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Two-phase flows with granular stress
T. Gallouet, P. Helluy, J.-M. Herard, J. Nussbaum
LATP MarseilleIRMA Strasbourg
EDF ChatouISL Saint-Louis
January 24, 2008
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Context
I flow of weakly compressible grains (powder, sand, etc.) insidea compressible gas;
I averaged model (the solid phase is represented by anequivalent continuous media);
I 2 densities, 2 velocities, 2 pressures, 1 volume fraction;
I relaxation approach to return to a 1 pressure model (classical:cf. bibliography);
I novelty: granular stress treated in a rigorous way;
I stable approximation;
I application.
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Hyperbolicity and stabilityHyperbolicityNumerical viscosity
A general granular flow modelTwo-pressure modelEntropyHyperbolicityGranular stressReduction: one pressure model
Numerical approximation: splitting methodConvection stepRelaxation stepNumerical applicationCombustion chamber
Conclusion
Biblio
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Hyperbolicity and stability
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Hyperbolicity
Consider w(x , t) ∈ R2 solution of
wt + Awx = 0,
A =
[0 ε1 0
], ε = ±1.
Space Fourier transform w(ξ, t) :=∫∞−∞ e−ixξw(x , t)dx .
w(ξ, t) = e−iξtAw(ξ, 0). (1)
I Hyperbolic case (ε = 1): the L2 norm of w(., t) is constant
I Elliptic case (ε = −1): the frequency ξ is amplified by a factore |ξ|t (unstable)
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Numerical viscosity
Classical approximations introduce a ”numerical viscosity”, whichcan be modelled by
wt + Awx − hswxx = 0.
h is the size of the cells, s = ρ(A) the spectral radius of A. Theamplification is now
w(ξ, t) = e−iξtA−hsξ2tw(ξ, 0). (2)
But in the elliptic case, the limit system when h→ 0 is stillunstable !Problem: many models in the two-phase flow community arenon-hyperbolic...
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A general granular flow model
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I flow of compressible grains (powder, sand, etc.) inside acompressible gas;
I averaged model;
I 2 densities, 2 velocities, 2 pressures, 1 volume fraction;
I relaxation approach to return to a 1 pressure model (classical:cf. bibliography);
I novelty: ”rigorous” granular stress (tramway);
I stable approximation;
I application.
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Two-pressure model
A gaz phase k = 1, a solid (powder) phase k = 27 unknowns: partial densities ρk , velocities uk , internal energies ek ,gas volume fraction α1.
Pressure law: pk = pk (ρk , ek ) = (γk − 1)ρkek − γkπk , γk > 1
Other definitions: mk = αkρk α2 = 1− α1 Ek = ek +u2
k
2
The balance of mass, momentum and energy reads
mk,t + (mkuk )x = 0,
(mkuk )t + (mku2k + αkpk )x − p1αk,x = 0,
(mkEk )t + ((mkEk + αkpk )uk )x + p1αk,t = 0,
αk,t + u2αk,x = ±P,
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Entropy
The phase entropies satisfy the following PDEs
T1ds1 = de1 −p1
ρ21
dρ1
T2ds2 = de2 −p2
ρ22
dρ2 −Θdα2
After some computations, we find the following entropy dissipationequation
(∑
mksk )t + (∑
mkuksk )x =P
T2(p1 + m2Θ− p2)
Natural choice to ensure positive dissipation
P =1
ε(p1 + m2Θ− p2), ε→ 0 + .
R := m2Θ is called the granular stress.
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HyperbolicityLet
Y = (α1, ρ1, u1, s1, ρ2, u2, s2)T .
In this set of variables the system becomes
Yt + B(Y )Yx = S(P),
B(Y ) =
u2ρ1(u1−u2)
α1u1 ρ1
c21
ρ1u1
p1,s1
ρ1
u1
u2 ρ2
p1−p2
m2
c22
ρ2u2
p2,s2
ρ2
u2
ck =
√γk (pk + πk )
ρk
The characteristic polynomial is
P(λ) = (u2−λ)2(u1−λ)(u1−c1−λ)(u1 +c1−λ)(u2−c2−λ)(u2 +c2−λ)
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Granular stress
How to choose the granular stress R = m2Θ ?
Θ = Θ(α2)⇒ Θ = 0
Thus a more general choice is necessary.Exemple: for a stiffened gas equation of state
p2 = (γ2 − 1)ρ2e2 − γ2π2 , γ2 > 1.
We suppose Θ = Θ(ρ2, α2). We find
Θ(ρ2, α2) = ργ2−12 θ(α2)
Particular choice
θ(α2) = λαγ2−12 ⇒ R = λmγ2
2 .
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Reduction: one pressure model
When ε→ 0+, formally, we end up with a standard one pressuremodel
p2 = p1 + m2Θ (3)
We can remove an equation (for example the volume fractionevolution) and we find a 6 equations system
Z = (ρ1, u1, s1, ρ2, u2, s2)T .
