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Euler equations

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Euler equations
Euler equations
Jakob Emanuel Handmann · Public domain · source
NameEuler equations
FieldFluid dynamics; Continuum mechanics; Mathematical physics
Introduced1757
DiscovererLeonhard Euler
RelatedNavier–Stokes equations; Bernoulli principle; Euler–Lagrange equation

Euler equations

Introduction

The Euler equations are a system of hyperbolic partial differential equations governing inviscid fluid flow appearing in works by Leonhard Euler, used across hydrodynamics, aerodynamics, astrophysics, meteorology, oceanography and engineering. They describe conservation of mass, momentum and energy in an idealized continuum, forming a foundation for models in Isaac Newtonian mechanics, complementing results from Daniel Bernoulli and linking to variational principles from Joseph-Louis Lagrange and William Rowan Hamilton. The equations underpin theoretical studies in École Polytechnique-era mathematical physics and practical designs at institutions such as NASA, Boeing, Royal Netherlands Navy testing and US Navy modelling efforts.

Mathematical Formulation

In conservative form the Euler equations express balance laws for density ρ, momentum ρu and total energy E, connecting to thermodynamic closure via an equation of state from Ludwig Boltzmann or Rudolf Clausius and conservation principles associated with Noether's theorem. The system couples nonlinear advection terms similar to structures in the Burgers' equation and features characteristic waves analyzed using eigenvalue methods developed by Augustin-Louis Cauchy and Peter Gustav Lejeune Dirichlet. Boundary-value problems involving the Euler equations often reference canonical test cases from von Kármán and stability criteria studied by Andrey Kolmogorov and Ludwig Prandtl. Weak solutions and entropy conditions link to concepts advanced by Sofia Kovalevskaya and Richard Courant in the context of hyperbolic systems.

Physical Applications

Applications include shock-capturing in supersonic flight design by Kelly Johnson-era teams at Lockheed Martin, weather forecasting models employed at the European Centre for Medium-Range Weather Forecasts and storm surge modelling by NOAA. In astrophysical accretion and supernova simulations performed by groups at Caltech and Princeton University, the Euler equations couple to gravity treatments from Albert Einstein and radiation transport methods developed at Argonne National Laboratory. Industrial processes such as turbomachinery optimisation at General Electric and combustion modelling in research at MIT use Euler-based inviscid approximations alongside empirical corrections from Sir Frank Whittle-inspired jet propulsion studies.

Analytical Properties and Solutions

The Euler equations admit classical smooth solutions under conditions studied by Sergiu Klainerman and blow-up scenarios investigated by Jean-Yves Chemin and Terence Tao in modern analysis. Shock formation and rarefaction waves connect to work by Peter Lax on conservation laws and the theory of Riemann problems formalized by Bernhard Riemann; exact self-similar solutions often reference the Riemann solution families and similarity methods linked to Joseph Fourier techniques. Existence and uniqueness of weak entropy solutions draw on methods from Lax and compactness frameworks by Lars Hörmander and Luc Tartar, while stability analyses use tools from spectral theory credited to David Hilbert and John von Neumann.

Numerical Methods and Simulation

Computational approaches include finite volume schemes introduced by Rolf Harten and high-resolution shock-capturing methods by Philip Roe and Boris Glimm, with modern adaptations in Godunov-type solvers referencing work by Sergei K. Godunov. Discretization strategies draw on multigrid concepts by Lance Fortnow-era numerical analysts and adaptive mesh refinement pioneered by groups at University of Chicago and Lawrence Livermore National Laboratory. Large-eddy simulations and hybrid methods combine inviscid Euler solvers with turbulence models from Andrey Kolmogorov and turbulence closure concepts influenced by G. I. Taylor for industrial codes developed at Siemens and Rolls-Royce for jet engine design.

Historical Development and Contributors

The equations were first formulated by Leonhard Euler in the mid-18th century during correspondence with contemporaries in the Royal Society and the St. Petersburg Academy of Sciences, building on earlier hydraulic studies by Daniel Bernoulli and mathematical methods advanced by Brook Taylor. Subsequent rigorous analysis and conservation-law theory were advanced by Bernhard Riemann, Richard Courant and Kurt Friedrichs, while 20th-century developments in shock theory and numerical analysis were driven by Peter Lax, Sergei Godunov and Stanislaw Ulam-associated computation initiatives. Modern interdisciplinary contributions span researchers at Princeton Plasma Physics Laboratory, Los Alamos National Laboratory and academic groups at Cambridge University and ETH Zurich who continue to extend the mathematical, computational and applied frontiers of the Euler framework.

Category:Partial differential equations Category:Fluid dynamics Category:Mathematical physics