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Lesson 57 — Linear Approximation and Differentials

Tangent line as local approximation. Differential dy. Error estimation via second derivative. Newton-Raphson as iterated linearization.

Used in: 2nd Year of Program (Calculus I) · Equivalent Japanese Math III §4 · Equivalent German Leistungskurs Differentialrechnung · Singapore H2 Math §4.3

L(x)=f(a)+f(a)(xa)L(x) = f(a) + f'(a)(x - a)

Linearization of f at point a: the tangent line to the graph at (a,f(a))(a,\,f(a)) is the best linear approximation of f near a. The error is O((xa)2)O((x-a)^2) — it shrinks much faster than the distance to the base point.

Choose your door

Rigorous notation, full derivation, hypotheses

Rigorous Definition and Error Theory

Linearization

"If ff is differentiable at aa, then L(x)=f(a)+f(a)(xa)L(x) = f(a) + f'(a)(x - a) is called the linearization of ff at aa. The approximation f(x)L(x)f(x) \approx L(x) is called the linear approximation or tangent line approximation of ff at aa." — OpenStax Calculus Vol.1 §4.2

Differential

"We define dxdx and dydy as real variables so that the following equation holds: dy=f(x)dxdy = f'(x)\,dx. The differential dydy is a linear approximation of the actual change Δy\Delta y." — OpenStax Calculus Vol.1 §4.2

Error Estimation via Taylor

Figure: Tangent Line as Local Approximation

xyy = f(x)L(x)aerrorx

The tangent line L(x)L(x) touches the graph of ff at (a,f(a))(a, f(a)). The error (orange segment) between the curve and the line grows with the square of the distance xa|x-a|.

Classic Approximations at a=0a = 0 (Linear Maclaurin Series)

f(x)f(x)L(x)L(x) at a=0a = 0Valid for
exe^x1+x1 + xsmall xx
sinx\sin xxxxx in radians, small
cosx\cos x11small xx
ln(1+x)\ln(1 + x)xxsmall xx
(1+x)n(1 + x)^n1+nx1 + nxsmall xx
1+x\sqrt{1 + x}1+x/21 + x/2small xx
tanx\tan xxxsmall xx
arctanx\arctan xxxsmall xx

Error Propagation

For y=f(x)y = f(x) with uncertainty σx\sigma_x in xx:

σyf(x)σx.\sigma_y \approx |f'(x)|\,\sigma_x.

For functions of several variables y=f(x1,,xn)y = f(x_1, \ldots, x_n) with independent errors σi\sigma_i:

σy2i=1n(fxi)2σi2.\sigma_y^2 \approx \sum_{i=1}^{n} \left(\frac{\partial f}{\partial x_i}\right)^2 \sigma_i^2.

Solved Examples

Exercise list

40 exercises · 10 with worked solution (25%)

22 4 8 4 2
  1. Ex. 57.1

    Approximate 4.1\sqrt{4.1} using linearization at a=4a = 4.

    Select the correct option
    Select an option first
    Show solution
    For f(x)=xf(x) = \sqrt{x} at a=4a = 4: f(4)=2f(4) = 2, f(4)=1/4f'(4) = 1/4. Thus L(4.1)=2+(1/4)(0.1)=2.025L(4.1) = 2 + (1/4)(0.1) = 2.025.
    Show step-by-step (with the why)
    1. Identify the function and base point. f(x)=xf(x) = \sqrt{x}, a=4a = 4. We choose a=4a = 4 because 4=2\sqrt{4} = 2 is exact.
    2. Calculate the derivative at a. f(x)=1/(2x)f'(x) = 1/(2\sqrt{x}), so f(4)=1/(22)=1/4f'(4) = 1/(2 \cdot 2) = 1/4.
    3. Write the linearization. L(x)=2+14(x4)L(x) = 2 + \frac{1}{4}(x - 4).
    4. Evaluate at x = 4.1. L(4.1)=2+14(0.1)=2+0.025=2.025L(4.1) = 2 + \frac{1}{4}(0.1) = 2 + 0.025 = 2.025.

    Rule of thumb: the actual error is 4.1=2.02485\sqrt{4.1} = 2.02485; the linearization error is only 0.00015 — less than 0.01%.

  2. Ex. 57.2

    Approximate 9.06\sqrt{9.06} using linearization at a=9a = 9. Compare with the actual value.

    Show solution
    f(x)=xf(x) = \sqrt{x}, a=9a = 9. f(9)=1/6f'(9) = 1/6. L(9.06)=3+(1/6)(0.06)=3.01L(9.06) = 3 + (1/6)(0.06) = 3.01. Actual value: 9.063.0100\sqrt{9.06} \approx 3.0100.
  3. Ex. 57.3

    Approximate sin(0.05)\sin(0.05) using linearization at a=0a = 0.

