Fluid Properties and Hydrostatics – Notes

Compressibility of water and basic fluid concepts

  • Myth vs reality: water is often treated as incompressible in everyday life, but it is compressible. A tap on a glass creates a compression wave in the water that travels at finite speed, not instantaneously. Sound in water is a longitudinal (compression) wave.

  • Importance of compressibility: essential for understanding phenomena like sound propagation, submarine sonar, and echolocation in whales. In everyday conditions, compressibility effects are tiny, but under high pressures or strong waves they become significant.

  • Quantitative example (compressibility under high pressure):

    • Depth example: a glass of water at roughly sea level, pressure ~1 atm. If the same water is at a depth of about 5 km (≈ 16,400 ft) below the ocean surface, the pressure is about 500 times higher than at the surface.

    • Resulting volume change: the water would compress by roughly racriangleVVext(at5extkm)2.3%.rac{ riangle V}{V} \, ext{(at }5 ext{ km)} \approx 2.3\%.

    • This illustrates that water compression is small but measurable under extreme pressures.

  • Everyday applications where compression matters:

    • Water jet cutting uses high-pressure water pumps: typically 200 to 600 MPa200\text{ to }600\ \text{MPa} (≈ 30,000 to 90,000 psi). Compare to surface glass pressure, this is about 2–6,000× higher, leading to significant compression effects on the jet fluid.

    • At around 350 MPa350\ \text{MPa} (~50,000 psi), water compresses by about 14.7%14.7\%, which is substantial.

    • At similar pressures, the chamber pressure of a high-powered rifle underwater is ~350 MPa350\ \text{MPa}; forward-projectiles must compress water ahead of them in the barrel, drastically affecting performance.

  • Where the myth comes from:

    • For most normal daily activities, water behaves nearly incompressibly due to its very large bulk modulus. Compressibility becomes relevant under high pressures or when strong waves/sonic disturbances propagate through the liquid.

Key fluid properties: density and specific volume

  • Density: ρ=mV\rho = \frac{m}{V}

    • SI unit: kg/m3\text{kg/m}^3

    • Dimension: [M L3][\text{M L}^{-3}] (mass per unit volume).

  • Specific volume: v=Vm=1ρv = \frac{V}{m} = \frac{1}{\rho}

    • SI unit: m3/kg\text{m}^3/\text{kg}

  • Dependence on temperature and pressure:

    • Liquids (e.g., water): density changes weakly with temperature/pressure. At a given pressure, density typically decreases with increasing temperature; there is a notable exception near four degrees Celsius where liquid water has maximum density at 1 bar (≈ 1000 kg/m31000\ \text{kg/m}^3).

    • Gases (e.g., air): density changes strongly with temperature and pressure; heating lowers density, increasing volume at the same pressure.

    • General rule: density variation is weak for liquids and strong for gases.

Specific weight and specific gravity

  • Specific weight: γ=ρg\gamma = \rho g

    • Units: N/m3\text{N/m}^3

    • Dimension: same as pressure per unit length; gamma is interchangeable with ρg\rho g.

  • Specific gravity: SG=ρρrefSG = \frac{\rho}{\rho_{\text{ref}}}

    • Dimensionless; reference density typically the density of water at 20°C: ρref998 kg/m3  (often rounded to 103 kg/m3)\rho_{\text{ref}} \approx 998 \ \text{kg/m}^3\;\text{(often rounded to }10^3\text{ kg/m}^3)

    • No units because the ratio cancels.

Pressure: definition and types

  • Pressure: p=FAp = \frac{F}{A}

    • Force is normal to a surface; pressure is a scalar.

  • Pressure vs pressure force:

    • Pressure is a scalar (magnitude only).

    • Pressure force on a surface is a vector, normal to the surface, with magnitude F=pAF = p A.

  • Gauge vs absolute (total) pressure:

    • Gauge pressure: P{gauge} = p{total} - p{atm}

    • Atmospheric pressure: patm101.3 kPap_{atm} \approx 101.3\ \text{kPa}

    • Absolute (total) pressure: p{total} = p{atm} + p{gauge}

  • In fluid mechanics, unless stated otherwise, pressure often means gauge pressure; be mindful of the context.

