Chapter 1 Notes - ME321: Introduction to Fluid Mechanics

Definition of Fluid

  • A substance that deforms continuously when acted on by a shearing stress of any magnitude.
  • A shearing stress (force per unit area) is created whenever a tangential force acts on a surface.

Continuum Theory

  • We assume that all the fluid characteristics we are interested in (pressure, velocity, etc.) vary continuously throughout the fluid.
  • We treat the fluid as a continuum and refer to very small volumes as a point in the flow.

Dimensions and Units

  • Dimensional Homogeneity: All theoretically derived equations are dimensionally homogeneous; the dimensions of the left side of the equation must be the same as those on the right side, and all additive terms must have the same dimensions.
  • Primary Units
    • Basic Dimension: L (length), T (time), M (mass), Q (temperature)
    • SI (Systems International):
    • Length: L = m
    • Time: T = s
    • Mass: M = kg
    • Temperature: Q = °C (K) or °F (°R)
    • British Gravitational System (BG):
    • Length: ft
    • Time: s
    • Mass: slug
    • Temperature: °F (°R)
  • Secondary Units (derived quantities)
    • Area: L2L^2
    • Velocity: LT1LT^{-1}
    • Acceleration: LT2LT^{-2}
    • Force: MLT2MLT^{-2} (N in SI or lbf in BG)
    • Density: ML3ML^{-3}
    • Pressure: ML1T2ML^{-1}T^{-2} (Pa or lbf/ft^2)
    • Energy: ML2T2ML^2T^{-2}
  • Conversion factors between BG and SI are provided in Tables 1.3 and 1.4 (not reproduced here).
  • Temperature conversions:
    • K=°C+273.15K = °C + 273.15
    • R=F+459.67^{\circ}R = ^{\circ}F + 459.67

Weight and Mass

  • Mass and force units:
    • In SI: mass unit is kilogram (kg); force unit is newton (N); 1 N=1 kg1 m/s21\text{ N} = 1\text{ kg} \cdot 1\text{ m/s}^2
    • In BG: mass unit is slug; force unit is pound-force (lbf); 1 lbf=1 slug1 ft/s21\text{ lbf} = 1\text{ slug} \cdot 1\text{ ft/s}^2
  • Weight: W=mgW = m g
    • In SI: W(N)=m(kg)gW (N) = m (kg) \cdot g with g=9.81 m/s2g = 9.81\ \text{m/s}^2
    • In BG: W(lbf)=m(slug)gW (lbf) = m (slug) \cdot g with g=32.2 ft/s2g = 32.2\ \text{ft/s}^2
  • English Engineering (EE) System:
    • W(lbf)=m(lbm)g732.2 ft/sW(\text{lbf}) = m(\text{lbm}) \, g_7 \cdot 32.2\ \text{ft/s}
    • where g_7 = 32.2\ \text{lbm\,ft/(lbf\,s^2)}

Density, Specific Volume, Specific Weight, Specific Gravity, and Ideal Gas Law

  • Density: ρ=mV\rho = \frac{m}{V}
    • Liquids: density variations with pressure/temperature are generally small.
    • Gases: density is strongly influenced by both pressure and temperature (i.e., ρp,T\rho\to p, T changes matter).
  • Specific Volume: ν=1ρ\nu = \frac{1}{\rho}
  • Specific Weight: γ=ρg\gamma = \rho g (N/m^3 or lbf/ft^3)
  • Specific Gravity: SG=ρρfSG = \frac{\rho}{\rho_f} (ratio relative to water at a specified temperature, usually water at 4°C)
  • Ideal Gas Law: p=ρRTp = \rho R T
    • pp: pressure (Pa or psf)
    • ρ\rho: density (kg/m^3 or slug/ft^3)
    • TT: absolute temperature (K or °R)
    • RR: gas constant (J/kg·K or ft·lb·slug^{-1}·K)

Viscosity and Fluid Resistance

  • Consider a material between two wide parallel plates: bottom plate fixed, top plate moving under load PP. A shear strain γ\gamma develops.
  • Equilibrium requires shear resistance tt at the plate–material interface: P=tAP = t A where AA is the plate area.
  • Solid response: τδβ\tau \propto \delta \beta; linear relation τ=Gδβ\tau = G \delta \beta (shear modulus GG, so τ=Gγ\tau = G\gamma if γ=δβ\gamma = \delta \beta).
  • Fluids: no-slip condition at the fluid–plate surface; the fluid in contact with the upper plate moves with velocity UU, while the fluid at the bottom plate has zero velocity.
  • For small time and small angles, the shear strain rate is
    • γ˙=dudy\dot{\gamma} = \frac{du}{dy} and tangent of the angle gives γβ˙=U  δtb\gamma \approx \dot{\beta} = \frac{U \; \delta t}{b}
  • Viscosity relation: τγ˙\tau \propto \dot{\gamma}; for Newtonian fluids, τ=μγ˙\tau = \mu \dot{\gamma}; where μ\mu is the dynamic (absolute) viscosity. Its value depends on the fluid and temperature.

