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Section A: Long Answer Questions

Attempt all questions.

5 questions
1long10 marks

The cross-sectional design of an open channel leads to the nonlinear equation

f(x)=x3x11=0f(x) = x^3 - x - 11 = 0

(a) Show that a real root lies in the interval [2,3][2, 3] and perform two iterations of the bisection method to bracket the root. (b) Taking x0=2.5x_0 = 2.5, apply the Newton-Raphson method until two successive iterates agree to four decimal places. (c) State the order of convergence of the Newton-Raphson method and explain one situation in which it may fail.

(a) Existence of a root and bisection (3 marks)

f(x)=x3x11f(x)=x^3-x-11.

f(2)=8211=5<0f(2)=8-2-11=-5<0, and f(3)=27311=13>0f(3)=27-3-11=13>0.

Since ff is continuous and f(2)f(3)<0f(2)\cdot f(3)<0, by the Intermediate Value Theorem a real root lies in [2,3][2,3].

Iteration 1: xm=2+32=2.5x_m=\tfrac{2+3}{2}=2.5, f(2.5)=15.6252.511=2.125>0f(2.5)=15.625-2.5-11=2.125>0. Root lies in [2,2.5][2,\,2.5].

Iteration 2: xm=2+2.52=2.25x_m=\tfrac{2+2.5}{2}=2.25, f(2.25)=11.390632.2511=1.85937<0f(2.25)=11.39063-2.25-11=-1.85937<0. Root lies in [2.25,2.5][2.25,\,2.5].

(b) Newton-Raphson (5 marks)

f(x)=3x21f'(x)=3x^2-1, so xn+1=xnxn3xn113xn21x_{n+1}=x_n-\dfrac{x_n^3-x_n-11}{3x_n^2-1}.

nnxnx_nf(xn)f(x_n)xn+1x_{n+1}
02.5000002.1250002.380282
12.3802820.1057782.373669
22.3736690.0003122.373650
32.3736500.0000002.373650

Iterates x2=2.3737x_2=2.3737 and x3=2.3737x_3=2.3737 agree to four decimals.

Root 2.3737\approx \mathbf{2.3737}.

(c) Convergence (2 marks)

Newton-Raphson has quadratic (second-order) convergence near a simple root: the error satisfies en+1Cen2e_{n+1}\approx C\,e_n^2. It may fail when f(xn)=0f'(x_n)=0 (or is very small), giving division by zero / divergence; it can also overshoot or cycle if the initial guess is far from the root.

roots-of-equationsnewton-raphsonconvergence
2long8 marks

The settlement yy (in mm) of a soil sample measured at equally spaced load steps xx is tabulated below.

xx0123
yy121134

(a) Construct the forward difference table. (b) Using Newton's forward difference interpolation formula, estimate the settlement at x=1.5x = 1.5. (c) Obtain the interpolating polynomial y(x)y(x) in expanded form.

(a) Forward difference table (3 marks)

xxyyΔy\Delta yΔ2y\Delta^2 yΔ3y\Delta^3 y
01186
12914
21123
334

(b) Newton forward interpolation at x=1.5x=1.5 (3 marks)

Here x0=0x_0=0, h=1h=1, p=xx0h=1.501=1.5p=\dfrac{x-x_0}{h}=\dfrac{1.5-0}{1}=1.5.

y=y0+pΔy0+p(p1)2!Δ2y0+p(p1)(p2)3!Δ3y0y = y_0 + p\,\Delta y_0 + \frac{p(p-1)}{2!}\Delta^2 y_0 + \frac{p(p-1)(p-2)}{3!}\Delta^3 y_0 y=1+(1.5)(1)+(1.5)(0.5)2(8)+(1.5)(0.5)(0.5)6(6)y = 1 + (1.5)(1) + \frac{(1.5)(0.5)}{2}(8) + \frac{(1.5)(0.5)(-0.5)}{6}(6) y=1+1.5+3.00.375=5.125y = 1 + 1.5 + 3.0 - 0.375 = 5.125

Settlement at x=1.5x=1.5 is 5.125 mm\mathbf{5.125\ \text{mm}}.

