Loterre: Astronomie: Euler equation

mathematical technique > mathematical analysis > differential equation > partial differential equation > Euler equation

Euler equation

In fluid dynamics, the Euler equations are a set of quasilinear partial differential equations governing adiabatic and inviscid flow. They are named after Leonhard Euler. In particular, they correspond to the Navier–Stokes equations with zero viscosity and zero thermal conductivity. The Euler equations can be applied to incompressible or compressible flow. The incompressible Euler equations consist of Cauchy equations for conservation of mass and balance of momentum, together with the incompressibility condition that the flow velocity is a solenoidal field. The compressible Euler equations consist of equations for conservation of mass, balance of momentum, and balance of energy, together with a suitable constitutive equation for the specific energy density of the fluid. Historically, only the equations of conservation of mass and balance of momentum were derived by Euler. However, fluid dynamics literature often refers to the full set of the compressible Euler equations – including the energy equation – as "the compressible Euler equations". (Wikipedia, The Free Encyclopedia, https://en.wikipedia.org/wiki/Euler_equations_(fluid_dynamics))

http://data.loterre.fr/ark:/67375/MDL-JXQJXC0H-L

RDF/XML TURTLE JSON-LD Dernière modif. 24/04/2023

LOTERRE