For time-dependent irrotational flow with , constant mass density, and no body force, the Euler equations for an inviscid fluid integrate to
A time-dependent change of gauge in may set .
This is the unsteady potential-flow version of Bernoulli's principle, with a time-dependent potential gauge.
A spherical balloon feeding an inviscid uniform tube plug, with entrance excess pressure , satisfies and . Eliminating yields the displayed equation. Its first integral is . From rest at radius , ; integration gives , where . The ideal emptying time is . Independently prescribed initial flow changes and therefore this time.
For a slender tube of length supplied from a large reservoir with excess pressure , negligible gravity and entrance inertia, the Unsteady Bernoulli equation gives . A stationary initial liquid column has the displayed speed and volume flux for tube radius . The inertial term controls the early linear acceleration; the kinetic-energy term sets the terminal inviscid speed. This is a leading slender-tube model while the reservoir remains large and the tube full.
An inviscid uniform tube plug driven by entrance excess pressure obeys and . From rest, the first zero of occurs after a quarter harmonic period, independent of its initial volume. The maximum speed is proportional to that initial volume. Entrance losses, a reservoir kinetic head or independently prescribed initial flow change this ideal model.

Ancestors (5)

  1. Euler equations for an inviscid fluid
  2. Fluid mechanics
  3. Branches of physics
  4. Physics
  5. Home

Discussion (0) New discussion

There are no discussions about this article yet.

Articles by others on the same topic (0)

There are currently no matching articles.