(c) Interpolating polynomial (2 marks)

With general p=xp=x (since h=1h=1, x0=0x_0=0):

y=1+x+x(x1)2(8)+x(x1)(x2)6(6)y = 1 + x + \frac{x(x-1)}{2}(8) + \frac{x(x-1)(x-2)}{6}(6) =1+x+4x(x1)+x(x1)(x2)= 1 + x + 4x(x-1) + x(x-1)(x-2) =1+x+4x24x+(x33x2+2x)= 1 + x + 4x^2 - 4x + (x^3 - 3x^2 + 2x) y(x)=x3+x2x+1\boxed{y(x) = x^3 + x^2 - x + 1}

Check: y(2)=8+42+1=11y(2)=8+4-2+1=11 ✓, y(3)=27+93+1=34y(3)=27+9-3+1=34 ✓.

interpolationnewton-forward-differencefinite-differences
3long8 marks

A structural analysis problem yields the system of linear equations

4xy+z=8,2x+5y+2z=3,x+2y+4z=11.4x - y + z = 8,\qquad 2x + 5y + 2z = 3,\qquad x + 2y + 4z = 11.

(a) Verify that the coefficient matrix is diagonally dominant and write the Gauss-Seidel iteration formulae. (b) Starting from (x,y,z)=(0,0,0)(x,y,z)=(0,0,0), perform iterations until each variable changes by less than 0.010.01 in absolute value. (c) State the converged solution.

(a) Diagonal dominance and iteration formulae (2 marks)

Row 1: 41+1=2|4| \ge |-1|+|1| = 2 ✓ Row 2: 52+2=4|5| \ge |2|+|2| = 4 ✓ Row 3: 41+2=3|4| \ge |1|+|2| = 3

The matrix is diagonally dominant, so Gauss-Seidel converges. Rearranging each equation for its diagonal variable:

x=8+yz4,y=32x2z5,z=11x2y4.x = \frac{8 + y - z}{4},\quad y = \frac{3 - 2x - 2z}{5},\quad z = \frac{11 - x - 2y}{4}.

(b) Iterations (5 marks) — each new value uses the most recent estimates.

Iterxxyyzz
12.00000-0.200002.35000
21.36250-0.885002.85187
31.06578-0.967062.96709
41.01646-0.993422.99259
51.00350-0.998442.99834
61.00080-0.999662.99963
71.00018-0.999922.99992

From iteration 6 to 7 the changes are Δx=0.00062|{\Delta x}|=0.00062, Δy=0.00026|{\Delta y}|=0.00026, Δz=0.00029|{\Delta z}|=0.00029, all <0.01<0.01. Stop.

(c) Solution (1 mark)

x1.000,y1.000,z3.000\boxed{x \approx 1.000,\quad y \approx -1.000,\quad z \approx 3.000}

Exact solution (1,1,3)(1,-1,3) confirms the result.

linear-systemsgauss-seideldiagonal-dominance
4long8 marks

The rate of change of water depth yy over distance xx in a flow model is governed by the initial value problem

dydx=x+y,y(0)=1.\frac{dy}{dx} = x + y,\qquad y(0) = 1.

Using the fourth-order Runge-Kutta (RK4) method with step size h=0.1h = 0.1, compute y(0.1)y(0.1) and y(0.2)y(0.2). Compare y(0.2)y(0.2) with the exact solution y=2exx1y = 2e^{x} - x - 1 and find the absolute error.

RK4 formulae: with f(x,y)=x+yf(x,y)=x+y,

k1=hf(xn,yn),  k2=hf ⁣(xn+h2,yn+k12),  k3=hf ⁣(xn+h2,yn+k22),  k4=hf(xn+h,yn+k3),k_1=hf(x_n,y_n),\;k_2=hf\!\left(x_n+\tfrac{h}{2},y_n+\tfrac{k_1}{2}\right),\;k_3=hf\!\left(x_n+\tfrac{h}{2},y_n+\tfrac{k_2}{2}\right),\;k_4=hf(x_n+h,y_n+k_3), yn+1=yn+16(k1+2k2+2k3+k4).y_{n+1}=y_n+\tfrac{1}{6}(k_1+2k_2+2k_3+k_4).

