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Sequential Methods for Coupled Geomechanics and Multiphase Flow

Sequential Methods for Coupled Geomechanics and Multiphase Flow

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122 CHAPTER 5. FIXED-STRAIN AND FIXED-STRESS SPLITS<br />

Note that the constant term of F α sn(γ), −b 2 , is negative, so one root is positive <strong>and</strong> the<br />

one is negative. The condition <strong>for</strong> linear stability is max(|γ|) ≤ 1, which is obtained <strong>for</strong><br />

F α sn(γ = 1) ≥ 0 <strong>and</strong> F α sn(γ = −1) ≥ 0. From Equation 5.14, we get<br />

F α sn(γ = 1) = kp∆t<br />

α2(1 − cos θ) ≥ 0 , (5.15)<br />

µh2 F α dr (γ = −1) = 2Kdr + (2α − 1)Kdr<br />

M<br />

kp∆t<br />

µh 2 2(1 − cos θ) − 2b2 ≥ 0. (5.16)<br />

Equation 5.15 is valid <strong>for</strong> all θ. Equation 5.16 is valid <strong>for</strong> all θ depending on the weight<br />

α, as follows:<br />

For 0.5 ≤ α ≤ 1 : τ = b2 M<br />

Kdr<br />

For 0 < α < 0.5 : τ = b2 M<br />

Kdr<br />

≤ 1 , (5.17)<br />

µh 2<br />

≤ 1 <strong>and</strong> ∆t ≤ ( Kdr<br />

M − b2 )<br />

. (5.18)<br />

2(1 − 2α)Kdrkp<br />

Equation 5.17 indicates that the stability of the fixed-strain split depends on the coupling<br />

strength only <strong>and</strong> is independent of time step size, when 0.5 ≤ α ≤ 1. In the case that<br />

0 < α < 0.5, we obtain an additional condition <strong>for</strong> stability with restriction on the time step<br />

size. Since one of the γ’s is negative, oscillation is anticipated even when the fixed-strain<br />

split is stable.<br />

Remark 5.1. For the backward Euler time discretization, α = 1, the characteristic equa-<br />

tion of the fixed-strain split (Equation 5.14) is identical to that of the drained split. Notice,<br />

however, that the fixed-strain split with the midpoint rule α = 0.5 is conditionally stable,<br />

even though the drained split with the midpoint rule is unconditionally unstable.<br />

5.2.2 Fixed-stress split<br />

The fixed-stress split freezes the variation of the total stress rate, which yields<br />

∆ε n = b<br />

(∆P<br />

Kdr<br />

n − ∆P n−1 ) + ∆ε n−1 . (5.19)

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