Ideal gas law (useful in thermodynamics and some fluid problems)

  • Equation: P=ρRTP = \rho R T

    • P: total pressure (Pa)

    • ρ: density (kg/m^3)

    • R: specific gas constant (J/(kg·K))

    • T: absolute temperature (K)

  • Gas constant for air (example): at about 15°C, R \approx 286.9\ \text{J/(kg·K)}

  • Temperature scale:

    • Absolute temperature: T(K)=T(°C)+273.15T(K) = T(°C) + 273.15

    • Absolute zero: T=0KT=273.15°CT = 0\,\text{K} \quad\leftrightarrow\quad T = -273.15°\text{C}

  • Note: R depends on the gas; for calculations in air at modest temperatures, the cited value is a typical reference.

Bulk modulus and compressibility

  • Concept: relationship between pressure change and volume change under compression/expansion.

  • Definition: B=VdPdVB = - V \frac{dP}{dV}

    • Rearranged: dPdV=BV\frac{dP}{dV} = -\frac{B}{V}

    • Unit: same as pressure (Pa).

  • Implications:

    • Liquids (like water) have very large bulk modulus; compressibility is negligible for many civil engineering problems.

    • Gases have small bulk modulus; they are easily compressible.

Viscosity and the nature of fluids

  • Viscosity concept: internal friction within a fluid; resistance to shear.

  • Newton's law of viscosity (dynamic/absolute viscosity):

    • Consider two parallel plates with a fluid in between; top plate moves with velocity u, bottom plate fixed.

    • Shear stress: τ=μdudy\tau = \mu \frac{du}{dy}

    • Here, μ\mu is the dynamic (absolute) viscosity (Pa·s).

  • Units of viscosity: typically Pa·s, but also N·s/m^2 or kg/(m·s) through unit equivalences.

  • Velocity profile under simple shear (no-slip at boundaries): linear profile between plates for small gaps.

  • Kinematic viscosity: ν=μρ\nu = \frac{\mu}{\rho}

    • Units: m^2/s

  • Newtonian vs non-Newtonian fluids:

    • Newtonian fluid: viscosity is constant for given temperature/pressure; plot of shear stress vs. shear rate is linear through the origin: τ=μdudy\tau = \mu \frac{du}{dy}.

    • Non-Newtonian fluids: viscosity varies with shear rate.

    • Shear thinning (pseudoplastic): viscosity decreases as shear rate increases.

    • Shear thickening (dilatant): viscosity increases as shear rate increases.

    • Examples:

    • Paint: shear thinning (easier to spread when stirred/painted).

    • Cornstarch–water mixture: shear thickening in some regimes.

  • Temperature and density effects on viscosity:

    • For liquids like water, increasing temperature generally decreases viscosity; density is relatively constant.

    • For gases, increasing temperature can increase viscosity, while density decreases with temperature; kinematic viscosity may increase with temperature for gases.

Isothermal atmosphere and vertical density variation (example with ideal gas law)

  • Isothermal atmosphere problem (density not constant in height):

    • Start with hydrostatic equation and ideal gas law; density ρ is not constant when height increases.

    • Hydrostatic equation (density variable):

    • General form: dPdz=ρ(z)g\frac{dP}{dz} = -\rho(z) g

    • Using ideal gas law with isothermal assumption (constant T): ρ = P/(R T).

    • Substitute into hydrostatic equation and separate variables:
      dPP=gRTdz\frac{dP}{P} = -\frac{g}{R T} dz

    • Integrate from sea level (z=0, pressure P0) to height h (z=h): ln(P(h)P</em>0)=ghRT\ln\left(\frac{P(h)}{P</em>0}\right) = -\frac{g h}{R T}

    • Solve for P(h):
      P(h)=P0exp(ghRT)P(h) = P_0 \exp\left(-\frac{g h}{R T}\right)

  • Example numbers (isothermal atmosphere):

    • Sea level pressure: P0101.3 kPaP_0 \approx 101.3\ \text{kPa}.

    • At height h=1000 mh = 1000\ \text{m}, using the isothermal relation, one gets roughly P(h)89.96 kPaP(h) \approx 89.96\ \text{kPa} (absolute).

    • Gauge pressure at that height would be P(h)P011.34 kPaP(h) - P_0 \approx -11.34\ \text{kPa} (lower than atmospheric pressure at the surface).

