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Section A: Long Answer Questions

Attempt all / any as specified.

4 questions
1long12 marks

(a) Define the rank of a matrix. Reduce the following matrix to its echelon form and hence find its rank:

A=[121324123621]A = \begin{bmatrix} 1 & 2 & -1 & 3 \\ 2 & 4 & 1 & -2 \\ 3 & 6 & 2 & -1 \end{bmatrix}

(b) Investigate for what values of λ\lambda and μ\mu the system of equations

x+y+z=6,x+2y+3z=10,x+2y+λz=μx + y + z = 6,\quad x + 2y + 3z = 10,\quad x + 2y + \lambda z = \mu

has (i) no solution, (ii) a unique solution, and (iii) infinitely many solutions. Solve the system completely in the case of infinitely many solutions.

(a) Rank of a matrix and echelon form

Definition. The rank of a matrix is the number of non-zero rows in its row-echelon form, equivalently the order of the largest non-vanishing minor. It equals the maximum number of linearly independent rows (or columns).

Reduce

A=[121324123621].A = \begin{bmatrix} 1 & 2 & -1 & 3 \\ 2 & 4 & 1 & -2 \\ 3 & 6 & 2 & -1 \end{bmatrix}.

R2R22R1,  R3R33R1R_2 \to R_2 - 2R_1,\; R_3 \to R_3 - 3R_1:

[1213003800510].\begin{bmatrix} 1 & 2 & -1 & 3 \\ 0 & 0 & 3 & -8 \\ 0 & 0 & 5 & -10 \end{bmatrix}.

R3R353R2R_3 \to R_3 - \tfrac{5}{3}R_2:

[12130038000103].\begin{bmatrix} 1 & 2 & -1 & 3 \\ 0 & 0 & 3 & -8 \\ 0 & 0 & 0 & \tfrac{10}{3} \end{bmatrix}.

There are 3 non-zero rows, so rank(A)=3\boxed{\operatorname{rank}(A) = 3}.

(b) Consistency of the system

x+y+z=6,x+2y+3z=10,x+2y+λz=μ.x+y+z=6,\quad x+2y+3z=10,\quad x+2y+\lambda z=\mu.

Form the augmented matrix and eliminate:

[11161231012λμ]R2R1,R3R1[1116012401λ1μ6]\left[\begin{array}{ccc|c} 1 & 1 & 1 & 6 \\ 1 & 2 & 3 & 10 \\ 1 & 2 & \lambda & \mu \end{array}\right] \xrightarrow{R_2-R_1,\,R_3-R_1} \left[\begin{array}{ccc|c} 1 & 1 & 1 & 6 \\ 0 & 1 & 2 & 4 \\ 0 & 1 & \lambda-1 & \mu-6 \end{array}\right] R3R2[1116012400λ3μ10].\xrightarrow{R_3-R_2} \left[\begin{array}{ccc|c} 1 & 1 & 1 & 6 \\ 0 & 1 & 2 & 4 \\ 0 & 0 & \lambda-3 & \mu-10 \end{array}\right].

The last row gives (λ3)z=μ10(\lambda-3)z = \mu-10.

  • (i) No solution: λ3=0\lambda - 3 = 0 and μ100\mu - 10 \ne 0, i.e. λ=3, μ10\lambda = 3,\ \mu \ne 10 (rank of coefficient matrix =2=2, augmented =3=3).
  • (ii) Unique solution: λ30\lambda - 3 \ne 0, i.e. λ3\lambda \ne 3 (any μ\mu); then rank =3==3= number of unknowns.
  • (iii) Infinitely many solutions: λ=3\lambda = 3 and μ=10\mu = 10 (rank =2<3=2 <3).