    Show solution
    f(x)=sinxf(x) = \sin x, a=0a = 0. f(0)=cos0=1f'(0) = \cos 0 = 1. L(x)=xL(x) = x. Then sin(0.05)0.05\sin(0.05) \approx 0.05. Actual value: 0.049980.04998.
    Show step-by-step (with the why)
    1. Base point. a=0a = 0 because sin(0)=0\sin(0) = 0 and cos(0)=1\cos(0) = 1 are trivial.
    2. Derivative at a. f(x)=cosxf'(x) = \cos x, f(0)=1f'(0) = 1.
    3. Linearization. L(x)=0+1x=xL(x) = 0 + 1 \cdot x = x. The approximation sinxx\sin x \approx x is fundamental in physics (small oscillations).
    4. Evaluation. L(0.05)=0.05L(0.05) = 0.05. Error: 0.050.04998=0.00002|0.05 - 0.04998| = 0.00002.

    Rule of thumb: sinxx\sin x \approx x is valid for x|x| up to about 0.17 rad (10°) with less than 0.5% error.

  4. Ex. 57.4Answer key

    Approximate cos(0.1)\cos(0.1) using linearization at a=0a = 0. Explain why the result is surprisingly inaccurate.

    Show solution
    f(x)=cosxf(x) = \cos x, a=0a = 0. f(0)=sin0=0f'(0) = -\sin 0 = 0. L(x)=1L(x) = 1. Then cos(0.1)1\cos(0.1) \approx 1. Actual value: 0.99500.9950. The 1st-order error is zero here: f(0)=0f'(0) = 0, so the linearization is constant and we need 2nd-order Taylor to improve.
  5. Ex. 57.5

    Approximate e0.03e^{0.03} using linearization at a=0a = 0.

    Show solution
    f(x)=exf(x) = e^x, a=0a = 0. f(0)=1f(0) = 1, f(0)=1f'(0) = 1. L(x)=1+xL(x) = 1 + x. L(0.03)=1.03L(0.03) = 1.03. Actual value: e0.03=1.03045e^{0.03} = 1.03045.
  6. Ex. 57.6

    Approximate ln(1.05)\ln(1.05) using linearization at a=1a = 1.

    Show solution
    f(x)=lnxf(x) = \ln x, a=1a = 1. f(1)=0f(1) = 0, f(1)=1f'(1) = 1. L(x)=x1L(x) = x - 1. L(1.05)=0.05L(1.05) = 0.05. Actual value: ln(1.05)=0.04879\ln(1.05) = 0.04879.
    Show step-by-step (with the why)
    1. Base point. a=1a = 1 because ln(1)=0\ln(1) = 0 is exact and simple.
    2. Derivative at a. f(x)=1/xf'(x) = 1/x, f(1)=1f'(1) = 1.
    3. Linearization. L(x)=0+1(x1)=x1L(x) = 0 + 1 \cdot (x - 1) = x - 1. Equivalently: ln(1+u)u\ln(1 + u) \approx u for small uu.
    4. Evaluation. L(1.05)=1.051=0.05L(1.05) = 1.05 - 1 = 0.05. Error: 0.050.04879=0.00121|0.05 - 0.04879| = 0.00121, or 2.5% error.

    Rule of thumb: the formula ln(1+u)u\ln(1+u) \approx u is widely used in finance to convert compound rates to simple rates when uu is small.

  7. Ex. 57.7

    Approximate (1.02)10(1.02)^{10} using the linearization of (1+x)10(1+x)^{10} at x=0x = 0.

    Show solution
    f(x)=(1+x)10f(x) = (1+x)^{10}, a=0a = 0. f(0)=10f'(0) = 10. L(x)=1+10xL(x) = 1 + 10x. L(0.02)=1.2L(0.02) = 1.2. Actual value: 1.0210=1.21901.02^{10} = 1.2190 — 1.6% error.
  8. Ex. 57.8

    Approximate 27.53\sqrt[3]{27.5} using linearization at a=27a = 27.

    Show solution
    f(x)=x1/3f(x) = x^{1/3}, a=27a = 27. f(27)=3f(27) = 3, f(27)=(1/3)(27)2/3=1/27f'(27) = (1/3)(27)^{-2/3} = 1/27. L(27.5)=3+(1/27)(0.5)=3+0.01853.019L(27.5) = 3 + (1/27)(0.5) = 3 + 0.0185 \approx 3.019. Actual value: 27.51/33.018527.5^{1/3} \approx 3.0185.
    Show step-by-step (with the why)
    1. Base point. a=27a = 27 because 271/3=327^{1/3} = 3 is an exact perfect cube.
    2. Derivative at a. f(x)=13x2/3f'(x) = \frac{1}{3}x^{-2/3}, f(27)=13272/3=1319=127f'(27) = \frac{1}{3} \cdot 27^{-2/3} = \frac{1}{3} \cdot \frac{1}{9} = \frac{1}{27}.
    3. Linearization. L(x)=3+127(x27)L(x) = 3 + \frac{1}{27}(x - 27).
    4. Evaluation. L(27.5)=3+0.5273.0185L(27.5) = 3 + \frac{0.5}{27} \approx 3.0185.

