Find the increment Δ V of the volume of a sphere when
Find the increment $\Delta V$ of the volume of a sphere when the radius changes by $\Delta r$. Compute $\Delta V$ and $dV$ for $r = 3$ with 1° $\Delta r = 0.5$; 2° $\Delta r = 0.1$; 3° $\Delta r = 0.01$, and determine the error made in replacing the increment by the differential.
Explanation of Method
A cubic law, so the remainder now has two terms.
Step 1: The exact increment
With $V = \dfrac{4}{3}\pi r^{3}$ and $\bigl(r+\Delta r\bigr)^{3} = r^{3}+3r^{2}\Delta r+3r(\Delta r)^{2}+(\Delta r)^{3}$: \[\Delta V = \frac{4\pi}{3}\Bigl[3r^{2}\Delta r+3r(\Delta r)^{2}+(\Delta r)^{3}\Bigr] = 4\pi r^{2}\Delta r+4\pi r(\Delta r)^{2}+\frac{4\pi}{3}(\Delta r)^{3}.\]
Step 2: The differential
\[ dV = V'_{r}\,\Delta r = 4\pi r^{2}\,\Delta r. \]
This is the surface area times the thickness — the volume of a thin spherical shell, which is exactly what the linear term should be.
Step 3: The error in closed form
\[ \bigl|\Delta V-dV\bigr| = 4\pi r(\Delta r)^{2}+\frac{4\pi}{3}(\Delta r)^{3} = \frac{4\pi(\Delta r)^{2}\bigl(3r+\Delta r\bigr)}{3}. \]
At $r = 3$ the formulas become
\[ \Delta V = 36\pi\,\Delta r+12\pi(\Delta r)^{2}+\frac{4\pi}{3}(\Delta r)^{3}, \qquad dV = 36\pi\,\Delta r, \qquad \bigl|\Delta V-dV\bigr| = \frac{4\pi(\Delta r)^{2}\bigl(9+\Delta r\bigr)}{3}. \]
Step 4: Case 1°: $\Delta r = 0.5$
\[ \Delta V = 18\pi+3\pi+\frac{\pi}{6} = \frac{127\pi}{6} \approx 66.497, \qquad dV = 18\pi \approx 56.549, \]
\[ \bigl|\Delta V-dV\bigr| = \frac{19\pi}{6} \approx 9.948, \qquad \frac{19}{127} \approx 14.96\%. \]
Step 5: Case 2°: $\Delta r = 0.1$
\[ \Delta V = 3.6\pi+0.12\pi+0.0013\overline{3}\pi \approx 11.6909, \qquad dV = 3.6\pi \approx 11.3097, \]
\[ \bigl|\Delta V-dV\bigr| \approx 0.3812, \qquad \frac{0.3812}{11.6909} \approx 3.26\%. \]
Step 6: Case 3°: $\Delta r = 0.01$
\[ \Delta V \approx 1.13475, \qquad dV = 0.36\pi \approx 1.13097, \]
\[ \bigl|\Delta V-dV\bigr| = \frac{4\pi(0.01)^{2}(9.01)}{3} \approx 0.003774, \qquad \frac{0.003774}{1.13475} \approx 0.33\%. \]
Step 7: Summary
\[\begin{array}{c|c|c|c|c} \Delta r & \Delta V & dV & \text{absolute} & \text{relative} \\ \hline 0.5 & 66.497 & 56.549 & 9.948 & 14.96\% \\ 0.1 & 11.6909 & 11.3097 & 0.3812 & 3.26\% \\ 0.01 & 1.13475 & 1.13097 & 0.003774 & 0.33\% \end{array}\]
\[\text{Direct check, } \Delta r = 0.5:\ \frac{4\pi}{3}\bigl(3.5^{3}-3^{3}\bigr) = \frac{4\pi}{3}\bigl(42.875-27\bigr) = \frac{4\pi\cdot 15.875}{3} \approx 66.497 \;\;\checkmark\]
\[\text{Relative error } \approx \frac{\Delta r}{r} \text{ for small } \Delta r:\ \frac{0.01}{3} = 0.33\% \;\;\checkmark\]
Result
Final answer:
\[\boxed{\,dV = 4\pi r^{2}\,\Delta r, \qquad \bigl|\Delta V-dV\bigr| = \dfrac{4\pi\bigl(\Delta r\bigr)^{2}\bigl(3r+\Delta r\bigr)}{3}\,}\]
Remark
Remark. To leading order the relative error is $\dfrac{4\pi r(\Delta r)^{2}}{4\pi r^{2}\Delta r} = \dfrac{\Delta r}{r}$ — for a cubic law it is the full relative change of the radius, against only half of it for the quadratic law of Problem 245. The higher the power, the more sharply the linear estimate degrades.