Solving the infinite case (λ=3,μ=10\lambda=3,\mu=10). Let z=tz = t (free). From R2R_2: y+2t=4y=42ty + 2t = 4 \Rightarrow y = 4 - 2t. From R1R_1: x+y+z=6x=6(42t)t=2+tx + y + z = 6 \Rightarrow x = 6 - (4-2t) - t = 2 + t.

x=2+t,y=42t,z=t,tR.\boxed{x = 2 + t,\quad y = 4 - 2t,\quad z = t,\quad t \in \mathbb{R}.}
determinants-and-matriceslinear-systems
2long12 marks

(a) Evaluate the double integral 01x2x(x2+y2)dydx\displaystyle\int_0^1 \int_{x^2}^{x} (x^2 + y^2)\, dy\, dx and sketch the region of integration. (b) Change the order of integration in 0ax2/a2axxydydx\displaystyle\int_0^a \int_{x^2/a}^{\,2a-x} xy\, dy\, dx and hence evaluate it. (c) Using a triple integral, find the volume of the region bounded by the cylinder x2+y2=4x^2 + y^2 = 4 and the planes z=0z = 0 and z=3xz = 3 - x.

(a) Evaluate 01x2x(x2+y2)dydx\displaystyle\int_0^1 \int_{x^2}^{x} (x^2+y^2)\,dy\,dx

Region: 0x10\le x\le 1, with yy from the parabola y=x2y=x^2 up to the line y=xy=x. The two curves meet at (0,0)(0,0) and (1,1)(1,1); the region is the lens between line and parabola in the first quadrant.

Inner integral:

x2x(x2+y2)dy=[x2y+y33]x2x=(x3+x33)(x4+x63)=43x3x413x6.\int_{x^2}^{x}(x^2+y^2)\,dy = \Big[x^2 y + \tfrac{y^3}{3}\Big]_{x^2}^{x} = \Big(x^3 + \tfrac{x^3}{3}\Big) - \Big(x^4 + \tfrac{x^6}{3}\Big) = \tfrac{4}{3}x^3 - x^4 - \tfrac{1}{3}x^6.

Outer integral:

01(43x3x413x6)dx=4314151317=1315121.\int_0^1\Big(\tfrac{4}{3}x^3 - x^4 - \tfrac{1}{3}x^6\Big)dx = \tfrac{4}{3}\cdot\tfrac14 - \tfrac15 - \tfrac13\cdot\tfrac17 = \tfrac13 - \tfrac15 - \tfrac{1}{21}.

LCD =105=105: 35215105=9105=335.\tfrac{35 - 21 - 5}{105} = \dfrac{9}{105} = \boxed{\dfrac{3}{35}}.

(b) Change the order of integration in 0ax2/a2axxydydx\displaystyle\int_0^a \int_{x^2/a}^{2a-x} xy\,dy\,dx

The region is bounded by the parabola y=x2/ay = x^2/a (i.e. x=ayx=\sqrt{ay}) and the line y=2axy = 2a - x (i.e. x=2ayx = 2a - y), with 0xa0\le x\le a. At x=ax=a both give y=ay=a, so the curves meet at (a,a)(a,a); the parabola meets x=0x=0 at y=0y=0 and the line meets x=0x=0 at y=2ay=2a.

Splitting on yy: for 0ya0\le y\le a, xx runs 0ay0 \to \sqrt{ay}; for ay2aa\le y\le 2a, xx runs 02ay0 \to 2a - y.

I=0a0ayxydxdy+a2a02ayxydxdy.I = \int_0^a \int_0^{\sqrt{ay}} xy\,dx\,dy + \int_a^{2a}\int_0^{2a-y} xy\,dx\,dy.

First part: 0ayxdx=ay2\int_0^{\sqrt{ay}} x\,dx = \tfrac{ay}{2}, so 0ayay2dy=a2a33=a46.\int_0^a y\cdot\tfrac{ay}{2}\,dy = \tfrac{a}{2}\cdot\tfrac{a^3}{3} = \tfrac{a^4}{6}.

Second part: 02ayxdx=(2ay)22\int_0^{2a-y} x\,dx = \tfrac{(2a-y)^2}{2}, so 12a2ay(2ay)2dy.\tfrac12\int_a^{2a} y(2a-y)^2\,dy. Let me expand y(4a24ay+y2)=4a2y4ay2+y3y(4a^2 - 4ay + y^2)=4a^2 y -4a y^2 + y^3. Then

a2a(4a2y4ay2+y3)dy=[2a2y24a3y3+y44]a2a.\int_a^{2a}(4a^2 y - 4a y^2 + y^3)\,dy = \Big[2a^2 y^2 - \tfrac{4a}{3}y^3 + \tfrac{y^4}{4}\Big]_a^{2a}.