    Curiosity: Newton used this type of calculation to compute roots without a calculator. The method was published in Arithmetica Universalis (1707).

  9. Ex. 57.9

    Write the linearization of f(x)=tanxf(x) = \tan x at a=0a = 0. This linearization is identical to that of sinx\sin x at a=0a = 0 — why?

    Show solution
    f(x)=tanxf(x) = \tan x, a=0a = 0. f(0)=0f(0) = 0, f(x)=sec2xf'(x) = \sec^2 x, f(0)=1f'(0) = 1. Linearization: L(x)=xL(x) = x.
  10. Ex. 57.10

    Write the linearization of f(x)=arctanxf(x) = \arctan x at a=1a = 1.

    Show solution
    f(x)=arctanxf(x) = \arctan x, a=1a = 1. f(1)=π/4f(1) = \pi/4, f(x)=1/(1+x2)f'(x) = 1/(1+x^2), f(1)=1/2f'(1) = 1/2. Linearization: L(x)=π/4+(1/2)(x1)L(x) = \pi/4 + (1/2)(x-1).
  11. Ex. 57.11

    Write the linearization of f(x)=exsinxf(x) = e^x \sin x at a=0a = 0.

    Show solution
    f(x)=exsinxf(x) = e^x \sin x, a=0a = 0. f(0)=0f(0) = 0. Product rule: f(x)=exsinx+excosxf'(x) = e^x \sin x + e^x \cos x. f(0)=0+1=1f'(0) = 0 + 1 = 1. Linearization: L(x)=xL(x) = x.
    Show step-by-step (with the why)
    1. Evaluate f at a = 0. f(0)=e0sin0=10=0f(0) = e^0 \sin 0 = 1 \cdot 0 = 0.
    2. Calculate f'(x) using the product rule. f(x)=(ex)sinx+ex(sinx)=exsinx+excosxf'(x) = (e^x)' \sin x + e^x (\sin x)' = e^x \sin x + e^x \cos x.
    3. Evaluate f'(0). f(0)=e0sin0+e0cos0=0+1=1f'(0) = e^0 \sin 0 + e^0 \cos 0 = 0 + 1 = 1.
    4. Write L(x). L(x)=0+1(x0)=xL(x) = 0 + 1 \cdot (x - 0) = x.

    Note: even though it's a complex product, the linearization is simple — exsinxxe^x \sin x \approx x near zero — because both factors have simple linearizations that multiply like (1+x)xx(1+x) \cdot x \approx x for small xx.

  12. Ex. 57.12

    Approximate 50\sqrt{50} using linearization at a=49a = 49.

    Show solution
    f(x)=xf(x) = \sqrt{x}, a=49a = 49. f(49)=7f(49) = 7, f(49)=1/14f'(49) = 1/14. L(50)=7+(1/14)(1)=7.0714L(50) = 7 + (1/14)(1) = 7.0714. Actual value: 50=7.0711\sqrt{50} = 7.0711.
  13. Ex. 57.13

    Calculate the differential dydy for y=x3y = x^3 at x=2x = 2, dx=0.01dx = 0.01. Compare with the actual change Δy\Delta y.

    Show solution
    y=x3y = x^3. dy=3x2dxdy = 3x^2\,dx. At x=2x = 2, dx=0.01dx = 0.01: dy=3(4)(0.01)=0.12dy = 3(4)(0.01) = 0.12. Actual change: Δy=(2.01)38=0.120601\Delta y = (2.01)^3 - 8 = 0.120601.
    Show step-by-step (with the why)
    1. Write the differential. dy=ddx(x3)dx=3x2dxdy = \frac{d}{dx}(x^3)\,dx = 3x^2\,dx. The differential is the derivative times the change in x.
    2. Substitute the values. x=2x = 2, dx=0.01dx = 0.01: dy=3(2)2(0.01)=340.01=0.12dy = 3(2)^2(0.01) = 3 \cdot 4 \cdot 0.01 = 0.12.
    3. Confirm with the actual change. Δy=(2.01)323=8.1206018=0.120601\Delta y = (2.01)^3 - 2^3 = 8.120601 - 8 = 0.120601. Difference: 0.1206010.12=0.0006010.120601 - 0.12 = 0.000601. Less than 0.5%.

    Rule of thumb: the differential is always a first-order approximation — it ignores all terms of order 2 in dxdx. The difference between Δy\Delta y and dydy is precisely these higher-order terms.

