Differential-Equations Β· Unit 4 Β· Video 1 Β· Interactive Practice

Scale Before You Solve: The Fourth-Power Cooling Law Made Dimensionless

IKey Formulas

FormulaNameWhat it says
x1=xa,y1=ybx_1 = \dfrac{x}{a}, \quad y_1 = \dfrac{y}{b}ScalingMeasure xx in units of size aa and yy in units of size bb (aa, bb constants)
dTdt=k (M4βˆ’T4)\dfrac{dT}{dt} = k\,(M^4 - T^4)Fourth-power cooling law (very high temperatures)Body TT, constant surroundings MM, both absolute; k>0k > 0
T=M T1:dTdt=M dT1dt,T4=M4 T14T = M\,T_1: \quad \dfrac{dT}{dt} = M\,\dfrac{dT_1}{dt}, \quad T^4 = M^4\,T_1^4SubstitutionDefine T1=T/MT_1 = T/M, substitute for TT; the derivative step needs MM constant
dT1dt=k1 (1βˆ’T14),k1=kM3\dfrac{dT_1}{dt} = k_1\,(1 - T_1^4), \quad k_1 = kM^3Scaled cooling lawT1T_1 has no units; k1k_1 is in per second

Key Insight: Define T1=T/MT_1 = T/M, but substitute T=MT1T = MT_1, because TT is what appears in the equation. The scaled equation is no easier to solve; it has a dimensionless temperature and one constant, k1=kM3k_1 = kM^3, in place of two.

IIVisualization 1 β€” Choosing the Unit of Temperature

Measuring TT in units of aa relabels the axis and leaves the curve alone; only a=Ma = M turns the bracket's constant into 11.

IIIVisualization 2 β€” Why the Temperatures Must Be Absolute

A difference of two temperatures ignores where zero is; a difference of their fourth powers does not.

IVVisualization 3 β€” Two Constants Lumped into One

After scaling, kk and MM enter only through k1=kM3k_1 = kM^3: equal k1k_1 and equal T1(0)T_1(0) give the same T1T_1 curve.

πŸ’‘ The substitution relies on MM being constant: if MM varied with tt, the product rule would give dTdt=M′ T1+M dT1dt\dfrac{dT}{dt} = M'\,T_1 + M\,\dfrac{dT_1}{dt}, and the scaled equation would gain the extra term βˆ’Mβ€²M T1-\dfrac{M'}{M}\,T_1.

VQuiz Questions

Problem 1 Β· Lump the Constants

Given: dTdt=k (M4βˆ’T4)\dfrac{dT}{dt} = k\,(M^4 - T^4) with k=2Γ—10βˆ’12k = 2\times10^{-12} per second per kelvin cubed and surroundings at M=500M = 500 K. The substitution T=MT1T = MT_1 turns it into dT1dt=k1 (1βˆ’T14)\dfrac{dT_1}{dt} = k_1\,(1 - T_1^4). Find k1k_1 in per second.

βœ… Correct! k1=kM3=(2Γ—10βˆ’12)(1.25Γ—108)=2.5Γ—10βˆ’4k_1 = kM^3 = (2\times10^{-12})(1.25\times10^{8}) = 2.5\times10^{-4} per second: the kelvin cubed in the units of kk cancels against M3M^3.
❌ That is kM4kM^4. The left side carries a factor of MM too, dTdt=M dT1dt\dfrac{dT}{dt} = M\,\dfrac{dT_1}{dt}, and dividing by it leaves kM3kM^3.
❌ Scaling does change the constant. Substituting T=MT1T = MT_1 pulls M4M^4 out of the bracket and MM out of the derivative, so the coefficient becomes the lump kM3kM^3.
❌ The powers of MM multiply kk. After substitution, M dT1dt=kM4(1βˆ’T14)M\,\dfrac{dT_1}{dt} = kM^4(1 - T_1^4); dividing by MM gives kM3kM^3, not k/M3k/M^3.
Show solution

Since MM is constant, T=MT1T = MT_1 gives dTdt=M dT1dt\dfrac{dT}{dt} = M\,\dfrac{dT_1}{dt} and T4=M4T14T^4 = M^4T_1^4. Substituting:

M dT1dt=k (M4βˆ’M4T14)=kM4 (1βˆ’T14)M\,\frac{dT_1}{dt} = k\,(M^4 - M^4T_1^4) = kM^4\,(1 - T_1^4)

Divide both sides by MM:

dT1dt=kM3 (1βˆ’T14),k1=kM3\frac{dT_1}{dt} = kM^3\,(1 - T_1^4), \qquad k_1 = kM^3

With the numbers, M3=5003=1.25Γ—108M^3 = 500^3 = 1.25\times10^{8}, so

k1=(2Γ—10βˆ’12)(1.25Γ—108)=2.5Γ—10βˆ’4k_1 = (2\times10^{-12})(1.25\times10^{8}) = 2.5\times10^{-4}

Units: per second per kelvin cubed, times kelvin cubed, leaves per second.