Hydrostatics: horizontal vs vertical pressure variation

  • Hydrostatic principles 1 Horizontal variation in static fluids is zero: in a static fluid, pressure does not vary with horizontal position along a horizontal plane.

    • If you consider a small control volume, forces in the x- and y-directions balance, giving P{Left} = P{Right}andandP{front} = P{back} for the same fluid.
      2) Vertical variation (hydrostatic equation):

    • For a small vertical element, include top/bottom pressures plus weight:
      dPdz=ρg\frac{dP}{dz} = -\rho g, which is pressure change in the z direction / change in depth, and this is the hydrostatic equation. (and this is equation is correct regardless the density being constant or not) and this is principal 2 (and if what to integrate the equation need to keep in mind if density is constant or not)

    • Sign convention on the RHS depends on the chosen axis; with the common choice of z positive upward, the derivative is negative.

    • Principal 3 (pressure at a given Hight)

    • If density is constant, integrate (the hydrostatic equation) to obtain the classic head relation: (had integrate both sides with lower limit 0 and upper limit as -h by dz)
      P(z)=P0+ρghP(z) = P_0 + \rho g h , this is general form z can be h also, also row g and be replaced by gama

    • P(h) = P0P_0 + ρgh\rho gh, which is Absolute Pressure

    • and if P0P_0 is P{atm}, P(h)-P0P_0= ρgh\rho gh , Then its Gauge Pressure

    • if density varies with height, integrate (the hydrostatic equation ) using the variable density:

  • Important remarks:

    • The negative sign in the hydrostatic equation matches the chosen coordinate system and gravity direction.

    • The hydrostatic equation holds regardless of whether density is constant or changing; the integration requires accounting for density variation if present.

Pressure measurement devices (basics)

  • Barometer:

    • Uses a mercury column to measure atmospheric pressure; standard is 760 mm Hg, equivalent to 101.3 kPa at sea level.

    • Pressure from the column: P<em>atmρ</em>Hggh<em>HgP<em>{atm} \approx \rho</em>{Hg} g h<em>{Hg} with h{Hg} ≈ 760 mm.

    • P{atm}=P{vapor}+ρgh\rho gh , since P{vapor} very small we ignore it so,

    • P{atm}=ρgh\rho gh

  • Piezometer:

    • A simple tube open to the atmosphere used to indicate the pressure in a pipe.

    • If the pipe fluid has density ρ1 and specific weight γ1, and the top is open to atmosphere, the reading is:

    • Total pressure: PA = P{atm} + γ1h1

    • Gauge pressure: p{g} = γ1h1

    • Limitations: only measures moderate pressures and requires a tall column for high pressures.

  • U-tube manometer:

    • Used to measure pressure difference between two points (A and B) in possibly different fluids or at different elevations.

    • The relation depends on fluid density and column heights; a standard exercise is to derive the equation relating P at point Aandand P at point B from the manometer readings.

    • Practical hint: horizontal pressure variation in static fluids is zero for the same fluid; be careful with different fluids.

Practical example problems (two illustrations from the lecture)

  • Example 1: belt on the surface of a long water tank

    • Setup: a belt moves on the surface with velocity u=10 m/su = 10\ \text{m/s}; fluid layer depth is given; viscosity is known; contact area A is known.

    • Force and power: the friction force acts to resist motion; the required power is
      P=FuP = F \cdot u

    • From Newton’s law of viscosity, friction (shear) stress is
      τ=μdudy\tau = \mu \frac{du}{dy}

    • Friction force is F=τAF = \tau \cdot A and velocity gradient is approximated by dudyuh\frac{du}{dy} \approx \frac{u}{h} (for a layer of thickness h).

    • Substitution gives
      Pμ(dudy)Au=μ(uh)A  u=μAu2hP \approx \mu \left(\frac{du}{dy}\right) A\, u = \mu \left(\frac{u}{h}\right) A \; u = \mu A \frac{u^2}{h}

    • With the provided numbers (viscosity, area, depth, velocity), the result given was approximately P1.34×102 WP \approx 1.34\times 10^2\ \text{W} (134.4 W).

  • Example 2: isothermal atmosphere and the ideal gas law

    • Question: what is the pressure at height h above the surface when ρ is not constant but P = ρ R T with T constant?

