14-7 Bernoulli’s Equation#

Prompts

  • State Bernoulli’s equation. What does each term represent (pressure, kinetic, gravitational)?

  • For horizontal flow (\(y\) constant), how are pressure and speed related? Where is pressure higher—in a narrow or wide section?

  • Why does a water stream from a faucet “neck down” as it falls?

  • A hole is punched in a water tank at depth \(h\) below the surface. What is the exit speed of the water? (Torricelli’s result)

  • Bernoulli’s equation is energy conservation. What are the three forms of energy per unit volume?

Lecture Notes#

Overview#

  • Bernoulli’s equation: Conservation of total energy density for ideal fluid flow.

  • Three energy densities (per unit volume): (1) Pressure \(p\)—work per volume, potential to expand; (2) Kinetic \(\frac{1}{2}\rho v^2\); (3) Gravitational \(\rho g y\).

  • Key result: Higher speed → lower pressure (for horizontal flow).


Bernoulli’s equation#

For steady, incompressible, nonviscous flow along a tube of flow:

(32)#\[ p_1 + \frac{1}{2}\rho v_1^2 + \rho g y_1 = p_2 + \frac{1}{2}\rho v_2^2 + \rho g y_2 = \text{constant} \]

Term

Physical name

Energy density

Intuitive meaning

\(p\)

Static pressure

Pressure energy density

Work per volume; energy stored from compression; fluid’s potential to expand and do work

\(\frac{1}{2}\rho v^2\)

Dynamic pressure

Kinetic energy (KE) density

KE per unit volume from macroscopic ordered motion

\(\rho g y\)

Hydrostatic pressure

Gravitational potential energy (PE) density

PE per unit volume from height in gravity field (\(y\) upward)

Physical meaning: The sum of pressure, kinetic, and gravitational energy per unit volume is conserved along a streamline. Bernoulli’s equation is energy conservation for an ideal fluid.

Note

Fluid at rest: Set \(v_1 = v_2 = 0\). Then \(p_2 = p_1 + \rho g(y_1 - y_2)\)—we recover hydrostatic pressure Eq. (16).


Horizontal flow: speed and pressure#

If \(y\) is constant (horizontal tube):

(33)#\[ p + \frac{1}{2}\rho v^2 = \text{constant} \]

Higher speed → lower pressure. Where streamlines are close together (fast flow), pressure is low; where they spread (slow flow), pressure is high.

  • Force perspective: A fluid element entering a narrow section must accelerate (\(F = ma\)). That requires higher pressure behind than in front—so pressure is lower in the narrow, fast region.

  • Energy perspective: Pressure energy is converted into kinetic energy.


Applications#

Faucet stream: Water falling from a tap speeds up (\(v\) increases). By continuity \(Av = \text{constant}\), so \(A\) must decrease—the stream “necks down.”

Leaky tank (Torricelli): A hole at depth \(h\) below the water surface. Take point 1 at the surface (\(p_1 = p_0\), \(v_1 \approx 0\), \(y_1 = h\)) and point 2 at the hole (\(p_2 = p_0\), \(y_2 = 0\)). Bernoulli gives

(34)#\[ v = \sqrt{2gh} \]

Same as the speed of free fall from height \(h\).


Summary#

  • Bernoulli’s equation: \(p + \frac{1}{2}\rho v^2 + \rho g y = \text{constant}\) (energy conservation)

  • Horizontal flow: \(p + \frac{1}{2}\rho v^2 = \text{constant}\); faster → lower pressure

  • Torricelli: Exit speed from hole at depth \(h\) is \(v = \sqrt{2gh}\)