At 2a2a: 8a4323a4+4a4=(12323)a4=43a4.8a^4 - \tfrac{32}{3}a^4 + 4a^4 = (12 - \tfrac{32}{3})a^4 = \tfrac{4}{3}a^4. At aa: 2a443a4+14a4=1112a4.2a^4 - \tfrac{4}{3}a^4 + \tfrac14 a^4 = \tfrac{11}{12}a^4. Difference =43a41112a4=512a4.= \tfrac{4}{3}a^4 - \tfrac{11}{12}a^4 = \tfrac{5}{12}a^4. Half of it: 524a4.\tfrac{5}{24}a^4.

I=a46+5a424=4a4+5a424=3a48.I = \tfrac{a^4}{6} + \tfrac{5a^4}{24} = \tfrac{4a^4 + 5a^4}{24} = \boxed{\dfrac{3a^4}{8}}.

(c) Volume bounded by x2+y2=4x^2+y^2=4, z=0z=0, z=3xz=3-x

Over the disk R:x2+y24R: x^2+y^2\le 4 the height is (3x)(3-x) (which is 1>0\ge 1>0 on the disk):

V=R(3x)dA=3(area of disk)RxdA.V = \iint_R (3-x)\,dA = 3\cdot(\text{area of disk}) - \iint_R x\,dA.

The area =π(2)2=4π=\pi(2)^2 = 4\pi and RxdA=0\iint_R x\,dA = 0 by symmetry.

V=3(4π)=12π cubic units.\boxed{V = 3(4\pi) = 12\pi \text{ cubic units.}}
multiple-integralschange-of-ordervolume
3long12 marks

(a) Solve the differential equation (D24D+4)y=e2x+x3(D^2 - 4D + 4)y = e^{2x} + x^3, where DddxD \equiv \dfrac{d}{dx}. (b) Using the method of variation of parameters, solve d2ydx2+y=secx\dfrac{d^2 y}{dx^2} + y = \sec x. (c) Solve the Cauchy–Euler equation x2d2ydx23xdydx+4y=x2lnxx^2 \dfrac{d^2 y}{dx^2} - 3x\dfrac{dy}{dx} + 4y = x^2 \ln x.

(a) (D24D+4)y=e2x+x3(D^2 - 4D + 4)y = e^{2x} + x^3

CF: auxiliary equation m24m+4=(m2)2=0m=2,2m^2 - 4m + 4 = (m-2)^2 = 0 \Rightarrow m = 2,2.

yc=(C1+C2x)e2x.y_c = (C_1 + C_2 x)e^{2x}.

PI for e2xe^{2x}: since 22 is a double root, multiply by x2x^2:

yp1=x22!e2x=x22e2x.y_{p1} = \frac{x^2}{2!}e^{2x} = \frac{x^2}{2}e^{2x}.

PI for x3x^3: 1(D2)2x3=14(1D)2x3\dfrac{1}{(D-2)^2}x^3 = \dfrac{1}{4}\Big(1 - D\Big)^{-2}x^3 with 14(1+D+34D2+12D3+)x3\dfrac{1}{4}\big(1 + D + \tfrac34 D^2 + \tfrac12 D^3 + \dots\big)x^3 where I expand (1D2)2=1+D+34D2+12D3+(1-\tfrac{D}{2})^{-2}=1 + D + \tfrac34 D^2 + \tfrac12 D^3+\cdots.

yp2=14(x3+3x2+346x+126)=14(x3+3x2+92x+3).y_{p2} = \tfrac14\big(x^3 + 3x^2 + \tfrac34\cdot 6x + \tfrac12\cdot 6\big) = \tfrac14\big(x^3 + 3x^2 + \tfrac{9}{2}x + 3\big).

General solution:

y=(C1+C2x)e2x+x22e2x+14(x3+3x2+92x+3).\boxed{y = (C_1 + C_2 x)e^{2x} + \tfrac{x^2}{2}e^{2x} + \tfrac14\Big(x^3 + 3x^2 + \tfrac92 x + 3\Big).}

(b) Variation of parameters: y+y=secxy'' + y = \sec x

CF: yc=C1cosx+C2sinxy_c = C_1\cos x + C_2\sin x, so y1=cosx, y2=sinxy_1=\cos x,\ y_2=\sin x, Wronskian W=cosxcosx(sinx)sinx...W = \cos x\cos x - (-\sin x)\sin x... actually W=y1y2y1y2=cos2x+sin2x=1.W = y_1 y_2' - y_1' y_2 = \cos^2 x + \sin^2 x = 1.