Step 1: x0=0,  y0=1,  h=0.1x_0=0,\;y_0=1,\;h=0.1 (3 marks)

  • k1=0.1(0+1)=0.100000k_1 = 0.1\,(0+1) = 0.100000
  • k2=0.1(0.05+1.05)=0.110000k_2 = 0.1\,(0.05 + 1.05) = 0.110000
  • k3=0.1(0.05+1.055)=0.110500k_3 = 0.1\,(0.05 + 1.055) = 0.110500
  • k4=0.1(0.1+1.1105)=0.121050k_4 = 0.1\,(0.1 + 1.1105) = 0.121050
y1=1+16(0.1+2(0.11)+2(0.1105)+0.12105)=1+0.110342=1.110342y_1 = 1 + \tfrac{1}{6}(0.1 + 2(0.11) + 2(0.1105) + 0.12105) = 1 + 0.110342 = 1.110342

y(0.1)1.110342y(0.1) \approx \mathbf{1.110342}.

Step 2: x1=0.1,  y1=1.110342x_1=0.1,\;y_1=1.110342 (3 marks)

  • k1=0.1(0.1+1.110342)=0.121034k_1 = 0.1\,(0.1 + 1.110342) = 0.121034
  • k2=0.1(0.15+1.170859)=0.132086k_2 = 0.1\,(0.15 + 1.170859) = 0.132086
  • k3=0.1(0.15+1.176385)=0.132639k_3 = 0.1\,(0.15 + 1.176385) = 0.132639
  • k4=0.1(0.2+1.242981)=0.144298k_4 = 0.1\,(0.2 + 1.242981) = 0.144298
y2=1.110342+16(0.121034+2(0.132086)+2(0.132639)+0.144298)=1.110342+0.132464=1.242806y_2 = 1.110342 + \tfrac{1}{6}(0.121034 + 2(0.132086) + 2(0.132639) + 0.144298) = 1.110342 + 0.132464 = 1.242806

y(0.2)1.242806y(0.2) \approx \mathbf{1.242806}.

Comparison with exact (2 marks)

Exact: y(0.2)=2e0.20.21=2(1.221403)1.2=1.242806y(0.2) = 2e^{0.2} - 0.2 - 1 = 2(1.221403) - 1.2 = 1.242806.

Absolute error =1.2428061.2428061×106= |1.242806 - 1.242806| \approx \mathbf{1\times10^{-6}}, showing RK4's high accuracy.

oderunge-kuttainitial-value-problem
5long8 marks

The steady-state temperature distribution over a thin square plate is governed by Laplace's equation 2u=0\nabla^2 u = 0. The plate is discretised by a uniform grid with four interior nodes u1,u2,u3,u4u_1, u_2, u_3, u_4 arranged as a 2×22\times2 block. The boundary values are: top edge =100= 100, all other edges =0= 0 (the four interior nodes share boundary neighbours symmetrically as shown).

        100   100
         |     |
   0 -- u1 -- u2 -- 0
         |     |
   0 -- u3 -- u4 -- 0
         |     |
         0     0

Using the five-point finite-difference (standard) formula ui,j=14(uleft+uright+utop+ubottom)u_{i,j}=\tfrac{1}{4}(u_{\text{left}}+u_{\text{right}}+u_{\text{top}}+u_{\text{bottom}}), set up the four linear equations and solve them exactly to find u1,u2,u3,u4u_1, u_2, u_3, u_4.

Five-point formula (2 marks): each interior node equals one-quarter of the sum of its four neighbours.

Neighbour bookkeeping (left/right/top/bottom):

  • u1u_1: left =0=0, right =u2=u_2, top =100=100, bottom =u3=u_3
  • u2u_2: left =u1=u_1, right =0=0, top =100=100, bottom =u4=u_4
  • u3u_3: left =0=0, right =u4=u_4, top =u1=u_1, bottom =0=0
  • u4u_4: left =u3=u_3, right =0=0, top =u2=u_2, bottom =0=0

Equations (2 marks):

4u1=100+u2+u3(1)4u_1 = 100 + u_2 + u_3 \quad(1) 4u2=100+u1+u4(2)4u_2 = 100 + u_1 + u_4 \quad(2) 4u3=u1+u4(3)4u_3 = u_1 + u_4 \quad(3) 4u4=u2+u3(4)4u_4 = u_2 + u_3 \quad(4)

Exact solution (4 marks): By symmetry of the boundary (left-right mirror), u1=u2u_1=u_2 and u3=u4u_3=u_4. Let u1=u2=au_1=u_2=a, u3=u4=bu_3=u_4=b.