  14. Ex. 57.14

    Calculate the differential dydy for y=exy = e^x at x=0x = 0, dx=0.1dx = 0.1.

    Show solution
    y=exy = e^x. dy=exdxdy = e^x\,dx. At x=0x = 0, dx=0.1dx = 0.1: dy=e00.1=0.1dy = e^0 \cdot 0.1 = 0.1. Actual value: e0.11=0.1052e^{0.1} - 1 = 0.1052.
  15. Ex. 57.15

    Approximate sin(31°)\sin(31°) using the linearization of sin\sin at a=30°a = 30°. Use sin(30°)=0.5\sin(30°) = 0.5 and cos(30°)=3/2\cos(30°) = \sqrt{3}/2.

    Show solution
    f(x)=sinxf(x) = \sin x, a=π/6a = \pi/6 (30°). f(π/6)=cos(π/6)=3/20.866f'(\pi/6) = \cos(\pi/6) = \sqrt{3}/2 \approx 0.866. Difference: 1°=π/1800.017451° = \pi/180 \approx 0.01745 rad. L=0.5+0.866×0.017450.5151L = 0.5 + 0.866 \times 0.01745 \approx 0.5151. Actual value: sin(31°)=0.5150\sin(31°) = 0.5150.
    Show step-by-step (with the why)
    1. Convert angles to radians. a=30°=π/6a = 30° = \pi/6, x=31°=31π/180x = 31° = 31\pi/180.
    2. Calculate x - a. xa=1°=π/1800.01745x - a = 1° = \pi/180 \approx 0.01745 rad.
    3. Derivative at a. f(π/6)=cos(π/6)=3/20.866f'(\pi/6) = \cos(\pi/6) = \sqrt{3}/2 \approx 0.866.
    4. Linearization. L=0.5+0.866×0.017450.5151L = 0.5 + 0.866 \times 0.01745 \approx 0.5151.

    Rule of thumb: when linearizing trigonometric functions at angles given in degrees, ALWAYS convert to radians before applying the derivative. Degrees do not work with the standard derivatives.

  16. Ex. 57.16Answer key

    Approximate cos(59°)\cos(59°) using the linearization of cos\cos at a=60°a = 60°.

    Show solution
    f(x)=cosxf(x) = \cos x, a=π/3a = \pi/3 (60°). f(π/3)=0.5f(\pi/3) = 0.5, f(π/3)=sin(π/3)=3/2f'(\pi/3) = -\sin(\pi/3) = -\sqrt{3}/2. Difference: 59°60°=π/18059° - 60° = -\pi/180. L=0.5+(0.866)(π/180)0.5151L = 0.5 + (-0.866)(-\pi/180) \approx 0.5151.
  17. Ex. 57.17

    What is the linearization of f(x)=1+xf(x) = \sqrt{1 + x} at a=0a = 0?

    Select the correct option
    Select an option first
    Show solution
    f(x)=1+xf(x) = \sqrt{1+x}, a=0a = 0. f(0)=1f(0) = 1, f(x)=1/(21+x)f'(x) = 1/(2\sqrt{1+x}), f(0)=1/2f'(0) = 1/2. L(x)=1+x/2L(x) = 1 + x/2. Distractor B ignores the 1/2 factor in the derivative. Distractor C gets the sign wrong. Distractor D forgets the value at a = 0.
  18. Ex. 57.18

    Approximate 1/4.11/\sqrt{4.1} using linearization at a=4a = 4.

    Show solution
    g(x)=x1/2g(x) = x^{-1/2}, a=4a = 4. g(4)=1/2g(4) = 1/2, g(x)=1/(2x3/2)g'(x) = -1/(2x^{3/2}), g(4)=1/16g'(4) = -1/16. L(4.1)=0.5(1/16)(0.1)=0.50.00625=0.4938L(4.1) = 0.5 - (1/16)(0.1) = 0.5 - 0.00625 = 0.4938.
  19. Ex. 57.19

    Write the linearization of f(x)=lnxf(x) = \ln x at a=ea = e.

    Show solution
    f(x)=lnxf(x) = \ln x, a=ea = e. f(e)=1f(e) = 1, f(e)=1/ef'(e) = 1/e. L(x)=1+(xe)/eL(x) = 1 + (x-e)/e.
  20. Ex. 57.20

    Calculate the absolute error of the linearization of 4.1\sqrt{4.1} at a=4a = 4 by comparing with 4.12.024846\sqrt{4.1} \approx 2.024846. Verify that the error is within the bound M2h2/2M_2 h^2/2.