With f(x)=secxf(x)=\sec x:

u1=y2fWdx=sinxsecxdx=tanxdx=lncosx,u_1 = -\int \frac{y_2 f}{W}dx = -\int \sin x\sec x\,dx = -\int \tan x\,dx = \ln|\cos x|, u2=y1fWdx=cosxsecxdx=1dx=x.u_2 = \int \frac{y_1 f}{W}dx = \int \cos x\sec x\,dx = \int 1\,dx = x. yp=u1y1+u2y2=cosxlncosx+xsinx.y_p = u_1 y_1 + u_2 y_2 = \cos x\,\ln|\cos x| + x\sin x. y=C1cosx+C2sinx+cosxlncosx+xsinx.\boxed{y = C_1\cos x + C_2\sin x + \cos x\,\ln|\cos x| + x\sin x.}

(c) Cauchy–Euler: x2y3xy+4y=x2lnxx^2 y'' - 3x y' + 4y = x^2\ln x

Put x=etx = e^t, t=lnxt=\ln x, θ=ddt\theta = \dfrac{d}{dt}. Then xy=θyx y' = \theta y and x2y=θ(θ1)yx^2 y'' = \theta(\theta-1)y. The equation becomes

θ(θ1)y3θy+4y=e2tt    (θ24θ+4)y=te2t.\theta(\theta-1)y - 3\theta y + 4y = e^{2t}\,t \;\Rightarrow\; (\theta^2 - 4\theta + 4)y = t\,e^{2t}.

CF: (θ2)2=0yc=(A+Bt)e2t=(A+Blnx)x2.(\theta-2)^2=0 \Rightarrow y_c = (A + Bt)e^{2t} = (A + B\ln x)x^2.

PI: 1(θ2)2te2t=e2t1θ2t=e2tt36.\dfrac{1}{(\theta-2)^2}t e^{2t} = e^{2t}\dfrac{1}{\theta^2}t = e^{2t}\dfrac{t^3}{6}. In terms of xx: x2(lnx)36.\dfrac{x^2 (\ln x)^3}{6}.

y=(A+Blnx)x2+x2(lnx)36.\boxed{y = (A + B\ln x)x^2 + \frac{x^2(\ln x)^3}{6}.}
higher-order-differential-equationsvariation-of-parameterscauchy-euler
4long12 marks

(a) Define the gradient of a scalar field and the divergence and curl of a vector field. Show that ×(ϕ)=0\nabla \times (\nabla \phi) = \vec{0} for any twice-differentiable scalar field ϕ\phi. (b) A vector field is given by F=(x2yz)i^+(y2zx)j^+(z2xy)k^\vec{F} = (x^2 - yz)\hat{i} + (y^2 - zx)\hat{j} + (z^2 - xy)\hat{k}. Show that F\vec{F} is irrotational and find a scalar potential ϕ\phi such that F=ϕ\vec{F} = \nabla \phi. (c) Verify Green's theorem in the plane for C[(xy+y2)dx+x2dy]\oint_C \big[(xy + y^2)\,dx + x^2\,dy\big], where CC is the closed curve bounded by y=xy = x and y=x2y = x^2.

