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Physics · Chapter

Mechanical Properties of Fluids

This chapter explores the mechanics of fluids, which are substances that can flow, like liquids and gases. It is divided into two main parts: fluid statics and fluid dynamics. Fluid statics deals with fluids at rest, covering concepts like pressure, density, and how pressure varies with depth. You will learn to apply Pascal's law, which explains how hydraulic systems work, and Archimedes' principle, which governs buoyancy and why objects float or sink.

Fluid dynamics examines fluids in motion. It introduces the ideas of streamline and turbulent flow, and the principle of mass conservation through the equation of continuity. The central concept here is Bernoulli's principle, an energy conservation equation for flowing fluids that explains phenomena like the lift on an airplane wing. The chapter also covers properties of real fluids, including viscosity (internal friction) and surface tension (the cohesive force at a liquid's surface), leading to topics like Stokes' law, terminal velocity, and capillary action.

The application of Bernoulli's theorem to complex systems can be difficult, as can problems that combine fluid dynamics with buoyancy or other forces. A strong foundation in Newton's Laws of Motion and the Work-Energy theorem is necessary, as many problems require setting up and solving force or energy balance equations for fluids.

Formulas for Mechanical Properties of Fluids

Pressure Variation with Depth
P=P0+ρghP = P_0 + \rho g h P is pressure at depth h, P₀ is surface pressure, ρ is fluid density.
Buoyant Force (Archimedes' Principle)
FB=VsubρfgF_B = V_{sub} \rho_f g V_sub is the submerged volume of the object, ρ_f is the fluid density.
Equation of Continuity
A1v1=A2v2A_1 v_1 = A_2 v_2 For an incompressible fluid in steady flow; A is cross-sectional area, v is fluid speed.
Bernoulli's Equation
P+12ρv2+ρgh=constantP + \frac{1}{2}\rho v^2 + \rho g h = \text{constant} For an ideal fluid in streamline flow; P is pressure, v is speed, h is height.
Stokes' Law
Fv=6πηrvF_v = 6 \pi \eta r v Viscous drag force on a sphere of radius r moving at speed v in a fluid of viscosity η.
Terminal Velocity
vt=29r2(ρs−ρl)gηv_t = \frac{2}{9} \frac{r^2 (\rho_s - \rho_l) g}{\eta} Constant velocity of a sphere (density ρ_s) falling in a fluid (density ρ_l).
Excess Pressure in a Liquid Drop
ΔP=2TR\Delta P = \frac{2T}{R} ΔP is the pressure difference across the surface; T is surface tension, R is radius.
Excess Pressure in a Soap Bubble
ΔP=4TR\Delta P = \frac{4T}{R} A soap bubble has two liquid-air interfaces, hence the factor of 4.
Capillary Rise or Fall
h=2Tcos⁡θrρgh = \frac{2T \cos\theta}{r \rho g} h is the height, T is surface tension, θ is the angle of contact, r is the tube radius.

One of these questions, worked through

JEE Advanced 2015

Two spheres PP and QQ of equal radii have densities ρ1\rho_1 and ρ2\rho_2, respectively. The spheres are connected by a massless string and placed in liquids L1L_1 and L2L_2 of densities σ1\sigma_1 and σ2\sigma_2 and viscosities η1\eta_1 and η2\eta_2, respectively. They float in equilibrium with the sphere PP in L1L_1 and sphere QQ in L2L_2 and the string being taut (see figure). If sphere PP alone in L2L_2 has terminal velocity V‾P\overline{V}_P and QQ alone in L1L_1 has terminal velocity V‾Q\overline{V}_Q, then
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Or read the worked solution below. Jump to the steps ↓

Step 1: Analyze the equilibrium of the connected spheres.

Sphere PP of volume VV floats in liquid L1L_1, and sphere QQ of volume VV floats in liquid L2L_2. Since the string is taut, the tension TT acts downwards on PP and upwards on QQ.

For sphere PP in liquid L1L_1:

σ1Vg=ρ1Vg+T\sigma_1 V g = \rho_1 V g + T

For sphere QQ in liquid L2L_2:

σ2Vg+T=ρ2Vg\sigma_2 V g + T = \rho_2 V g

Step 2: Relate the densities using the tension.

Solve both equations for the tension TT.

T=(σ1−ρ1)Vg=(ρ2−σ2)VgT = (\sigma_1 - \rho_1) V g = (\rho_2 - \sigma_2) V g

Equating the terms gives:

σ1−ρ1=ρ2−σ2\sigma_1 - \rho_1 = \rho_2 - \sigma_2

Rearranging the terms yields:

ρ1−σ2=−(ρ2−σ1)\rho_1 - \sigma_2 = -(\rho_2 - \sigma_1)

Taking the absolute values:

∣ρ1−σ2∣=∣ρ2−σ1∣|\rho_1 - \sigma_2| = |\rho_2 - \sigma_1|

Step 3: Write the expressions for the terminal velocities.

The terminal velocity of a sphere of radius rr and density ρ\rho in a liquid of density σ\sigma and viscosity η\eta is given by Stokes' Law.

For sphere PP alone in liquid L2L_2:

V‾P=29r2g(ρ1−σ2)η2\overline{V}_P = \frac{2}{9}\frac{r^2 g(\rho_1 - \sigma_2)}{\eta_2}

For sphere QQ alone in liquid L1L_1:

V‾Q=29r2g(ρ2−σ1)η1\overline{V}_Q = \frac{2}{9}\frac{r^2 g(\rho_2 - \sigma_1)}{\eta_1}

Step 4: Find the ratio of the magnitudes of the terminal velocities.

Using the equality of the density differences ∣ρ1−σ2∣=∣ρ2−σ1∣|\rho_1 - \sigma_2| = |\rho_2 - \sigma_1|, we find the ratio of the speeds:

∣V‾P∣∣V‾Q∣=η1η2\frac{|\overline{V}_P|}{|\overline{V}_Q|} = \frac{\eta_1}{\eta_2}

Step 5: Determine the sign of the dot product of the velocities.

Since the density differences have opposite signs:

ρ1−σ2=−(ρ2−σ1)\rho_1 - \sigma_2 = -(\rho_2 - \sigma_1)

The terminal velocities V‾P\overline{V}_P and V‾Q\overline{V}_Q point in opposite directions. Thus, their dot product is negative:

V‾P⋅V‾Q<0\overline{V}_P \cdot \overline{V}_Q < 0

Answer: The correct relations are ∣V‾P∣∣V‾Q∣=η1η2\dfrac{|\overline{V}_P|}{|\overline{V}_Q|} = \dfrac{\eta_1}{\eta_2} and V‾P⋅V‾Q<0\overline{V}_P \cdot \overline{V}_Q < 0.

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