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A near-vacuum Euler state remains positive under symmetric HLL speeds

Example

Take γ=7/5, density ρ=10−8, pressure p=10−12, and velocities uL=−1/100, uR=1/100. The conserved states have mL,R=∓10−10 and EL,R=3×10−12. Choose the symmetric HLL speed a=11/500 at every face and Courant ratio ν=Δt/h=125/11. For the four-cell periodic data (UL,UL,UR,UR), one HLL forward-Euler update preserves positive density and pressure despite the very small initial values. The calculation illustrates a first-order positivity branch; it does not claim accuracy of the shock profile.

Facts & Assumptions

Given: The ideal-gas Euler flux and HLL update, with the parameters above. Verify the states, speed branch, CFL condition, and positivity after one update.

[F1]

Admissible states and pressure for one-dimensional ideal-gas Euler: p=(γ−1)(E−m2/(2ρ)) and c2=γp/ρ.

[F2]

Ideal-gas Euler states remain positive under Lax–Friedrichs flux splitting: if a≥∣u∣+c, then U±F(U)/a∈Gγ.

[F4]

First-order HLL updates are averages of adjacent half-cell fan averages: under 2νa≤1, the HLL update is the mean of adjacent half-cell fan averages.

[F5]

Symmetric HLL speeds preserve ideal-gas density and internal-energy positivity: the symmetric HLL branch with a≥∣u∣+c and 2νa≤1 preserves Gγ.

[F6]

First-order finite-volume update using supplied HLL speeds: Ui+=Ui−ν(F^i+1/2−F^i−1/2).

[F7]

HLL two-wave approximate flux: the symmetric middle-branch HLL flux is used at every interface, with equal-state data substituted into its displayed formula.

Verification

1.1givenF1algebra

The kinetic energy density is ρu2/2=5×10−13 and p/(γ−1)=5/2×10−12, so E=3×10−12. Hence [F1] gives the specified pressure and positive internal energy, so both states lie in Gγ.

2.1givenF1F2F5step 1.1algebra

Their sound speed satisfies c2=7/50000<(3/250)2, hence ∣u∣+c<1/100+3/250=11/500=a. Also νa=1/4, so 2νa=1/2≤1. The symmetric-speed hypotheses in [F2]–[F5] hold, with the positive admissibility verified in step 1.1.

3.1givenF1F2F3F4F6F7step 2.1algebra∎

At the discontinuity, substitution of SL=−a,SR=a into [F7] and the HLL intermediate-state formula of [F4] gives U∗=(UL+FL/a+UR−FR/a)/2. Both split states are in Gγ by [F2], so U∗∈Gγ by [F3]. At equal-state faces, the same middle-state formula gives U∗=UL or UR. Substituting the shared face fluxes in [F6], or equivalently using [F4], yields Ui+=(3/4)UL+(1/4)U∗ and Ui+1+=(3/4)UR+(1/4)U∗. Convexity keeps both states in Gγ, and [F1] gives positive density and pressure, using the CFL verification in step 2.1.

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