(a) Definitions and ×(ϕ)=0\nabla\times(\nabla\phi)=\vec 0

  • Gradient of a scalar field ϕ\phi: ϕ=ϕxi^+ϕyj^+ϕzk^\nabla\phi = \dfrac{\partial\phi}{\partial x}\hat i + \dfrac{\partial\phi}{\partial y}\hat j + \dfrac{\partial\phi}{\partial z}\hat k — a vector giving the direction and rate of greatest increase of ϕ\phi.
  • Divergence of F=F1i^+F2j^+F3k^\vec F = F_1\hat i + F_2\hat j + F_3\hat k: F=F1x+F2y+F3z\nabla\cdot\vec F = \dfrac{\partial F_1}{\partial x} + \dfrac{\partial F_2}{\partial y} + \dfrac{\partial F_3}{\partial z} — a scalar measuring net outflow per unit volume.
  • Curl: ×F=(F3yF2z)i^+(F1zF3x)j^+(F2xF1y)k^\nabla\times\vec F = \Big(\dfrac{\partial F_3}{\partial y}-\dfrac{\partial F_2}{\partial z}\Big)\hat i + \Big(\dfrac{\partial F_1}{\partial z}-\dfrac{\partial F_3}{\partial x}\Big)\hat j + \Big(\dfrac{\partial F_2}{\partial x}-\dfrac{\partial F_1}{\partial y}\Big)\hat k — measures local rotation.

Proof ×(ϕ)=0\nabla\times(\nabla\phi)=\vec 0. With F=ϕ\vec F = \nabla\phi, the i^\hat i-component of the curl is

y(ϕz)z(ϕy)=ϕzyϕyz=0\frac{\partial}{\partial y}\Big(\frac{\partial\phi}{\partial z}\Big) - \frac{\partial}{\partial z}\Big(\frac{\partial\phi}{\partial y}\Big) = \phi_{zy} - \phi_{yz} = 0

since mixed partials are equal for a twice-differentiable ϕ\phi. Likewise the j^\hat j and k^\hat k components vanish. Hence ×(ϕ)=0.\nabla\times(\nabla\phi)=\vec 0.

(b) F=(x2yz)i^+(y2zx)j^+(z2xy)k^\vec F=(x^2-yz)\hat i+(y^2-zx)\hat j+(z^2-xy)\hat k

Irrotational check: ×F\nabla\times\vec F. i^\hat i: y(z2xy)z(y2zx)=x(x)=0.\partial_y(z^2-xy)-\partial_z(y^2-zx) = -x-(-x)=0. j^\hat j: z(x2yz)x(z2xy)=y(y)=0.\partial_z(x^2-yz)-\partial_x(z^2-xy) = -y-(-y)=0. k^\hat k: x(y2zx)y(x2yz)=z(z)=0.\partial_x(y^2-zx)-\partial_y(x^2-yz) = -z-(-z)=0. So ×F=0\nabla\times\vec F=\vec 0irrotational.

Potential ϕ\phi: ϕx=x2yzϕ=x33xyz+g(y,z).\phi_x = x^2-yz \Rightarrow \phi = \tfrac{x^3}{3} - xyz + g(y,z). Then ϕy=xz+gy=y2zxgy=y2g=y33+h(z).\phi_y = -xz + g_y = y^2 - zx \Rightarrow g_y = y^2 \Rightarrow g = \tfrac{y^3}{3} + h(z). Then ϕz=xy+h(z)=z2xyh=z2h=z33.\phi_z = -xy + h'(z) = z^2 - xy \Rightarrow h'=z^2 \Rightarrow h=\tfrac{z^3}{3}.

ϕ=13(x3+y3+z3)xyz+C.\boxed{\phi = \tfrac13(x^3 + y^3 + z^3) - xyz + C.}

(c) Green's theorem for C[(xy+y2)dx+x2dy]\oint_C[(xy+y^2)dx + x^2 dy], CC: y=x2y=x^2 to y=xy=x

Here M=xy+y2, N=x2M = xy+y^2,\ N = x^2, region RR: between y=x2y=x^2 (lower) and y=xy=x (upper), 0x10\le x\le 1, traversed counter-clockwise.

Double integral side: NxMy=2x(x+2y)=x2y.N_x - M_y = 2x - (x+2y) = x - 2y.

R(x2y)dA=01x2x(x2y)dydx.\iint_R (x-2y)\,dA = \int_0^1\int_{x^2}^{x}(x-2y)\,dy\,dx.

Inner: [xyy2]x2x=(x2x2)(x3x4)=x4x3.[xy - y^2]_{x^2}^{x} = (x^2 - x^2) - (x^3 - x^4) = x^4 - x^3. Outer: 01(x4x3)dx=1514=120.\int_0^1(x^4 - x^3)dx = \tfrac15 - \tfrac14 = -\tfrac{1}{20}.

