Bernoulli’s Equation is a fundamental principle in fluid mechanics that describes the conservation of energy along a streamline for an ideal fluid.

It states that the total mechanical energy per unit volume remains constant in steady, incompressible, inviscid flow.

Equations

Basic Form

Where:

  • P = Static pressure
  • ρ = Fluid density
  • v = Flow velocity
  • g = Gravitational acceleration
  • h = Elevation head

Per unit mass (specific energy)

Head form (per unit weight)

Where:

    • H = Total head

With Energy Losses

Where = head loss due to Friction and minor losses

With Energy Addition

Where = head added by Pump

Energy Components

Static Pressure Energy

  • P/ρ: Pressure energy per unit mass
  • Energy due to fluid pressure at a point
  • Can do work by pushing against surfaces

Kinetic Energy

  • v²/2: Kinetic energy per unit mass
  • Energy due to fluid motion
  • Increases with velocity squared

Potential Energy

  • gh: Gravitational potential energy per unit mass
  • Energy due to elevation above reference level
  • Constant for horizontal flow

Assumptions & Limitations

Valid When:

  • Steady flow: No time-dependent changes
  • Incompressible fluid: Constant density (ρ)
  • Inviscid flow: No viscous losses
  • No energy addition/removal: No pumps, turbines, or heat transfer
  • Along a streamline: Energy balance applies to same fluid particle

Invalid When:

  • High-speed compressible flow (Mach > 0.3)
  • Significant viscous effects (Viscosity)
  • Unsteady flow conditions
  • Energy input/output devices present
  • Across streamlines in rotational flow