    Show solution
    Absolute error of the linearization of 4.1\sqrt{4.1}: L(4.1)4.1=2.0252.0248460.000154|L(4.1) - \sqrt{4.1}| = |2.025 - 2.024846| \approx 0.000154. Theoretical bound: M2(0.1)2/2M_2(0.1)^2/2 where M2=1/(443/2)=1/32M_2 = 1/(4 \cdot 4^{3/2}) = 1/32. Bound: (1/32)(0.01)/2=0.000156(1/32)(0.01)/2 = 0.000156. Actual error is within the bound.
  21. Ex. 57.21Answer key

    Perform one iteration of Newton-Raphson to find 5\sqrt{5}, starting from x0=2x_0 = 2.

    Show solution
    f(x)=x25f(x) = x^2 - 5, f(x)=2xf'(x) = 2x. With x0=2x_0 = 2: x1=2(45)/4=2+1/4=2.25x_1 = 2 - (4-5)/4 = 2 + 1/4 = 2.25. Actual value: 5=2.2361\sqrt{5} = 2.2361.
    Show step-by-step (with the why)
    1. Rephrase the problem. Finding 5\sqrt{5} is equivalent to solving x25=0x^2 - 5 = 0. Define f(x)=x25f(x) = x^2 - 5, f(x)=2xf'(x) = 2x.
    2. Apply Newton-Raphson. x1=x0f(x0)/f(x0)=2(45)/(22)=2(1)/4=2+0.25=2.25x_1 = x_0 - f(x_0)/f'(x_0) = 2 - (4 - 5)/(2 \cdot 2) = 2 - (-1)/4 = 2 + 0.25 = 2.25.
    3. Evaluate the error. 52.25=2.23612.25=0.0139|\sqrt{5} - 2.25| = |2.2361 - 2.25| = 0.0139. Starting from 0, we already have 2 correct digits in 1 iteration.

    Rule of thumb: convergence is quadratic — in the next iteration the error would be C(0.014)20.0001\approx C(0.014)^2 \approx 0.0001, giving another 2 decimal places for free.

  22. Ex. 57.22Answer key

    Perform two iterations of Newton-Raphson to solve x32=0x^3 - 2 = 0 with x0=1x_0 = 1.

    Show solution
    f(x)=x32f(x) = x^3 - 2, f(x)=3x2f'(x) = 3x^2. x1=1(1)/3=4/31.333x_1 = 1 - (-1)/3 = 4/3 \approx 1.333. f(4/3)=64/272=10/27f(4/3) = 64/27 - 2 = 10/27. x2=4/3(10/27)/(316/9)=4/310/1441.2637x_2 = 4/3 - (10/27)/(3 \cdot 16/9) = 4/3 - 10/144 \approx 1.2637. Actual: 21/3=1.25992^{1/3} = 1.2599.
  23. Ex. 57.23

    A sphere has radius r=5.0±0.1r = 5.0 \pm 0.1 cm. Estimate the maximum error in the volume V=43πr3V = \frac{4}{3}\pi r^3 using the differential.

    Show solution
    V=(4/3)πr3V = (4/3)\pi r^3. dV=4πr2drdV = 4\pi r^2\,dr. With r=5r = 5, dr=0.1dr = 0.1: dV=4π(25)(0.1)=10π31.4dV = 4\pi(25)(0.1) = 10\pi \approx 31.4 cm³. Relative error: 10π/(500π/3)6%10\pi/(500\pi/3) \approx 6\%.
    Show step-by-step (with the why)
    1. Differential of volume. V=43πr3dV=4πr2drV = \frac{4}{3}\pi r^3 \Rightarrow dV = 4\pi r^2\,dr. Note that 4πr24\pi r^2 is the surface area of the sphere — it makes geometric sense.
    2. Substitute values. r=5r = 5 cm, dr=0.1dr = 0.1 cm: dV=4π(25)(0.1)=10π31.4dV = 4\pi(25)(0.1) = 10\pi \approx 31.4 cm³.
    3. Calculate relative error. V(5)=(4/3)π(125)=500π/3524V(5) = (4/3)\pi(125) = 500\pi/3 \approx 524 cm³. Relative error: 31.4/5246%31.4/524 \approx 6\%.

    Curiosity: the relative error in volume is 3 times the relative error in radius — a direct consequence of Vr3V \propto r^3. General rule: for f(x)=xnf(x) = x^n, the relative error in ff is nn times the relative error in xx.

  24. Ex. 57.24Answer key

    The period of a pendulum is T=2πL/gT = 2\pi\sqrt{L/g}. If the length LL has a relative error of 1%1\%, what is the relative error in TT?