Line integral side: Along C1:y=x2C_1: y=x^2, x:01x:0\to1, dy=2xdxdy=2x\,dx: Mdx+Ndy=(xx2+x4)dx+x2(2xdx)=(x3+x4+2x3)dx=(3x3+x4)dx.M\,dx + N\,dy = (x\cdot x^2 + x^4)dx + x^2(2x\,dx) = (x^3 + x^4 + 2x^3)dx = (3x^3 + x^4)dx. 01(3x3+x4)dx=34+15=1920.\int_0^1(3x^3+x^4)dx = \tfrac34 + \tfrac15 = \tfrac{19}{20}. Along C2:y=xC_2: y=x back, x:10x:1\to0, dy=dxdy=dx: Mdx+Ndy=(xx+x2)dx+x2dx=(x2+x2+x2)dx=3x2dx.M\,dx + N\,dy = (x\cdot x + x^2)dx + x^2 dx = (x^2 + x^2 + x^2)dx = 3x^2 dx. 103x2dx=1.\int_1^0 3x^2 dx = -1. Total line integral =19201=120.= \tfrac{19}{20} - 1 = -\tfrac{1}{20}.

Both sides equal 120-\dfrac{1}{20}, so Green's theorem is verified.

vector-calculusdivergence-curlgreens-theorem
B

Section B: Short Answer Questions

Attempt all / any as specified.

7 questions
5short8 marks

Find the eigenvalues and the corresponding eigenvectors of the matrix

A=[211121001].A = \begin{bmatrix} 2 & 1 & 1 \\ 1 & 2 & 1 \\ 0 & 0 & 1 \end{bmatrix}.

Hence verify the Cayley–Hamilton theorem for AA.

Eigenvalues and eigenvectors of A=[211121001]A=\begin{bmatrix}2&1&1\\1&2&1\\0&0&1\end{bmatrix}

Characteristic equation det(AλI)=0\det(A-\lambda I)=0. Expanding along the third row:

det[2λ1112λ1001λ]=(1λ)[(2λ)21].\det\begin{bmatrix}2-\lambda&1&1\\1&2-\lambda&1\\0&0&1-\lambda\end{bmatrix} = (1-\lambda)\big[(2-\lambda)^2 - 1\big].

(2λ)21=λ24λ+3=(λ1)(λ3).(2-\lambda)^2 - 1 = \lambda^2 - 4\lambda + 3 = (\lambda-1)(\lambda-3). So

(1λ)(λ1)(λ3)=0λ=1,1,3.(1-\lambda)(\lambda-1)(\lambda-3)=0 \Rightarrow \boxed{\lambda = 1,\,1,\,3.}

Eigenvector for λ=3\lambda=3: (A3I)x=0(A-3I)x=0: x1+x2+x3=0, x1x2+x3=0, 2x3=0.-x_1+x_2+x_3=0,\ x_1 - x_2 + x_3=0,\ -2x_3=0. So x3=0, x1=x2x_3=0,\ x_1=x_2. Eigenvector v1=(1,1,0)T.\mathbf{v_1}=(1,1,0)^T.

Eigenvectors for λ=1\lambda=1: (AI)x=0(A-I)x=0: x1+x2+x3=0x_1 + x_2 + x_3 = 0 (rows 1 and 2 identical), third row 0=00=0. One independent equation \Rightarrow two free parameters. Choosing x3=0,x2=1x_3=0,x_2=1 gives (1,1,0)T(-1,1,0)^T; choosing x2=0,x3=1x_2=0,x_3=1 gives (1,0,1)T(-1,0,1)^T. So eigenvectors v2=(1,1,0)T, v3=(1,0,1)T.\mathbf{v_2}=(-1,1,0)^T,\ \mathbf{v_3}=(-1,0,1)^T.

Cayley–Hamilton verification

The characteristic polynomial is (λ1)2(λ3)=λ35λ2+7λ3.(\lambda-1)^2(\lambda-3) = \lambda^3 - 5\lambda^2 + 7\lambda - 3. We must show A35A2+7A3I=0.A^3 - 5A^2 + 7A - 3I = 0.