Zt + C (Z )Zx = 0.(4)
Let∆ = α1α2 + δ(α1ρ2a
22 + α2ρ1c
21 ), (5)
and
δ =α
1−1/γ2
2
λγ2ργ22
. (6)
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Then we find
The eigenvalues can be computed only numerically.We observe that when λ→ 0, the system is generally nothyperbolic.We observe also that when λ→∞, we recover hyperbolicity.
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Numerical approximation: splitting method
Approximation of the one-pressure model by the more generaltwo-pressure model.At the end of each time step, we have to return to the pressureequilibriumRelaxation approach.
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Convection stepLet
w = (α1,m1,m1u1,m1E1,m2,m2u2,m2E2)T
The system can be written
wt + f (w)x + G (w)wx = Σ(P).
In the first half step the source term is omitted. We use a standardRusanov scheme
w∗i − wni
∆t+
f ni+1/2 − f n
i−1/2
∆x+ G (wn
i )wn
i+1 − wni−1
2∆x= 0,
f ni+1/2 = f (wn
i ,wni+1) numerical conservative flux
f (a, b) =f (a) + f (b)
2− s
2(b − a)
For s large enough, the scheme is entropy dissipative. Typically, wetake
s = max(ρ(f ′(a)), ρ(f ′(b))
)
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Relaxation step
In the second half step, we have formally to solve
αk,t = ±P,
mk,t = uk,t = 0,
(mkek )t + p1αk,t = 0.
(7)
Because of mass and momentum conservation we have mk = m∗kand uk = u∗k . In each cell we have to compute (α1, p1, p2) fromthe previous state w∗
p2 = p1 + λmγ22 ,
m1e1 + m2e2 = m∗1e∗1 + m∗2e
∗2 ,
(m1e1 −m∗1e∗1 ) + p1(α1 − α∗1) = 0.
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After some manipulations, we have to solve
H(α2) = (π2 − π1)(α1 + (γ1 − 1)(α1 − α∗1))(α2 + (γ2 − 1)(α2 − α∗2))
+(λα2mγ22 − A2)(α1 + (γ1 − 1)(α1 − α∗1))
+A1(α2 + (γ2 − 1)(α2 − α∗2)) = 0
withwith Ak = α∗k (p∗k + πk ) > 0.
The solution is unique in the interval [0, 1− β1] with
β1 =γ1 − 1
γ1α∗1 (8)
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Numerical application
We have constructed an entropy dissipative approximation of anon-hyperbolic system !What happens numerically ?Consider a simple Riemann problem in the interval [−1/2, 1/2].γ1 = 1.0924 and γ2 = 1.0182. We compute the solution at timet = 0.0008. The CFL number is 0.9.Data:
(L) (R)ρ1 76.45430093 57.34072568u1 0 0p1 200× 105 150× 105
ρ2 836.1239718 358.8982226u2 0 0p2 200× 105 150× 105
α1 0.25 0.25
(9)
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Figure: Void fraction, 50 cells, no granular stress .
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Figure: Void fraction, 1000 cells, no granular stress .
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Figure: Void fraction, 10000 cells, no granular stress .
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Figure: Void fraction, 100000 cells, no granular stress .
Linearly unstable but non-linearly stable...
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Combustion chamber
We consider now a simplified gun. The right boundary of thecomputational domain is moving. We activate the granular stressand other source terms (chemical reaction and drag), which are allentropy dissipative. The instabilities would occur on much finergrids...
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Figure: Pressure evolution at the breech and the shot base during time.Comparison between the Gough and the relaxation model.
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Figure: Porosity at the final time. Relaxation model with granular stress.
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Figure: Velocities at the final time. Relaxation model with granularstress.
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Figure: Pressures at the final time. Relaxation model with granular stress.
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Figure: Density of the solid phase at the final time. Relaxation modelwith granular stress.
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Conclusion
I Good generalization of the one pressure models;
I Rigorous entropy dissipation and maximum principle on thevolume fraction;
I Stability for a finite relaxation time;
I The instability is (fortunately) preserved by the scheme forfast pressure equilibrium;
I The model can be used in practical configurations (the solidphase remains almost incompressible).
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Biblio
M. R. Baer and J. W. Nunziato.
A two phase mixture theory for the deflagration to detonation transition (ddt) in reactive granular materials.Int. J. for Multiphase Flow, 16(6):861–889, 1986.
Thierry Gallouet, Jean-Marc Herard, and Nicolas Seguin.
Numerical modeling of two-phase flows using the two-fluid two-pressure approach.Math. Models Methods Appl. Sci., 14(5):663–700, 2004.
P. S. Gough.
Modeling of two-phase flows in guns.AIAA, 66:176–196, 1979.
A. K. Kapila, R. Menikoff, J. B. Bdzil, S. F. Son, and D. S. Stewart.
Two-phase modeling of deflagration-to-detonation transition in granular materials: reduced equations.Physics of Fluids, 13(10):3002–3024, 2001.
Julien Nussbaum, Philippe Helluy, Jean-Marc Herard, and Alain Carriere.
Numerical simulations of gas-particle flows with combustion.Flow, Turbulence and Combustion, 76(4):403–417, 2006.
R. Saurel and R. Abgrall.
A simple method for compressible multifluid flows.SIAM Journal on Scientific Computing, 21(3):1115–1145, 1999.