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Pressure-Equilibrium Preserving Method

Updated 11 December 2025
  • Pressure-Equilibrium Preserving Method is a discretization approach that maintains uniform pressure and velocity while allowing variable density.
  • It employs techniques like harmonic mean flux construction and equilibrium projection to enforce pressure and velocity invariance down to machine precision.
  • The method prevents nonphysical pressure oscillations at interfaces, enhancing simulation stability in low-Mach and multi-material flow regimes.

A pressure-equilibrium preserving method is a numerical discretization for the Euler or related compressible flow equations that guarantees discrete preservation of pressure equilibrium states—i.e., solutions in which velocity and pressure are constant or satisfy an equilibrium constraint, while other variables (such as density or species concentrations) may have strong spatial variation. These methods are critical in avoiding nonphysical “pressure oscillations” or “pressure blips” at contact interfaces, material boundaries, or flows with large density ratios, particularly in low-Mach or multi-material regimes. Pressure-equilibrium preservation (PEP) is established through careful design of fluxes, reconstruction operators, or source-term discretizations that enforce the invariance of pressure and velocity equilibria in the fully discrete update, typically down to machine precision.

1. Mathematical Criteria for Pressure-Equilibrium Preservation

The core requirement for PEP is that if the initial numerical solution satisfies a pressure (and possibly velocity) equilibrium condition, then the discretization should ensure that pressure and velocity remain invariant under the evolution equations, regardless of density, composition, or other advected scalars. For compressible Euler systems, a prototypical pressure equilibrium state satisfies

u(x)U,p(x)P,ρ(x)  arbitrary.u(x) \equiv U, \qquad p(x) \equiv P, \qquad \rho(x) \;\text{arbitrary}.

For a scheme to be PEP, the update of the pressure (either as a conservative variable, a primary state variable, or via the equation of state) must yield tpn=0\partial_t p_n = 0 at every node/cell if pnPp_n \equiv P and unUu_n \equiv U at the previous time, for arbitrary local density (Michele et al., 3 Jul 2024).

Formally, the semi-discrete update should yield, for all cells or nodes nn,

ddtpn=0,ddtun=0if initialized in pressure- and velocity-equilibrium.\frac{d}{dt} p_n = 0, \quad \frac{d}{dt} u_n = 0 \quad \text{if initialized in pressure- and velocity-equilibrium.}

The specifics of these constraints depend on whether the update uses the conservative variables (ρ,ρu,ρE)(\rho, \rho u, \rho E), the pressure evolution form, or an alternative variable projection.

2. Design Mechanisms in Modern Schemes

2.1 Flux Construction

Pressure-equilibrium preservation is tightly linked to the structure of the flux functions in finite volume (FV), finite difference (FD), or discontinuous Galerkin (DG) methods. Classical schemes may fail to preserve pressure equilibrium due to the separate interpolation of primitive or conservative variables, causing arithmetic-mean inconsistencies (e.g., in the energy flux) and violation of the algebraic linkage imposed by the equation of state. A rigorous algebraic criterion for PEP at the flux level states that, for ideal gases and second-order central or split forms, the energy flux should interpolate the density by harmonic mean rather than arithmetic mean to fulfill

ρ~ρ1~=1,\widetilde \rho \cdot \widetilde{\rho^{-1}} = 1,

for all face averages between adjacent cells. For instance, the energy flux may be written as

FρE=ρHeu+,ρH=2ρLρRρL+ρR,e=eL+eR2,F_{\rho E}^* = \rho_H \overline{e} \overline{u} + \cdots, \qquad \rho_H = \frac{2 \rho_L \rho_R}{\rho_L + \rho_R}, \quad \overline{e} = \frac{e_L + e_R}{2},

where LL, RR denote left/right states at the face (Michele et al., 3 Jul 2024). This minimal modification ensures discrete preservation of pressure at all time steps.

2.2 Equilibrium-Projection and Pressure-Based Formulations

Alternative methodologies use equilibrium projection or pressure-based formulations. For DG schemes, one approach is to reconstruct or project the state vector onto equilibrium manifolds characterized by constant pressure (and possibly velocity), computing face fluxes in terms of these projected states (Ching et al., 2022, Ching et al., 21 Jan 2025). For example, one can define a pressure-projected state vector y~\tilde{y} by:

y~(y,p~)=(ρv,ρu~(C,p~)+12ρv2,C),\tilde{y}(y, \tilde{p}) = (\rho v, \rho \tilde{u}(C, \tilde{p}) + \frac{1}{2} \rho v^2, C),

where u~(C,p~)\tilde{u}(C, \tilde{p}) is chosen to ensure the pressure is equal to the polynomial projection p~\tilde{p} in each cell (Ching et al., 2022).

A related strategy replaces the total energy equation with a pressure evolution equation, directly evolving PP with a DG method and supplementing with energy correction terms for semidiscrete conservation (Ching et al., 21 Jan 2025).