A2=[544454001],A3=A2A=[141313131413001].A^2 = \begin{bmatrix}5&4&4\\4&5&4\\0&0&1\end{bmatrix},\qquad A^3 = A^2 A = \begin{bmatrix}14&13&13\\13&14&13\\0&0&1\end{bmatrix}.

Then A35A2+7A3IA^3 - 5A^2 + 7A - 3I, computed entrywise:

  • (1,1):1425+143=0(1,1):14 - 25 + 14 - 3 = 0; (1,2):1320+70=0(1,2):13-20+7-0=0; (1,3):1320+70=0.(1,3):13-20+7-0=0.
  • (2,1):1320+70=0(2,1):13-20+7-0=0; (2,2):1425+143=0(2,2):14-25+14-3=0; (2,3):1320+70=0.(2,3):13-20+7-0=0.
  • Row 3: 0,0, 15+73=0.0,0,\ 1-5+7-3=0.

All entries are zero, so A35A2+7A3I=0A^3 - 5A^2 + 7A - 3I = 0, verifying the Cayley–Hamilton theorem.

determinants-and-matriceseigenvalues-eigenvectors
6short8 marks

(a) If a=2i^j^+k^\vec{a} = 2\hat{i} - \hat{j} + \hat{k}, b=i^+2j^3k^\vec{b} = \hat{i} + 2\hat{j} - 3\hat{k} and c=3i^4j^+5k^\vec{c} = 3\hat{i} - 4\hat{j} + 5\hat{k}, evaluate the scalar triple product [a b c][\vec{a}\ \vec{b}\ \vec{c}] and state whether the three vectors are coplanar. (b) Prove, using vector methods, that the diagonals of a rhombus bisect each other at right angles.

(a) Scalar triple product [a b c][\vec a\ \vec b\ \vec c]

a=(2,1,1), b=(1,2,3), c=(3,4,5).\vec a=(2,-1,1),\ \vec b=(1,2,-3),\ \vec c=(3,-4,5).

[a b c]=211123345.[\vec a\ \vec b\ \vec c] = \begin{vmatrix}2&-1&1\\1&2&-3\\3&-4&5\end{vmatrix}.

Expand along row 1:

2(25(3)(4))(1)(15(3)(3))+1(1(4)23)2(2\cdot5 - (-3)(-4)) - (-1)(1\cdot5 - (-3)(3)) + 1(1\cdot(-4) - 2\cdot3) =2(1012)+1(5+9)+(46)=2(2)+1410=4+1410=0.= 2(10-12) + 1(5+9) + (-4-6) = 2(-2) + 14 - 10 = -4 + 14 - 10 = 0.

Since [a b c]=0[\vec a\ \vec b\ \vec c] = 0, the three vectors are coplanar (they lie in one plane / are linearly dependent).

(b) Diagonals of a rhombus bisect each other at right angles

Let the rhombus be ABCDABCD with AB=a\vec{AB} = \vec a and AD=b\vec{AD} = \vec b, where a=b|\vec a| = |\vec b| (all sides equal). Then AC=a+b\vec{AC} = \vec a + \vec b (one diagonal) and BD=ba\vec{BD} = \vec b - \vec a (the other diagonal).

Bisection: In a parallelogram (which a rhombus is) the diagonals bisect each other — the midpoint of ACAC is 12(a+b)\tfrac12(\vec a+\vec b) and the midpoint of BDBD (from AA) is a+12(ba)=12(a+b)\vec a + \tfrac12(\vec b-\vec a)=\tfrac12(\vec a+\vec b); same point.

Right angles: Compute the dot product of the diagonals:

ACBD=(a+b)(ba)=aba2+b2ba=b2a2.\vec{AC}\cdot\vec{BD} = (\vec a+\vec b)\cdot(\vec b-\vec a) = \vec a\cdot\vec b - |\vec a|^2 + |\vec b|^2 - \vec b\cdot\vec a = |\vec b|^2 - |\vec a|^2.

Since a=b|\vec a| = |\vec b|, this is 00. Hence the diagonals are perpendicular.

Therefore the diagonals of a rhombus bisect each other at right angles. \blacksquare

vector-algebravector-geometry
7short8 marks

(a) State De Moivre's theorem. Use it to express cos4θ\cos 4\theta and sin4θ\sin 4\theta in terms of cosθ\cos\theta and sinθ\sin\theta. (b) Find all the values of (1+i)1/3(1 + i)^{1/3} and represent them on the Argand diagram.