    Show solution
    T=2πL/gT = 2\pi\sqrt{L/g}. dT/T=(1/2)dL/LdT/T = (1/2)\,dL/L. A relative error in LL of 1% results in dT/T=0.5%dT/T = 0.5\%. The error in the period is half the error in the length.
    Show step-by-step (with the why)
    1. Write T as a power of L. T=2πg1/2L1/2T = 2\pi g^{-1/2} L^{1/2}. The exponent of LL is 1/21/2.
    2. Relative error rule. For TL1/2T \propto L^{1/2}, the relative error in TT is 1/21/2 times the relative error in LL.
    3. Apply. dT/T=(1/2)1%=0.5%dT/T = (1/2) \cdot 1\% = 0.5\%.

    Rule of thumb: the exponent appears as a multiplicative factor for relative errors. For a square root (exponent 1/2), the relative error is halved. For squaring (exponent 2), the relative error doubles.

  25. Ex. 57.25Answer key

    For R=V/IR = V/I with independent errors σV\sigma_V and σI\sigma_I, write the error propagation formula for σR\sigma_R using partial derivatives.

    Show solution
    R=V/IR = V/I. R/V=1/I\partial R/\partial V = 1/I, R/I=V/I2\partial R/\partial I = -V/I^2. σR2(σV/I)2+(VσI/I2)2\sigma_R^2 \approx (\sigma_V/I)^2 + (V\sigma_I/I^2)^2, so σR=(σV/I)2+(VσI/I2)2\sigma_R = \sqrt{(\sigma_V/I)^2 + (V\sigma_I/I^2)^2}. The formula propagates errors quadratically for independent errors.
  26. Ex. 57.26

    The area of a circle is A=πr2A = \pi r^2 with r=3.0±0.064r = 3.0 \pm 0.064 cm. Estimate the maximum error in AA using the differential.

    Show solution
    A=πr2A = \pi r^2. dA=2πrdrdA = 2\pi r\,dr. With r=3r = 3, dr=0.064dr = 0.064 (since dA=1.2dr=1.2/(2π3)=0.0637dA = 1.2 \Rightarrow dr = 1.2/(2\pi \cdot 3) = 0.0637): dA=2π(3)(0.0637)1.2dA = 2\pi(3)(0.0637) \approx 1.2 cm².
  27. Ex. 57.27

    Why is the linearization error f(x)L(x)|f(x) - L(x)| said to be O((xa)2)O((x-a)^2)? What theorem supports this?

    Select the correct option
    Select an option first
    Show solution
    From Taylor's theorem with remainder: f(x)L(x)=f(ξ)(xa)2/2f(x) - L(x) = f''(\xi)(x-a)^2/2. The error grows with the square of the distance to the base point. Distractor B confuses it with the growth of the linearization itself. Distractors C and D have no basis in Taylor's theorem.
    Show step-by-step (with the why)
    1. Write Taylor with remainder. f(x)=f(a)+f(a)(xa)+f(ξ)2(xa)2f(x) = f(a) + f'(a)(x-a) + \frac{f''(\xi)}{2}(x-a)^2 for some ξ\xi between aa and xx.
    2. Identify the error. f(x)L(x)=f(ξ)2(xa)2f(x) - L(x) = \frac{f''(\xi)}{2}(x-a)^2. The term is quadratic in (xa)(x-a).
    3. Interpret. If xa|x-a| is halved, the error drops by a factor of 4. If it doubles, the error quadruples.

    Rule of thumb: "2nd order" means the exponent of (xa)(x-a) in the error is 2 — this is why linearization is so useful for small distances but fails for large ones.

  28. Ex. 57.28

    Under what circumstance is the linearization of ff at aa particularly inaccurate, even for xx close to aa? What should be done in such cases?

    Show solution
    When f(a)=0f'(a) = 0, the linearization L(x)=f(a)L(x) = f(a) is constant. The behavior of ff near aa is dominated by curvature (ff''), not slope. Linearization is unnecessarily inaccurate at these points — use 2nd-order Taylor: f(x)f(a)+f(a)(xa)2/2f(x) \approx f(a) + f''(a)(x-a)^2/2.
  29. Ex. 57.29

    Show that sinxx\sin x \approx x is the linearization of sin\sin at a=0a = 0. For what values of xx (in radians) is the error less than 1%?

    Show solution
    f(x)=sinxf(x) = \sin x, a=0a = 0: f(0)=cos(0)=1f'(0) = \cos(0) = 1. Linearization: L(x)=xL(x) = x. The approximation sinxx\sin x \approx x has less than 1% error for x<0.17|x| < 0.17 rad (about 10°). The error bound is x2/2|x|^2/2; for 1% of sinxx\sin x \approx x, solve x2/2<0.01xx^2/2 < 0.01 x, i.e., x<0.02x < 0.02 — but the practical engineering criterion is up to 14°.
  30. Ex. 57.30

    What is the relationship between Δy\Delta y (actual change) and dydy (differential)?

