2.2.21Fluid Mechanics

Boundary layer thickness, displacement thickness, momentum thickness

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1. Boundary layer thickness δ\delta

WHY 99% and not 100%? Because uUu \to U only as yy\to\infty (asymptotic). We need a finite cutoff, so we pick a conventional threshold. 99% is the standard.

WHAT it represents: a geometric edge of the slowed-down region.

HOW it grows: For laminar flow over a flat plate (Blasius), δ\delta grows with distance xx: δ5xRex,Rex=Uxν\delta \approx \frac{5x}{\sqrt{Re_x}}, \qquad Re_x = \frac{Ux}{\nu} So the layer thickens downstream — there's more slowed fluid the longer the wall has acted.

Figure — Boundary layer thickness, displacement thickness, momentum thickness

2. Displacement thickness δ\delta^* — derive it

Derivation from first principles (mass conservation):

Mass flux per unit width if the whole region moved at UU (ideal): m˙ideal=0ρUdy\dot m_{ideal} = \int_0^{\infty} \rho\, U \, dy

Actual mass flux (real, slowed): m˙real=0ρudy\dot m_{real} = \int_0^{\infty} \rho\, u \, dy

The deficit in mass flux: Δm˙=0ρ(Uu)dy\Delta \dot m = \int_0^{\infty} \rho\,(U - u)\, dy

We define δ\delta^* as the thickness of an ideal stream (speed UU) carrying this same deficit: ρUδ=0ρ(Uu)dy\rho U \,\delta^* = \int_0^{\infty}\rho\,(U-u)\,dy


3. Momentum thickness θ\theta — derive it

Derivation: The momentum actually carried by the slowed fluid is ρuudy\int \rho u \cdot u\, dy. The momentum that this same mass flow ρu\rho u would carry if moving at UU is ρuUdy\int \rho u \cdot U\, dy. The deficit: Δ(momentum)=0ρu(Uu)dy\Delta(\text{momentum}) = \int_0^\infty \rho\, u\,(U - u)\, dy

Set this equal to the momentum of an ideal slab of thickness θ\theta at speed UU, i.e. ρU2θ\rho U^2 \theta: ρU2θ=0ρu(Uu)dy\rho U^2 \theta = \int_0^\infty \rho\,u\,(U-u)\,dy


4. Worked Examples


5. Common Mistakes


6. Active Recall Flashcards

What is the no-slip condition?
At a solid wall, fluid velocity equals the wall velocity (zero for a stationary wall), so u(0)=0u(0)=0.
Define boundary layer thickness δ\delta.
Distance from the wall where u=0.99Uu = 0.99U (99% of free-stream speed).
Why 99% and not 100%?
Because uUu \to U only asymptotically; a finite cutoff is needed, 99% is the convention.
Formula for displacement thickness.
δ=0(1u/U)dy\delta^* = \int_0^\infty (1 - u/U)\,dy.
Physical meaning of δ\delta^*.
Distance the outer streamlines are pushed away from the wall = thickness of an ideal UU-stream carrying the missing mass flux.
Formula for momentum thickness.
θ=0uU(1u/U)dy\theta = \int_0^\infty \frac{u}{U}(1 - u/U)\,dy.
Physical meaning of θ\theta.
Thickness of an ideal UU-stream carrying the momentum lost to the wall; related to wall drag.
Why does θ\theta have the extra u/Uu/U factor?
Momentum deficit =ρu(Uu)= \rho u (U-u): needs the actual mass-flow uu AND the velocity gap (Uu)(U-u).
Order of the three thicknesses.
θ<δ<δ\theta < \delta^* < \delta.
Define shape factor HH and its laminar value.
H=δ/θH = \delta^*/\theta; Blasius laminar H2.59H \approx 2.59; rising HH signals impending separation.
For a linear profile u/U=y/δu/U=y/\delta, give δ\delta^*, θ\theta, HH.
δ=δ/2\delta^*=\delta/2, θ=δ/6\theta=\delta/6, H=3H=3.
Blasius growth law for δ\delta.
δ5x/Rex\delta \approx 5x/\sqrt{Re_x}, with Rex=Ux/νRe_x = Ux/\nu.