Problem 2 Β· Which Quantity Ignores the Zero?

Given: a body at T=1200T = 1200 K in surroundings at M=300M = 300 K, that is 926.85 °C926.85\,\degree\text{C} and 26.85 °C26.85\,\degree\text{C}. Which quantity has the same value whether both temperatures are written in kelvin or in degrees Celsius?

βœ… Correct! Celsius is kelvin shifted by 273.15273.15, and a shift cancels in a difference: 926.85βˆ’26.85=1200βˆ’300=900926.85 - 26.85 = 1200 - 300 = 900.
❌ A ratio depends on where zero is. 1200/300=41200/300 = 4, but 926.85/26.85β‰ˆ34.5926.85/26.85 \approx 34.5. T1T_1 is the same on every absolute scale, not on Celsius.
❌ A fourth power depends on where zero is. 3004βˆ’12004β‰ˆβˆ’2.07Γ—1012300^4 - 1200^4 \approx -2.07\times10^{12}, but 26.854βˆ’926.854β‰ˆβˆ’7.38Γ—101126.85^4 - 926.85^4 \approx -7.38\times10^{11}.
❌ Only one of them survives. Shifting the zero by 273.15273.15 cancels in a difference, but it changes a ratio and it changes fourth powers.
Show solution

Celsius readings are kelvin readings shifted: TC=Tβˆ’273.15T_C = T - 273.15, MC=Mβˆ’273.15M_C = M - 273.15.

Difference: TCβˆ’MC=(Tβˆ’273.15)βˆ’(Mβˆ’273.15)=Tβˆ’MT_C - M_C = (T - 273.15) - (M - 273.15) = T - M. Here 926.85βˆ’26.85=900=1200βˆ’300926.85 - 26.85 = 900 = 1200 - 300. Same value.

Ratio: 1200/300=41200/300 = 4, while 926.85/26.85β‰ˆ34.5926.85/26.85 \approx 34.5. Different: a ratio is unchanged by a change of unit size (kelvin to Rankine), not by a shift of zero.

Fourth powers: 3004βˆ’12004β‰ˆβˆ’2.07Γ—1012300^4 - 1200^4 \approx -2.07\times10^{12}, while 26.854βˆ’926.854β‰ˆβˆ’7.38Γ—101126.85^4 - 926.85^4 \approx -7.38\times10^{11}. Different.

So the answer is Tβˆ’MT - M. This is why Newton's law, which uses only Mβˆ’TM - T, works in Celsius, while the fourth-power law needs absolute temperatures.

Problem 3 Β· The Initial Cooling Rate

Given: the scaled law dT1dt=k1 (1βˆ’T14)\dfrac{dT_1}{dt} = k_1\,(1 - T_1^4) with k1=0.0027k_1 = 0.0027 per second, surroundings M=300M = 300 K and T(0)=1200T(0) = 1200 K. Find the rates at t=0t = 0.

What is dT1/dtdT_1/dt at t=0t = 0, in per second?

What is dT/dtdT/dt at t=0t = 0, in kelvin per second?