2.3 Source Term Discretization in Balance Laws

For systems with nontrivial source terms (e.g., Euler–gravity, shallow water with topography), equilibrium preservation hinges on discretizing source terms and flux gradients in a manner that exactly cancels at hydrostatic or other equilibrium solutions. This is often realized by:

  • Rewriting the source terms using known equilibrium identities (e.g., replacing ρϕx-\rho \phi_x by (ρ/ρe)xpe-(\rho/\rho^e)\partial_x p^e).
  • Using entropy-conservative or equilibrium-consistent flux differences for spatial derivatives.
  • Carefully constructing nodal or cellwise source terms to match the discretized pressure gradients, ensuring that for any interpolant of the equilibrium state, the discrete residual vanishes (Liu et al., 1 Mar 2025, Zhang et al., 2 Feb 2024, Fan et al., 17 Jul 2025).

3. Algorithmic Structures and Implementation

Several algorithmic structures for PEP can be identified:

Methodology Key Discrete Mechanism Applicability
Harmonic-mean-based FV/FD fluxes Facewise harmonic-mean for ρ\rho in energy flux Compressible Euler (ideal gas)
Pressure-projection at faces Project local state to fixed pp, reconstruct uu Multicomponent, real fluids
Pressure evolution DG Replace EE-update by PP-update, correct energy Multicomponent, arbitrary EOS
Well-balanced nodal DG Entropy-conservative fluxes, equilibrium-based src Gravity/coupled source systems
Equilibrium-variable projection Approximate DG space in equilibrium variables VV Euler, shallow water, Ripa
EC-WENO / EC-MRWENO reconstructions Unified weights ensure (v,p)(v,p) const in interface Cut-cell, multi-material flow

In most cases, such mechanisms can be implemented as modular modifications of the flux evaluation or state-reconstruction routines in existing solvers, without the need for a change in mesh, time stepping, or limiter subroutines (Michele et al., 3 Jul 2024, Cai et al., 26 Jul 2025).

4. Theoretical Properties and Well-Balancedness

The PEP property is closely related to the broader concept of well-balancedness—exact preservation of nontrivial equilibria (steady, possibly nonzero-velocity, or nonuniform pressure states) in balance laws.

  • For the Euler–gravity system, well-balanced nodal DG achieves machine-precision preservation of hydrostatic equilibrium for any prescribed profile, provided a careful equilibrium-based discretization of both fluxes and sources is applied (Liu et al., 1 Mar 2025).
  • In DG schemes for general hyperbolic balance laws, constructing the polynomial approximation space in terms of equilibrium variables (e.g., V=(K,m,ε)V=(K, m, \varepsilon), with K=p/ργK=p/\rho^\gamma) and using hydrostatic reconstruction at cell faces guarantees that the discrete scheme remains at equilibrium when so initialized (Zhang et al., 2 Feb 2024).
  • Pressure-equilibrium preservation is ensured in multi-material sharp-interface methods even under geometric uncertainties by advancing geometric moments and using equilibrium-compatible reconstructions (Cai et al., 26 Jul 2025).

The discrete well-balanced property has been proven for a variety of systems and methods, including arbitrary-order DG for both hydrostatic and moving equilibria (Zhang et al., 2 Feb 2024, Fan et al., 17 Jul 2025), and for cut-cell methods with moving interfaces (Cai et al., 26 Jul 2025).

5. Practical Implications, Limitations, and Extensions

PEP methods have significant implications for accuracy, robustness, and stability:

Limitations include:

  • For real-gas, multi-component, or nonideal EOS, the construction of the dual mean in the flux or equilibrium-projection procedure must be carefully adapted (DeGrendele et al., 4 Dec 2025). The harmonic mean for density suffices only for ideal gases.
  • For conservative versus pressure-based forms, the latter may require correction terms to recover strict global conservation, especially at the fully discrete level (Ching et al., 21 Jan 2025).
  • Shock capturing and nonlinear stability are not automatically guaranteed by PEP alone; appropriate Riemann solvers or limiters are still necessary in the presence of strong discontinuities (Michele et al., 3 Jul 2024).

Extensions include pressure-robustness in incompressible Stokes/VEM contexts, where using divergence-preserving reconstruction operators in test and right-hand sides eliminates velocity error dependence on irrotational forces and achieves true pressure-independence (Zhao et al., 2020, Frerichs et al., 2020).

6. Impact and Representative Applications

Pressure-equilibrium preserving methods have been deployed in a wide spectrum of contexts, including:

Numerical validation demonstrates that PEP methods prevent the build-up of artificial pressure oscillations and preserve equilibrium in challenging test cases across a variety of applications and mesh types, offering both machine-precision equilibrium and competitive—often optimal—convergence rates away from interfaces or discontinuous source features.

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