    Select the correct option
    Select an option first
    Show solution
    Δy=f(x+Δx)f(x)\Delta y = f(x + \Delta x) - f(x) is the actual change. dy=f(x)Δxdy = f'(x)\,\Delta x is the linear change. The difference Δydy=O(Δx2)\Delta y - dy = O(\Delta x^2) tends to zero faster than Δx\Delta x. Distractor B ignores the 2nd-order error. Distractor C is correct for affine functions but the question is about general equality. Distractor D is false: for concave functions Δy<dy\Delta y < dy.
  31. Ex. 57.31Answer key

    Explain where the Newton-Raphson formula xn+1=xnf(xn)/f(xn)x_{n+1} = x_n - f(x_n)/f'(x_n) comes from in terms of linearization.

    Show solution
    Newton-Raphson: xn+1=xnf(xn)/f(xn)x_{n+1} = x_n - f(x_n)/f'(x_n). Origin: we zero the linearization of ff at xnx_n. The tangent line is L(x)=f(xn)+f(xn)(xxn)L(x) = f(x_n) + f'(x_n)(x - x_n); setting to zero: x=xnf(xn)/f(xn)x = x_n - f(x_n)/f'(x_n). Each iteration is a local linearization whose zero becomes the next estimate.
  32. Ex. 57.32

    Use linearization to approximate (1.002)30(1.002)^{30}.

    Show solution
    f(x)=(1+x)30f(x) = (1+x)^{30}, a=0a = 0. f(0)=30f'(0) = 30. L(0.002)=1+30(0.002)=1.06L(0.002) = 1 + 30(0.002) = 1.06. Actual value: (1.002)301.0618(1.002)^{30} \approx 1.0618.
  33. Ex. 57.33Answer key

    The side of a cube is measured with a relative error of 1%1\%. What is the relative error in the volume V=s3V = s^3?

    Show solution
    V=s3V = s^3. dV=3s2dsdV = 3s^2\,ds. Relative error in VV: dV/V=3ds/s=3×1%=3%dV/V = 3\,ds/s = 3 \times 1\% = 3\%. The exponent 3 appears as a multiplicative factor.
    Show step-by-step (with the why)
    1. Differential of volume. V=s3dV=3s2dsV = s^3 \Rightarrow dV = 3s^2\,ds.
    2. Relative error. Divide dVdV by VV: dV/V=3s2ds/s3=3(ds/s)dV/V = 3s^2 ds / s^3 = 3(ds/s).
    3. Substitute. ds/s=1%dV/V=3×1%=3%ds/s = 1\% \Rightarrow dV/V = 3 \times 1\% = 3\%.

    Rule of thumb: for any f(x)=xnf(x) = x^n, the relative error in ff is nn times the relative error in xx. This follows directly from the power rule applied to the differential.

  34. Ex. 57.34

    Write the linearization of g(x)=1/1+xg(x) = 1/\sqrt{1+x} at a=0a = 0.

    Show solution
    g(x)=(1+x)1/2g(x) = (1+x)^{-1/2}, a=0a = 0. g(x)=12(1+x)3/2g'(x) = -\frac{1}{2}(1+x)^{-3/2}, g(0)=1/2g'(0) = -1/2. L(x)=1x/2L(x) = 1 - x/2. This is the binomial approximation for exponent 1/2-1/2.
  35. Ex. 57.35Answer key

    Calculate the absolute and relative error of the linearization of exe^x at a=0a = 0 when approximating e1=ee^1 = e. Is the result surprising? Explain.

    Show solution
    See the referenced source for the detailed solution.
    Show step-by-step (with the why)
    1. Calculate L(1). L(x)=1+xL(x) = 1 + x; L(1)=2L(1) = 2.
    2. Actual value. e1=e2.71828e^1 = e \approx 2.71828.
    3. Absolute error. e2=0.71828|e - 2| = 0.71828.
    4. Relative error. 0.71828/2.7182826.4%0.71828/2.71828 \approx 26.4\%. Large: the point x=1x = 1 is far from a=0a = 0.

    Note: to improve for x=1x = 1, use base point a=1a = 1 and target e0.1e^{0.1} — or use a higher-degree Taylor expansion.

  36. Ex. 57.36

    Newton-Raphson fails when f(xn)=0f'(x_n) = 0. Explain geometrically and give an example function where this occurs.

    Show solution
    If f(xn)=0f'(x_n) = 0, the tangent line at xnx_n is horizontal and never crosses the xx-axis. Newton-Raphson attempts to divide by f(xn)=0f'(x_n) = 0: undefined. Example: f(x)=x2f(x) = x^2 with root at x=0x^* = 0 and f(0)=0f'(0) = 0. Newton oscillates or diverges in this case — the horizontal tangent provides no directional information.
  37. Ex. 57.37Answer key

    Derive the error bound f(x)L(x)M22(xa)2|f(x) - L(x)| \leq \frac{M_2}{2}(x-a)^2 from Taylor's theorem with the Lagrange remainder.