βœ… Correct! dT1/dt=0.0027Γ—(βˆ’255)=βˆ’0.6885dT_1/dt = 0.0027 \times (-255) = -0.6885 per second, and dT/dt=300Γ—(βˆ’0.6885)=βˆ’206.55dT/dt = 300 \times (-0.6885) = -206.55 kelvin per second.
❌ Check the fourth power. T1(0)=1200/300=4T_1(0) = 1200/300 = 4 and T14=256T_1^4 = 256, so the bracket is 1βˆ’256=βˆ’2551 - 256 = -255, not 1βˆ’4=βˆ’31 - 4 = -3.
❌ Check the sign. The body is hotter than its surroundings, T1=4>1T_1 = 4 > 1, so 1βˆ’T14<01 - T_1^4 \lt 0 and the temperature falls.
❌ The 11 is still in the bracket. 1βˆ’T14=1βˆ’256=βˆ’2551 - T_1^4 = 1 - 256 = -255, not βˆ’256-256: the 11 is what the surroundings' term M4M^4 becomes once M4M^4 is factored out.
❌ That is dT1/dtdT_1/dt. Convert back with T=MT1T = MT_1: dTdt=M dT1dt\dfrac{dT}{dt} = M\,\dfrac{dT_1}{dt}.
❌ Multiply by MM, do not divide. T=MT1T = MT_1, so dTdt=M dT1dt=300Γ—(βˆ’0.6885)\dfrac{dT}{dt} = M\,\dfrac{dT_1}{dt} = 300 \times (-0.6885).
❌ That uses 1βˆ’4=βˆ’31 - 4 = -3. The bracket is 1βˆ’44=βˆ’2551 - 4^4 = -255.
Show solution

Step 1: scaled starting value. T1(0)=T(0)/M=1200/300=4T_1(0) = T(0)/M = 1200/300 = 4.

Step 2: scaled rate.

dT1dt=0.0027 (1βˆ’44)=0.0027Γ—(βˆ’255)=βˆ’0.6885Β perΒ second\frac{dT_1}{dt} = 0.0027\,(1 - 4^4) = 0.0027 \times (-255) = -0.6885 \text{ per second}

Step 3: back to kelvin. T=MT1T = MT_1 with MM constant, so

dTdt=M dT1dt=300Γ—(βˆ’0.6885)=βˆ’206.55Β kelvinΒ perΒ second\frac{dT}{dt} = M\,\frac{dT_1}{dt} = 300 \times (-0.6885) = -206.55 \text{ kelvin per second}

Check with the original law. k=k1/M3=0.0027/3003=1Γ—10βˆ’10k = k_1/M^3 = 0.0027/300^3 = 1\times10^{-10}, and k (M4βˆ’T4)=10βˆ’10 (3004βˆ’12004)=10βˆ’10Γ—(βˆ’2.0655Γ—1012)=βˆ’206.55k\,(M^4 - T^4) = 10^{-10}\,(300^4 - 1200^4) = 10^{-10} \times (-2.0655\times10^{12}) = -206.55 βœ“

Problem 4 Β· Scale a Falling Body

Given: a body falling against air resistance, dvdt=gβˆ’c v2\dfrac{dv}{dt} = g - c\,v^2, with gg and cc positive constants. Scale by the terminal speed: v1=v/Vv_1 = v/V with V=g/cV = \sqrt{g/c}. The equation becomes dv1dt=k1 (1βˆ’v12)\dfrac{dv_1}{dt} = k_1\,(1 - v_1^2). Find k1k_1.

βœ… Correct! k1=g/V=gck_1 = g/V = \sqrt{gc}. With gg in metres per second squared and cc in per metre, gc\sqrt{gc} is in per second: inverse time only, like k1=kM3k_1 = kM^3.
❌ That is VV itself. g/c\sqrt{g/c} is a speed (metres per second), but k1k_1 must be in per second because v1v_1 has no units.
❌ The left side carries a factor of VV. v=Vv1v = Vv_1 gives dvdt=V dv1dt\dfrac{dv}{dt} = V\,\dfrac{dv_1}{dt}, so you must divide gg by VV.
❌ Divide by VV, do not multiply. V dv1dt=g (1βˆ’v12)V\,\dfrac{dv_1}{dt} = g\,(1 - v_1^2), so k1=g/Vk_1 = g/V.
Show solution

Define v1=v/Vv_1 = v/V, but substitute v=Vv1v = Vv_1 (VV is constant):

V dv1dt=gβˆ’cV2v12V\,\frac{dv_1}{dt} = g - cV^2v_1^2

Since V2=g/cV^2 = g/c, the term cV2=gcV^2 = g, and the right side factors:

V dv1dt=g (1βˆ’v12)V\,\frac{dv_1}{dt} = g\,(1 - v_1^2)

Divide by VV:

dv1dt=gV (1βˆ’v12),k1=gg/c=gc\frac{dv_1}{dt} = \frac{g}{V}\,(1 - v_1^2), \qquad k_1 = \frac{g}{\sqrt{g/c}} = \sqrt{gc}

Two constants, gg and cc, have been lumped into one, exactly as kk and MM were lumped into k1=kM3k_1 = kM^3.

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