    • Start with hydrostatic equation and ideal gas to derive the isothermal atmosphere relation:

    • Isothermal hydrostatics leads to
      dPP=gRTdz\frac{dP}{P} = -\frac{g}{R T} dz

    • Integrating from 0 to h gives
      P(h)=P0exp(ghRT)P(h) = P_0 \exp\left(-\frac{g h}{R T}\right)

    • Example numbers (isothermal Earth scenario): at h = 1000 m, with typical surface conditions, one finds

    • Absolute pressure: P(h)89.96 kPaP(h) \approx 89.96\ \text{kPa}

    • Gauge pressure: P(h){gauge} = P(h) - P{atm} = approx -11.34 kPa

    • This demonstrates how pressure decreases with height in an isothermal atmosphere.

Connections to core principles and real-world relevance

  • Foundational concepts traced back to earlier lectures in fluid mechanics:

    • Pressure is a scalar; pressure forces act normal to surfaces.

    • The difference between gauge and absolute pressure and the role of atmospheric pressure in measurements.

    • The distinction between density for liquids (weak sensitivity to T/P) and gases (strong sensitivity to T/P).

    • The ideal gas law as a bridge between macroscopic properties (P, V, T) and microscopic behavior for gases.

    • The hydrostatic equation as a fundamental tool for static fluids and the derivation of pressure with depth.

  • Practical engineering relevance:

    • Designing piping, reservoirs, and hydrostatic structures requires accounting for pressure variation with depth and density changes.

    • Viscosity and non-Newtonian behavior impact flow resistance and energy losses in pipes, coatings, and processes (e.g., paint, clumping materials).

    • High-pressure processes (e.g., water-jet cutting) require awareness of compressibility effects and bulk modulus.

    • Atmospheric pressure and buoyancy considerations in civil and environmental engineering rely on hydrostatics and the ideal gas law for air.

Summary of key equations (LaTeX)

  • Density and specific volume
    ρ=mV\rho = \frac{m}{V}
    v=Vm=1ρv = \frac{V}{m} = \frac{1}{\rho}

  • Specific weight and specific gravity
    γ=ρg\gamma = \rho g
    SG=ρρrefSG = \frac{\rho}{\rho_{\text{ref}}}

  • Pressure concepts
    p=FAp = \frac{F}{A}
    p<em>g=pp</em>atmp<em>{g} = p - p</em>{atm}
    patm101.3 kPap_{atm} \approx 101.3\ \text{kPa}

  • Ideal gas law (isothermal context)
    P=ρRTP = \rho R T
    T(K)=T(°C)+273.15T(K) = T(°C) + 273.15
    R \approx 286.9\ \text{J/(kg·K)}\;\text{(air at ~15°C)}

  • Bulk modulus
    B=VdPdVB = - V \frac{dP}{dV}
    dPdV=BV\frac{dP}{dV} = -\frac{B}{V}

  • Viscosity and shear (Newton’s law)
    τ=μdudy\tau = \mu \frac{du}{dy}
    ν=μρ\nu = \frac{\mu}{\rho}

  • Newtonian vs non-Newtonian (conceptual)

    • Newtonian: line through origin in τ\tau vs. dudy\frac{du}{dy} plot.

    • Shear thinning: viscosity decreases with shear rate.

    • Shear thickening: viscosity increases with shear rate.

  • Hydrostatics dPdz=ρg\frac{dP}{dz} = -\rho g

    • With constant density: P(z)=P0+ρghP(z) = P_0 + \rho g h

    • With variable density: P(h)=P<em>0+</em>0hρ(z)gdzP(h) = P<em>0 + \int</em>0^h \rho(z) g \, dz

  • Barometer relation
    P<em>atm=ρ</em>Hggh<em>Hg(h</em>Hg=760 mm)P<em>{atm} = \rho</em>{Hg} g h<em>{Hg} \quad (h</em>{Hg} = 760\ \text{mm})

  • Isothermal atmosphere pressure variant
    P(h)=P0exp(ghRT)P(h) = P_0 \exp\left(-\frac{g h}{R T}\right)

  • Pressure at depth (barometric-like relation)
    P(h)  and gauge=P(h)PatmP(h) \;\text{and gauge} = P(h) - P_{atm}

  • U-tube manometer (pressure difference, generic form)

    • For same fluid: P<em>AP</em>B=γh(difference in column heights)P<em>A - P</em>B = \gamma h\,\text{(difference in column heights)}