Newtonian vs Non-Newtonian Fluids; Apparent Viscosity

  • Newtonian fluids: τ\tau is linearly related to γ˙\dot{\gamma} (i.e., τ=μγ˙\tau = \mu \dot{\gamma}).
  • Non-Newtonian fluids: the relation is not linear and may depend on shear history.
  • Apparent viscosity: μap=slope of (τ vs γ˙)\mu_{\text{ap}} = \text{slope of } (\tau \text{ vs } \dot{\gamma}) in the linear region.
  • Shear thinning: μap\mu_{\text{ap}} decreases with increasing γ˙\dot{\gamma}.
  • Shear thickening: μap\mu_{\text{ap}} increases with increasing γ˙\dot{\gamma}.
  • Temperature and pressure effects:
    • Viscosity is mildly dependent on pressure (often neglected).
    • Temperature sensitivity: liquids – viscosity decreases with temperature; gases – viscosity increases with temperature.
  • Viscosity units:
    • SI: [μ]=Pas[\mu] = \mathrm{Pa\cdot s}
    • BG: often given as lbs/ft2\mathrm{lb\cdot s/ft^2} (unit convention in notes)
    • CGS: dynes/cm2\mathrm{dyne\cdot s/cm^2} (poise, P)
  • Kinematic viscosity: ν=μρ\nu = \frac{\mu}{\rho}
    • Units: SI m2/s\mathrm{m^2/s}; BG ft2/s\mathrm{ft^2/s}; CGS St\mathrm{St} (Stokes)
    • Conversions: 1 m2/s=104 St1\ \mathrm{m^2/s} = 10^4\ \mathrm{St}; 1 St=100 cSt1\ \mathrm{St} = 100\ \mathrm{cSt}; hence 1 m2/s=106 cSt1\ \mathrm{m^2/s} = 10^6\ \mathrm{cSt}
  • Empirical correlations for viscosity
    • Sutherland equation (gases): μ=CT3/2T+S\mu = C \frac{T^{3/2}}{T + S}
    • Andrade’s equation (liquids): μ=Aexp(BT)\mu = A \exp\left(\frac{B}{T}\right)
    • Constants: C,SC, S for Sutherland; A,BA, B for Andrade

Compressibility of Fluids and Speed of Sound

  • Compressibility concept: how a fluid volume changes with pressure.
  • Bulk modulus of elasticity (bulk modulus):
    • General form: E<em>g=VpV</em>T=ρpρTE<em>g = -V \frac{\partial p}{\partial V}\Big|</em>T = \rho \frac{\partial p}{\partial \rho}\Big|_T
    • Units: Nm2\mathrm{N\,m^{-2}} (or psi in imperial units)
    • Larger EgE_g means less compressible; liquids are generally incompressible (example: water ~ 2.15 GN/m^2).
  • Gas compressibility: EgvarieswithpressureE_g varies with pressure; two limiting processes:
    • Isothermal: p=ρRTp = \rho R Tpρ=const\frac{\partial p}{\partial \rho} = \text{const}Eg=pE_g = p
    • Isentropic (adiabatic, reversible): pρκ=constEg=κpp \rho^{-\kappa} = \text{const} \Rightarrow E_g = \kappa p
  • Speed of sound: disturbance propagation speed in a fluid given byc=Egρc = \sqrt{\frac{E_g}{\rho}}
    • For ideal gases: c=γpρ=γRTc = \sqrt{\frac{\gamma p}{\rho}} = \sqrt{\gamma R T} where γ\gamma is the ratio of specific heats.
  • Note: heat transfer during sound propagation is very small; process is essentially isentropic.
  • The speed of sound in air at various temperatures is listed in reference appendices (Appendix B in notes).

Vapor Pressure and Cavitation

  • Vapor pressure pvp_v: pressure at which a completely liquid-filled container has its vapor in equilibrium with the liquid.
  • If the end is moved without allowing air, the space becomes filled with vapor at pvp_v. Local pressure drops may cause boiling; bubbles can form in low-pressure regions.
  • Bubbles may implode when entering high-pressure regions, releasing energy that can damage structures over time.
  • Reference video provided for context: https://www.youtube.com/watch?v=U-uUYCFDTrc

Surface Tension and Capillarity

  • Surface tension σ\sigma: cohesive molecular forces act along the surface, creating a contracted “skin” at the interface (liquid–gas or immiscible liquid interfaces).
  • Pressure difference across a curved interface (spherical droplet):
    • Δp=p<em>insidep</em>outside=2σR\Delta p = p<em>{\text{inside}} - p</em>{\text{outside}} = \frac{2\sigma}{R}
  • Capillary tube phenomena and wetting
    • Wetting: adhesion between wall and liquid is strong enough to pull liquid up the wall (contact angle \theta < 90^{\circ}).
    • Non-wetting: adhesion is weak relative to cohesion; liquid level in tube is depressed (contact angle \theta > 90^{\circ}, e.g., mercury).
  • Capillary rise in a tube of radius RR (balance of forces):
    • 2πRσcosθ=πR2ρghh=2σcosθρgR2 \pi R \sigma \cos \theta = \pi R^2 \rho g h \Rightarrow h = \frac{2 \sigma \cos \theta}{\rho g R}
    • Alternatively, using the specific weight γ=ρg\gamma = \rho g: h=2σcosθγRh = \frac{2 \sigma \cos \theta}{\gamma R}
  • Note: wetting angle conventions apply: θ<90wetting,θ>90non-wetting\theta < 90^{\circ}\Rightarrow\text{wetting}, \theta > 90^{\circ}\Rightarrow\text{non-wetting}
  • Examples: water wets common glasses (low contact angle); mercury does not wet glass (high contact angle).

Additional Notes and References

  • The transcript includes a video link for cavitation and mentions Appendix B for speed of sound data.
  • Tables for conversion factors (BG↔SI) are provided in the source material (Tables 1.3 and 1.4).
  • Equations and constants cited reflect standard fluid mechanics conventions, with some notation variations in the original lecture notes.