    Show solution
    See the referenced source for the detailed solution.
  38. Ex. 57.38

    Volume of a cylinder: V=πr2hV = \pi r^2 h. With r=5.0±0.1r = 5.0 \pm 0.1 cm and h=10.0±0.2h = 10.0 \pm 0.2 cm, estimate the maximum error in VV using the total differential.

    Show solution
    V=πr2hV = \pi r^2 h. Total differential: dV=2πrhdr+πr2dhdV = 2\pi r h\,dr + \pi r^2\,dh. With r=5r = 5, h=10h = 10, dr=0.1dr = 0.1, dh=0.2dh = 0.2: dV=2π(5)(10)(0.1)+π(25)(0.2)=10π+5π=15π47.1dV = 2\pi(5)(10)(0.1) + \pi(25)(0.2) = 10\pi + 5\pi = 15\pi \approx 47.1 cm³.
    Show step-by-step (with the why)
    1. Total differential. For functions of two variables: dV=Vrdr+VhdhdV = \frac{\partial V}{\partial r}\,dr + \frac{\partial V}{\partial h}\,dh.
    2. Partial derivatives. V/r=2πrh\partial V/\partial r = 2\pi r h, V/h=πr2\partial V/\partial h = \pi r^2.
    3. Substitute. dV=2π(5)(10)(0.1)+π(25)(0.2)=10π+5π=15π47.1dV = 2\pi(5)(10)(0.1) + \pi(25)(0.2) = 10\pi + 5\pi = 15\pi \approx 47.1 cm³.

    Rule of thumb: the total differential generalizes the one-dimensional differential to functions of multiple variables — each variable contributes its partial derivative times its change.

  39. Ex. 57.39

    Prove that L(x)=f(a)+f(a)(xa)L(x) = f(a) + f'(a)(x-a) is the degree 1 Taylor polynomial of ff at aa, and that the error is O((xa)2)O((x-a)^2).

    Show solution
    Full Taylor series: f(x)=k=0f(k)(a)k!(xa)kf(x) = \sum_{k=0}^{\infty} \frac{f^{(k)}(a)}{k!}(x-a)^k. Truncating at k=1k = 1: P1(x)=f(a)+f(a)(xa)=L(x)P_1(x) = f(a) + f'(a)(x-a) = L(x). Linearization is the degree 1 Taylor polynomial. The error f(x)P1(x)=k=2f(k)(a)k!(xa)kf(x) - P_1(x) = \sum_{k=2}^{\infty} \frac{f^{(k)}(a)}{k!}(x-a)^k has dominant term O((xa)2)O((x-a)^2).
  40. Ex. 57.40

    Prove that Newton-Raphson has quadratic convergence: if en=xnxe_n = x_n - x^* is the error at the nn-th iteration and f(x)0f'(x^*) \neq 0, then en+1Cen2|e_{n+1}| \leq C\,|e_n|^2 for some constant C>0C > 0.

    Show solution
    Let xx^* be the exact root (f(x)=0f(x^*) = 0), en=xnxe_n = x_n - x^*. Taylor at xx^*: f(xn)=f(x)en+f(ξn)en2/2f(x_n) = f'(x^*) e_n + f''(\xi_n) e_n^2/2. Newton iteration: en+1=xn+1x=xnf(xn)/f(xn)xe_{n+1} = x_{n+1} - x^* = x_n - f(x_n)/f'(x_n) - x^*. Expanding and simplifying: en+1f(x)en2/(2f(x))e_{n+1} \approx -f''(x^*) e_n^2 / (2f'(x^*)). Thus en+1Cen2|e_{n+1}| \leq C|e_n|^2 with C=f(x)/(2f(x))C = |f''(x^*)| / (2|f'(x^*)|). Quadratic convergence.

Sources

  • Active Calculus — Boelkins · 2024 · §1.8 "The tangent line approximation" · CC-BY-NC-SA. Primary source. Exercises 57.1–57.2, 57.5, 57.7, 57.11–57.12, 57.15, 57.20–57.21, 57.27, 57.29, 57.31, 57.35, 57.37, 57.39–57.40.
  • Calculus Volume 1 — OpenStax · 2016 · §4.2 "Linear Approximations and Differentials" · CC-BY-NC-SA. Exercises 57.3–57.4, 57.6, 57.13–57.14, 57.17–57.19, 57.23, 57.25, 57.28, 57.30, 57.33.
  • APEX Calculus — Hartman et al. · 2024 · v5 · §4.4 "Differentials" · CC-BY-NC. Exercises 57.8–57.10, 57.16, 57.22, 57.24, 57.26, 57.31, 57.34, 57.36, 57.38.

Updated on 2024-05-15 · Author(s): Clube da Matemática

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