438 Shock stability in gas dynamics
the uniform stability condition here above is obviously always satisfied. There-
fore, we have the following.
Theorem 15.2 All Lax shocks are uniformly stable in ideal gases.
This result has been well-known since Majda’s work [125]. It was, nevertheless,
questioned, wrongly, very recently (see [42] for more details).
Weak shocks As noted by M´etivier in [133], the uniform stability condition
(15.2.16) is satisfied for shocks of small enough amplitude. As a matter of fact,
k tends to 2 and r tends to 1 when the amplitude of the shock goes to 0.
Isentropic case We claim that stability conditions for isentropic gas dynamics
are a byproduct of stability conditions for complete gas dynamics, because isen-
tropic stability conditions are merely obtained by suppressing the penultimate
row and column of ∆. This just amounts to setting Γ = 0, or equivalently
k = 2, in the complete stability conditions. Therefore, we see from (15.2.14) that
the one-dimensional condition reduces to 1 + M = 0, which is always satisfied.
Accordingly, the first inequality in the weak multidimensional stability condi-
tion (15.2.15) is trivially satisfied. And the uniform multidimensional stability
condition reduces to
M
2
( r − 1) < 1 , (15.2.24)
or equivalently
p − p
0
−vp
v
< 1 .
This condition holds true in particular for the γ-law p =cstv
−γ
with γ ≥ 1.
15.2.3 Kreiss symmetrizers
The explicit construction of Kreiss’ symmetrizers given in Chapter 14 for regular
Initial Boundary Value problems is easily generalized to the shock stability
problem.
To stay close to the notations of Chapter 12, we denote here U =(v, u,s)
the set of thermodynamic and kinematic dependent variables, and
U : R
d−1
× R
+
× R → R
d+2
× R
d+2
× R × R
d−1
(y, z, t) → ( U
−
(y, z, t),U
+
(y, z, t),∂
t
χ(y, t), ∇
y
χ(y, t))
the sought shock solution, where χ is the unknown front and U
±
=(v
±
, u
±
,s
±
)
correspond to the unknown states on either side (both defined on R
d−1
× R
+
× R
after a suitable change of variables, see Chapter 12). For X =(y,z,t,η,τ) ∈
R
d−1
× R
+
× R
d−1
× C, we denote by A
U
(X)the2(d +2)×2(d + 2) matrix
obtained, as in the abstract framework of Chapter 12, through the following
successive transformations of the Euler equations on both sides of the unknown
front: