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