Recall Feynman: explain to a 12-year-old

Imagine running your hand flat through water. The water touching your hand drags along with it, but water far away barely cares. There's a thin "sticky layer" near your hand where water goes from "stuck" to "free." That layer's height is δ\delta. Now, because some water near the hand is moving slower, less water slips past than you'd expect — it's as if the hand were a tiny bit fatter and blocked a sliver of water. That fattening is the displacement thickness δ\delta^*. And the hand also steals momentum (push) from the water, which is what makes drag — the amount of stolen push, written as a thickness, is the momentum thickness θ\theta. Three rulers, three different things they measure.

Connections

  • No-slip condition — the physical origin of the boundary layer.
  • Reynolds number — governs whether the layer is laminar or turbulent.
  • Blasius solution — exact flat-plate laminar profile giving δ=5x/Rex\delta = 5x/\sqrt{Re_x}.
  • Skin friction drag — directly proportional to θ\theta via the momentum-integral equation.
  • Boundary layer separation — predicted by rising shape factor HH.
  • Viscosity — the property that creates the velocity gradient at the wall.

Concept Map

creates

velocity climbs 0 to U

needs finite cutoff

defined at 99% of U

grows with x

slows fluid near wall

equivalent slab thickness

integral 1 minus u over U

removes momentum

equivalent slab thickness

relates to wall drag

No-slip condition

Boundary layer

Asymptotic approach to U

Boundary layer thickness delta

u equals 0.99 U

Blasius 5x over sqrt Rex

Mass flux deficit

Displacement thickness delta star

Streamline outward push

Momentum loss / drag

Momentum thickness theta

Wall shear stress

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, jab koi real fluid (viscous) kisi wall ke paas se behta hai, to wall ko touch karne wala fluid bilkul ruk jaata hai — isko no-slip condition kehte hain. Wall pe speed zero, aur door free-stream speed UU. Beech ki jo patli si layer hai jahan velocity 00 se UU tak chadhti hai, usko boundary layer bolte hain. Problem yeh hai ki yeh layer kahan "khatam" hoti hai yeh clearly nahi pata, kyunki uu dheere-dheere UU tak pahunchti hai. Isliye hum 99% wali jagah ko δ\delta keh dete hain — yeh bas geometry ka ruler hai.

Ab do aur important measures hain. Displacement thickness δ\delta^* batata hai ki wall ke paas fluid slow hone ki wajah se kitna mass flow kam ho gaya — jaise wall thoda mota ho gaya ho aur streamlines ko bahar push kar raha ho. Formula: δ=(1u/U)dy\delta^*=\int(1-u/U)\,dy. Momentum thickness θ\theta batata hai ki wall ne kitna momentum (push) chura liya — yahi cheez drag banati hai. Formula: θ=uU(1u/U)dy\theta=\int \frac{u}{U}(1-u/U)\,dy. Yaad rakho: momentum mein ek extra u/Uu/U factor isliye aata hai kyunki momentum u2\sim u^2 hota hai — ek uu mass-flow ke liye, doosra velocity gap ke liye.

Trick samajh lo: δ\delta^* mein ek deficit factor (mass), θ\theta mein deficit ko u/Uu/U se multiply (momentum). Aur hamesha order yeh: θ<δ<δ\theta < \delta^* < \delta. Inka ratio H=δ/θH=\delta^*/\theta shape factor hai — agar yeh badhne lage to flow separate hone wala hai, yeh engineering mein bahut kaam aata hai. Exam mein aksar linear ya sine profile dekar δ,θ\delta^*,\theta nikalne ko aata hai — bas integral lagao, ho gaya!

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Connections