From (1): 4a=100+a+b3ab=100.4a = 100 + a + b \Rightarrow 3a - b = 100. From (3): 4b=a+b3b=aa=3b.4b = a + b \Rightarrow 3b = a \Rightarrow a = 3b.

Substitute: 3(3b)b=1008b=100b=12.5,  a=37.5.3(3b) - b = 100 \Rightarrow 8b = 100 \Rightarrow b = 12.5,\; a = 37.5.

u1=u2=37.5,u3=u4=12.5\boxed{u_1 = u_2 = 37.5,\qquad u_3 = u_4 = 12.5}

Check (2): 4(37.5)=1504(37.5)=150 and 100+37.5+12.5=150100+37.5+12.5=150 ✓. The nodes nearer the hot top edge are hotter, as physically expected.

pdelaplace-equationfinite-difference
B

Section B: Short Answer Questions

Attempt all questions.

6 questions
6short6 marks

Evaluate 01dx1+x2\displaystyle\int_0^1 \frac{dx}{1+x^2} using Simpson's 1/31/3 rule with n=4n = 4 subintervals. Compare your result with the exact value and compute the absolute error.

Setup (2 marks): a=0a=0, b=1b=1, n=4n=4, h=104=0.25h=\dfrac{1-0}{4}=0.25, f(x)=11+x2f(x)=\dfrac{1}{1+x^2}.

iixix_if(xi)f(x_i)
00.001.000000
10.250.941176
20.500.800000
30.750.640000
41.000.500000

Simpson's 1/3 rule (3 marks):

I=h3[f0+f4+4(f1+f3)+2f2]I = \frac{h}{3}\Big[f_0 + f_4 + 4(f_1+f_3) + 2f_2\Big] =0.253[1.0+0.5+4(0.941176+0.640000)+2(0.8)]= \frac{0.25}{3}\Big[1.0 + 0.5 + 4(0.941176 + 0.640000) + 2(0.8)\Big] =0.253[1.5+4(1.581176)+1.6]=0.253(9.424706)=0.785392= \frac{0.25}{3}\big[1.5 + 4(1.581176) + 1.6\big] = \frac{0.25}{3}(9.424706) = 0.785392

I0.785392I \approx \mathbf{0.785392}.

Comparison (1 mark): Exact value =arctan(1)=π4=0.785398=\arctan(1)=\dfrac{\pi}{4}=0.785398.

Absolute error =0.7853980.785392=6×106= |0.785398 - 0.785392| = \mathbf{6\times10^{-6}}.

integrationsimpson-rulecivil-application
7short6 marks

A vehicle's velocity vv (m/s) is recorded every 2 seconds during a test run:

tt (s)0246810
vv (m/s)01225333840

Using the trapezoidal rule, estimate the total distance travelled in the 10-second interval. State the formula and one source of error in the estimate.

Trapezoidal rule (2 marks): distance =010vdth2[v0+vn+2i=1n1vi]= \displaystyle\int_0^{10} v\,dt \approx \frac{h}{2}\Big[v_0 + v_n + 2\sum_{i=1}^{n-1} v_i\Big], with h=2h=2 s, n=5n=5.

Computation (3 marks):

Distance=22[(0+40)+2(12+25+33+38)]\text{Distance} = \frac{2}{2}\Big[(0 + 40) + 2(12 + 25 + 33 + 38)\Big] =1×[40+2(108)]=40+216=256= 1\times\big[40 + 2(108)\big] = 40 + 216 = 256

Total distance 256 m\approx \mathbf{256\ \text{m}}.

Source of error (1 mark): The trapezoidal rule replaces the true velocity curve by straight-line segments between data points. Where the curve is concave (as during acceleration here), the chords lie below the curve, so the estimate is slightly lower than the true distance; the error is O(h2)O(h^2) and shrinks as the sampling interval hh decreases.

integrationtrapezoidal-rulekinematics
8short6 marks

Using Lagrange's interpolation formula, estimate f(2)f(2) from the following data:

xx134
f(x)f(x)12764

Lagrange formula (2 marks): for three points,

f(x)=if(xi)Li(x),Li(x)=jixxjxixj.f(x) = \sum_{i} f(x_i)\, L_i(x),\qquad L_i(x)=\prod_{j\ne i}\frac{x-x_j}{x_i-x_j}.

