Throughout, remember the two headline results built in the parent note:
ΔPdrop=r2γ,ΔPsoap bubble=r4γ,ΔP=γ(R11+R21).
Here γ (surface tension) is force-per-length or energy-per-area, r is the sphere radius, and R1,R2 are the two principal radii (how sharply the surface bends in two perpendicular directions). Unless told otherwise, take γwater=0.072N/m and atmospheric pressure P0=1.013×105Pa.
WHAT to spot: the only difference is the number of liquid–air interfaces.
A drop has one interface (liquid inside, air outside) → ΔP=r2γ.
A soap bubble is a thin film with air on both sides → two interfaces → ΔP=r4γ.
With r=2×10−3m:
ΔPdrop=2×10−32(0.072)=72Pa,ΔPbubble=2×10−34(0.072)=144Pa.
The bubble’s excess pressure is exactly twice the drop’s — because it has twice as many skins squeezing.
Recall Solution — L1·Q2
Force per length: mN.
Energy per area: m2J=m2N⋅m=mN.
Same unit ⇒ the two definitions describe one physical number. That is why the parent note could write γ=F/L=energy/area.
WHY energy, not pressure: the question asks for work done against the surface, which is γ×(area created).
A soap bubble has two surfaces (inner + outer), each of area 4πR2:
Atotal=2×4πR2=8πR2.W=γAtotal=0.030×8π(0.03)2=0.030×8π×9×10−4.W=6.786×10−4J≈6.79×10−4J.What it means: less than a milli-joule — surfaces are cheap, which is why a gentle breath makes a big bubble.
Recall Solution — L2·Q2
A film has two faces, so both pull down on the wire:
F=2γL=2(0.025)(0.08)=4.0×10−3N=4.0mN.WHY the 2: forgetting it halves the answer — the classic F=2γL frame result.
WHY compare 1/r: each bubble's excess pressure is ΔP=r4γ∝r1. Smaller r ⇒ larger excess pressure.
Bubble B (r=2cm) has the higher internal pressure.
Air therefore flows from B (small) to A (big) — the small bubble shrinks, the big one grows.
(b) Both bubbles sit in the same atmosphere P0, so the driving difference is the difference of excess pressures:
ΔPA=0.044(0.030)=3.0Pa,ΔPB=0.024(0.030)=6.0Pa.ΔPA−ΔPB=3.0−6.0=−3.0Pa.
The negative sign confirms B's pressure exceeds A's by 3.0Pa, pushing air toward A. See the figure: the tighter (redder) skin squeezes harder.
Recall Solution — L3·Q2
WHAT the middle film feels: on one side is bubble B's inside (higher pressure PB), on the other side is bubble A's inside (lower pressure PA). The film curves toward the low-pressure side (bulges into A), and its own Young–Laplace jump must equal the pressure difference across it.
A single dividing film still has two faces, so:
jump across mid filmrmid4γ=PB−PA=rB4γ−rA4γ.
Cancel 4γ:
rmid1=rB1−rA1=0.021−0.041=50−25=25m−1.rmid=251=0.04m=4cm=rA.Neat result:rmid=rA−rBrArB; here it equals rA because rA=2rB.
(a) Volume is conserved (liquid is nearly incompressible):
8×34πa3=34πR3⇒R3=8a3⇒R=2a=2mm.(b) Compare surface areas (a drop has one interface):
Asmall,totalAbig=8×4πa24πR2=8a2R2=8a2(2a)2=84=21.
Surface energy =γA, so the energy halves — the merged drop stores half the surface energy of the eight droplets.
(c) Energy went down, so surface energy is released (appears as heat / slight warming). This is why small droplets spontaneously coalesce: it lowers the system's energy.
Recall Solution — L4·Q2
(a) A hemispherical meniscus is one interface with R1=R2=r:
ΔP=γ(r1+r1)=r2γ=2.0×10−42(0.072)=720Pa.
The pressure just below the curved meniscus is 720Palower than atmospheric (the surface curves away from the liquid).
(b) That deficit is balanced by the weight of the raised column, ρgh:
ρgh=r2γ⇒h=ρgr2γ=1000×9.8×2.0×10−42(0.072).h=1.960.144=0.07347m≈7.35cm.What it means: the same Young–Laplace jump that pressurises a drop pulls water up a thin tube — the physics is identical, just curved the other way.
WHY PV conservation: temperature is fixed, so for the trapped air Boyle's law PV=const holds for the total enclosed air. Each bubble's internal absolute pressure is P=P0+r4γ (excess pressure added to atmosphere), and its volume is 34πr3.
Conserve total PV:
(P0+r14γ)34πr13+(P0+r24γ)34πr23=(P0+r4γ)34πr3.
Cancel 34π and expand:
P0r3+4γr2=P0(r13+r23)+4γ(r12+r22).
Plug numbers (r1=0.03,r2=0.04m,4γ=0.12):
So the equation is:
1.013×105r3+0.12r2=9.2183+3.0×10−4=9.21860.
The surface terms are tiny next to P0r3, so to good accuracy r3≈r13+r23=9.1×10−5:
r≈(9.1×10−5)1/3=0.04497m≈4.50cm.
Solving the full cubic numerically shifts r by well under 0.01mm, so r≈4.50cm. Insight: at ordinary atmospheric pressure the surface-energy terms barely matter — the merged volume is essentially r13+r23. The Young–Laplace correction only dominates in vacuum, where P0→0.
Recall Solution — L5·Q2
With P0=0 the PV equation loses its P0r3 term. Using P=r4γ:
r14γ⋅34πr13+r24γ⋅34πr23=r4γ⋅34πr3.
Cancel 34π⋅4γ:
r12+r22=r2⇒r=r12+r22=0.032+0.042=0.0025=0.05m=5cm.WHY it changed: with no external pressure, the only pressure comes from surface tension, so the conserved quantity becomes surface area (4γ/r×r3∝r2) rather than volume. The merged bubble is a 3-4-5 right triangle in radii — a clean signature that areas add, not volumes. In atmosphere, the huge P0 makes volume the near-conserved quantity instead (Q1). This is the same "which quantity is conserved" theme as the coalescing drops, now sharpened.
Drop vs soap-bubble excess pressure? ::: 2γ/r vs 4γ/r (one surface vs two).
Work to blow a bubble of radius R? ::: γ×8πR2 (two surfaces).
Eight drops of radius a merge — big radius and energy factor? ::: R=2a; surface energy halves.
Coalescing bubbles in air — what is nearly conserved? ::: total volume, r3≈r13+r23.
Coalescing bubbles in vacuum — what is conserved? ::: total area, r2=r12+r22.