T) / (RT/p) (compressibility factor)
The real gas effect increases if T is lower and p is higher.
Estimation of equation of state for real gases
- Tables and Diagrams with experimental data
- Best-Fit Function of experimental data
- General Equation of State, trying to model also the real gases
Ex: (p + n2a/v2)(V - nb) = nRuT (Van Der Waals)
a = measure of the average attraction force between molecules
b = volume occupied by the molecules
Fundamental relations
T ds = du - vdp
(dH = dU + pdV + Vdp)
T ds = du + pdv
For ideal gases: Cv = ∂U/∂T = dU/dT and Cv(T)
CP = Cv + R
R = Ru/MN
u(T) = u(Tref) + ∫TrefT Cv(T) dT = u(Tref) + Cv(T-Tref)
mean integral value: Cv = ∫TrefT Cv(T) dT/T - Tref
h(T) = h(Tref) + ∫TrefT CP(T) dT
Monoatomic Gases - Perfect Gases (Cv = const):
s(T,p) = s(Tref, pref) + CP lnT/Tref -R lnP/Pref
Biatomic or Triatomic Gases - Ideal Gases: we need to resolve the integrals dS = CP(T) dT/ T - v dp/T
Liquid phase
To have an accurate estimate of v, h, u, etc. is required to use Best-Fit Equations.
To have a fairly accurate estimate the General Equation of State is enough.
In a defined range of T and p, we can make the assumption of incompressible fluid:
v = const
C = const
transformation from closest saturation liquid point
because the properties of saturated liquid are available
dl = du + pdv + vdp
for ideal liquids: u = U (T)
hA = hC + ∫CA(dupdpvdp) = hC + v(pA-PC ) T = const v = const
hA = hB - ∫AB(dupdpvdp) = hB - C(TB-TA) v = const p = const
Mass balance equation
The fundamental principle is the "Principle of Conservation of Mass" by Lavoisier. It's valid only if particles move at a speed much lower than the speed of light.
The mass of particles contained in a material control volume Ω(t) remain constant during time.
dMΩ(t)/dt = 0
Material (Lagrangian) Control Volume: it follows the particles Ω(t)
Eulerian Control Volume: fixed in space, particles can cross it V
For t = t0 : Ω(t0) = V
∀t dMΩ(t)/dt = d/dt ∫Ω(t) ρ(x,t) dv = 0
∫Ω(t) (∂ρ/∂t) dv + ∫∂Ω(t) ρ V · η dA = 0
∫Ω(t0) = V (∂ρ/∂t) dv + ∫∂Ω(t0) = ∂V ρ V · η dA = 0
Reynolds Transport Theorem
∫V (∂ρ/∂t) dV + ∫Sin ρ V · η dA + ∫Sout ρ V · η dA + ∫SL ρ V · η dA
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