Data: (x0,f0)=(1,1)(x_0,f_0)=(1,1), (x1,f1)=(3,27)(x_1,f_1)=(3,27), (x2,f2)=(4,64)(x_2,f_2)=(4,64). Evaluate at x=2x=2.

Basis polynomials at x=2x=2 (3 marks):

L0=(23)(24)(13)(14)=(1)(2)(2)(3)=26=0.33333L_0 = \frac{(2-3)(2-4)}{(1-3)(1-4)} = \frac{(-1)(-2)}{(-2)(-3)} = \frac{2}{6} = 0.33333 L1=(21)(24)(31)(34)=(1)(2)(2)(1)=22=1.00000L_1 = \frac{(2-1)(2-4)}{(3-1)(3-4)} = \frac{(1)(-2)}{(2)(-1)} = \frac{-2}{-2} = 1.00000 L2=(21)(23)(41)(43)=(1)(1)(3)(1)=13=0.33333L_2 = \frac{(2-1)(2-3)}{(4-1)(4-3)} = \frac{(1)(-1)}{(3)(1)} = \frac{-1}{3} = -0.33333

Interpolated value (1 mark):

f(2)=1(0.33333)+27(1.00000)+64(0.33333)f(2) = 1(0.33333) + 27(1.00000) + 64(-0.33333) =0.33333+2721.33333=6.0= 0.33333 + 27 - 21.33333 = 6.0

f(2)6f(2) \approx \mathbf{6}. (Consistent with the cubic trend x3x^3 giving 88; the quadratic Lagrange fit through three points yields 66.)

interpolationlagrangecurve-fitting
9short5 marks

Given the function values f(1.0)=2.7183f(1.0)=2.7183, f(1.1)=3.0042f(1.1)=3.0042, f(1.2)=3.3201f(1.2)=3.3201 (which are values of exe^x), use the appropriate finite-difference formulae to estimate f(1.1)f'(1.1) and f(1.1)f''(1.1) with h=0.1h=0.1. Compare f(1.1)f'(1.1) with the exact value e1.1=3.0042e^{1.1}=3.0042.

Central difference for first derivative (2 marks):

f(x)f(x+h)f(xh)2hf'(x) \approx \frac{f(x+h)-f(x-h)}{2h} f(1.1)f(1.2)f(1.0)2(0.1)=3.32012.71830.2=0.60180.2=3.0090f'(1.1) \approx \frac{f(1.2)-f(1.0)}{2(0.1)} = \frac{3.3201 - 2.7183}{0.2} = \frac{0.6018}{0.2} = 3.0090

f(1.1)3.0090f'(1.1) \approx \mathbf{3.0090}.

Central difference for second derivative (2 marks):

f(x)f(x+h)2f(x)+f(xh)h2f''(x) \approx \frac{f(x+h)-2f(x)+f(x-h)}{h^2} f(1.1)3.32012(3.0042)+2.7183(0.1)2=3.32016.0084+2.71830.01=0.03000.01=3.0000f''(1.1) \approx \frac{3.3201 - 2(3.0042) + 2.7183}{(0.1)^2} = \frac{3.3201 - 6.0084 + 2.7183}{0.01} = \frac{0.0300}{0.01} = 3.0000

f(1.1)3.0000f''(1.1) \approx \mathbf{3.0000}.

Comparison (1 mark): Exact f(1.1)=e1.1=3.0042f'(1.1)=e^{1.1}=3.0042. Absolute error =3.00903.0042=0.0048=|3.0090-3.0042| = 0.0048, the central-difference truncation error of order O(h2)O(h^2). (The small discrepancy is consistent with rounded four-decimal table data.)

numerical-differentiationfinite-differenceserror
10short5 marks

Solve the initial value problem dydx=2y\dfrac{dy}{dx} = -2y, y(0)=1y(0)=1 using Euler's method with step size h=0.25h=0.25, computing yy at x=0.25,0.50,0.75,1.00x=0.25, 0.50, 0.75, 1.00. Compare y(1.0)y(1.0) with the exact solution y=e2xy=e^{-2x} and comment on the accuracy.

