Basic Fluid Mechanics

Module 1

1.1 Fluid Properties
1.2 Types of Fluid flow
1.3 Conservation Law
1.4 Dimensional analysis
1.5 Losses of Pipes
1.1 Fluid Properties
Basic Fluid Properties
Density (ρ)

Mass per unit volume: ρ = m / V. Units: kg·m⁻³. Water (25°C) ≈ 1000 kg/m³, Air (25°C) ≈ 1.184 kg/m³.

Specific weight & specific gravity

Specific weight γ = ρ g (N/m³).
Specific gravity SG = ρ_fluid / ρ_water (dimensionless).

Viscosity (μ, ν)

Viscosity is internal resistance to shear. Dynamic μ relates shear stress to velocity gradient: τ = μ du/dy. Kinematic ν = μ/ρ. Liquids: μ ↓ with T; gases: μ ↑ with T.

Compressibility & Bulk Modulus

Bulk modulus K = −V dP/dV. Liquids have high K (low compressibility), gases low K. Speed of sound: a = √(K/ρ).

Vapor pressure & cavitation

Vapor pressure is the pressure at which liquid vaporizes. High vapor pressure → easier evaporation; important for cavitation in pumps and propellers.

Surface tension & capillarity

Surface tension σ causes liquids to minimize surface area; capillary rise formula:

h = (2 σ cos θ) / (ρ g r)

θ = contact angle, r = tube radius.

1.2 Types of Fluid flow
Fluid Flow
Newtonian Law of Viscosity
The Newtonian law of viscosity states that the shear stress between adjacent fluid layers is directly proportional to the velocity gradient (rate of shear strain). Formula: τ = μ (du/dy)
Non-Newtonian Fluids
  • Shear-Thinning: Paint, blood, ketchup
  • τ = k (du/dy)n, n < 1
  • Shear-Thickening: Cornflour mixture (oobleck)
  • τ = k (du/dy)n, n > 1
  • Bingham Plastic: Toothpaste
  • τ = τ₀ + μₚ (du/dy)
  • Thixotropic: Gels, yogurt
  • μ = μ(t)
  • Rheopectic: Gypsum paste
Newtonian vs Non-Newtonian Fluids
CategoryNewtonian FluidsNon-Newtonian Fluids
Nature / BehaviorViscosity remains constant, independent of shear rate.Viscosity changes with shear rate or time.
Mathematical Modelτ = μ (du/dy)τ = k (du/dy)n or τ = τ₀ + μₚ (du/dy)
Shear Stress vs Shear RateLinear relationshipNon-linear relationship
Viscosity DependenceDepends only on temperatureDepends on shear rate, time, and molecular structure
Flow CurveStraight lineCurved / non-linear
ExamplesWater, air, kerosene, alcohol, mercuryHoney, ketchup, blood, toothpaste, paints, oobleck
Types— (No types; simple behavior)Pseudoplastic, Dilatant, Bingham Plastic, Thixotropic, Rheopectic
ApplicationsAerodynamics, lubrication, pipelines, hydraulic systemsFood processing, cosmetics, drilling mud, biomedical fluids, paints
Industries UsedAviation, aerospace, chemical plants, HVACFMCG, oil & gas, biomedical, pharmaceuticals, construction
Behavior Under ForcePredictable, easy to modelComplex, may require rheometers for analysis
Temperature SensitivityModerateHigh (strong dependence on structure)
Fluid Flow
1. Steady & Unsteady Flow
Steady flow properties do not change with time.

Steady: ∂(property)/∂t = 0

Example (Steady): Water flowing through a constant pipe

Unsteady flow properties vary with time. ∂(property)/∂t ≠ 0
Example (Unsteady): Pump start-up flow

2. Uniform & Non-uniform Flow

Uniform: Velocity same at every point.

∂u/∂x = 0
Example: Long straight pipe flow

Non-uniform: Velocity varies along path.

∂u/∂x ≠ 0
Example: Flow through a nozzle

3. Laminar & Turbulent Flow
Re = (ρUD)/μ
Laminar: Smooth, orderly motion of fluid layers.E.g., Honey or oil flow (Re < 2000)
Turbulent:Chaotic, mixing flow. E.g., Water from a fast-open tap (Re > 4000)
4. Compressible & Incompressible Flow
Compressible: Density changes significantly, dρ/dt = 0
or, ∇·V = 0
Example: High-speed air flow.
Incompressible: Constant density, dρ/dt ≠ 0
Example: Water at low speeds.
5. Rotational & Irrotational Flow
ω = ∇ × V ≠ 0
Rotational: Vortex near drain
∇ × V = 0
Irrotational: Potential flow over airfoils
6. 1D, 2D & 3D Flow
V = V(x) 1D: Simple pipe flow
V = V(x, y) 2D: Flow over a flat plate
V = V(x, y, z) 3D: Turbulent flow in real world

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1.3 Conservation Law
1.4 Dimensional analysis

Silver mist suffused the deck of the ship.

As I went on, still gaining velocity, the palpitation of night and day merged into one continuous greyness; the sky took on a wonderful deepness of blue, a splendid luminous color like that of early twilight; the jerking sun became a streak of fire, a brilliant arch, in space; the moon a fainter fluctuating band; and I could see nothing of the stars, save now and then a brighter circle flickering in the blue.

Andorson

1.5 Losses of Pipes

The spectacle before us was indeed sublime.

Apparently we had reached a great height in the atmosphere, for the sky was a dead black, and the stars had ceased to twinkle. By the same illusion which lifts the horizon of the sea to the level of the spectator on a hillside, the sable cloud beneath was dished out, and the car seemed to float in the middle of an immense dark sphere, whose upper half was strewn with silver. Looking down into the dark gulf below.

Kevin D. Roberts - CEO

Aerodynamics Notes by Dr Aishwarya Dhara
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