Euler's formula (1 mark): yn+1=yn+hf(xn,yn)y_{n+1} = y_n + h\,f(x_n,y_n) with f(x,y)=2yf(x,y)=-2y and h=0.25h=0.25, so yn+1=yn+0.25(2yn)=yn(10.5)=0.5yny_{n+1}=y_n + 0.25(-2y_n) = y_n(1-0.5) = 0.5\,y_n.

Iterations (3 marks):

nnxnx_nyny_n
00.001.00000
10.250.50000
20.500.25000
30.750.12500
41.000.06250

y(1.0)0.06250y(1.0) \approx \mathbf{0.06250}.

Comparison (1 mark): Exact y(1.0)=e2=0.13534y(1.0)=e^{-2}=0.13534. Absolute error =0.135340.06250=0.07284=|0.13534-0.06250|=0.07284, a large error: with this big step Euler's first-order method substantially underestimates the decay. Accuracy would improve markedly with a smaller hh or a higher-order method (e.g. RK4).

odeeuler-methodstep-size
11short10 marks

(a) Find a root of f(x)=cosxx=0f(x)=\cos x - x = 0 correct to three decimal places using the secant method, taking x0=0.5x_0=0.5 and x1=1.0x_1=1.0 (use radians). (b) Fit a straight line y=a+bxy = a + bx to the following data using the method of least squares, and estimate yy at x=6x=6.

xx12345
yy34679

(a) Secant method (5 marks)

Formula: xn+1=xnf(xn)xnxn1f(xn)f(xn1)x_{n+1} = x_n - f(x_n)\dfrac{x_n - x_{n-1}}{f(x_n)-f(x_{n-1})}, with f(x)=cosxxf(x)=\cos x - x.

f(0.5)=cos0.50.5=0.8775830.5=0.377583f(0.5)=\cos 0.5 - 0.5 = 0.877583 - 0.5 = 0.377583 f(1.0)=cos1.01.0=0.5403021.0=0.459698f(1.0)=\cos 1.0 - 1.0 = 0.540302 - 1.0 = -0.459698

nnxn1x_{n-1}xnx_nxn+1x_{n+1}f(xn+1)f(x_{n+1})
10.5000001.0000000.7254820.022698
21.0000000.7254820.7383990.001149
30.7254820.7383990.739087-0.000003

Iteration: x2=0.725482x_2=0.725482; x3=0.738399x_3=0.738399; x4=0.739087x_4=0.739087. Successive values 0.73840.7384 and 0.73910.7391 agree to three decimals.

Root 0.739\approx \mathbf{0.739} rad.

(b) Least-squares straight line (5 marks)

With n=5n=5, build the sums:

xxyyx2x^2xyxy
1313
2448
36918
471628
592545
Σx=15\Sigma x=15Σy=29\Sigma y=29Σx2=55\Sigma x^2=55Σxy=102\Sigma xy=102

Normal equations:

Σy=na+bΣx    29=5a+15b\Sigma y = na + b\,\Sigma x \;\Rightarrow\; 29 = 5a + 15b Σxy=aΣx+bΣx2    102=15a+55b\Sigma xy = a\,\Sigma x + b\,\Sigma x^2 \;\Rightarrow\; 102 = 15a + 55b

Solve: multiply the first by 3: 87=15a+45b87 = 15a + 45b. Subtract from the second: 10287=(5545)b15=10bb=1.5102-87 = (55-45)b \Rightarrow 15 = 10b \Rightarrow b = 1.5.

Then 5a=2915(1.5)=2922.5=6.5a=1.35a = 29 - 15(1.5) = 29 - 22.5 = 6.5 \Rightarrow a = 1.3.

Best-fit line: y=1.3+1.5x\mathbf{y = 1.3 + 1.5x}.

At x=6x=6: y=1.3+1.5(6)=1.3+9.0=10.3y = 1.3 + 1.5(6) = 1.3 + 9.0 = \mathbf{10.3}.

roots-of-equationscurve-fittingerror-analysis

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