(a) De Moivre's theorem and cos4θ,sin4θ\cos4\theta,\sin4\theta

Statement. For any integer nn, (cosθ+isinθ)n=cosnθ+isinnθ.(\cos\theta + i\sin\theta)^n = \cos n\theta + i\sin n\theta.

With n=4n=4, expand the left side by the binomial theorem (write c=cosθ, s=sinθc=\cos\theta,\ s=\sin\theta):

(c+is)4=c4+4c3(is)+6c2(is)2+4c(is)3+(is)4(c+is)^4 = c^4 + 4c^3(is) + 6c^2(is)^2 + 4c(is)^3 + (is)^4 =c4+4ic3s6c2s24ics3+s4.= c^4 + 4ic^3 s - 6c^2 s^2 - 4i c s^3 + s^4.

Equating real and imaginary parts with cos4θ+isin4θ\cos4\theta + i\sin4\theta:

cos4θ=cos4θ6cos2θsin2θ+sin4θ,\boxed{\cos4\theta = \cos^4\theta - 6\cos^2\theta\sin^2\theta + \sin^4\theta,} sin4θ=4cos3θsinθ4cosθsin3θ.\boxed{\sin4\theta = 4\cos^3\theta\sin\theta - 4\cos\theta\sin^3\theta.}

(b) Cube roots of 1+i1+i

Write 1+i1+i in polar form: r=12+12=2r = \sqrt{1^2+1^2} = \sqrt2, argument θ=π4\theta = \dfrac{\pi}{4}. So

1+i=2(cosπ4+isinπ4).1+i = \sqrt2\Big(\cos\tfrac\pi4 + i\sin\tfrac\pi4\Big).

By De Moivre, the three cube roots are

(1+i)1/3=21/6[cosπ4+2kπ3+isinπ4+2kπ3],k=0,1,2.(1+i)^{1/3} = 2^{1/6}\Big[\cos\frac{\tfrac\pi4 + 2k\pi}{3} + i\sin\frac{\tfrac\pi4 + 2k\pi}{3}\Big],\quad k=0,1,2.

The arguments are π12, π12+2π3=9π12=3π4, π12+4π3=17π12.\dfrac{\pi}{12},\ \dfrac{\pi}{12}+\dfrac{2\pi}{3}=\dfrac{9\pi}{12}=\dfrac{3\pi}{4},\ \dfrac{\pi}{12}+\dfrac{4\pi}{3}=\dfrac{17\pi}{12}. Thus

z0=21/6(cosπ12+isinπ12), z1=21/6(cos3π4+isin3π4), z2=21/6(cos17π12+isin17π12).z_0 = 2^{1/6}\big(\cos\tfrac{\pi}{12} + i\sin\tfrac{\pi}{12}\big),\ z_1 = 2^{1/6}\big(\cos\tfrac{3\pi}{4} + i\sin\tfrac{3\pi}{4}\big),\ z_2 = 2^{1/6}\big(\cos\tfrac{17\pi}{12} + i\sin\tfrac{17\pi}{12}\big).

Argand diagram (described): the three roots all lie on a circle of radius 21/61.1222^{1/6}\approx 1.122 centred at the origin, spaced 120120^\circ apart, at angles 15, 135, 25515^\circ,\ 135^\circ,\ 255^\circ — forming the vertices of an equilateral triangle.

complex-numbersde-moivre-theorem
8short8 marks

(a) State the ratio test (D'Alembert's test) for the convergence of a series of positive terms. Test the convergence of the series n=1n!nn\displaystyle\sum_{n=1}^{\infty} \frac{n!}{n^n}. (b) Examine the convergence of the series n=11np\displaystyle\sum_{n=1}^{\infty} \frac{1}{n^p} for different values of pp using the integral test.

(a) Ratio test and n!/nn\sum n!/n^n

D'Alembert's ratio test. For a series un\sum u_n of positive terms, let L=limnun+1unL = \lim_{n\to\infty}\dfrac{u_{n+1}}{u_n}. Then the series converges if L<1L<1, diverges if L>1L>1, and the test is inconclusive if L=1L=1.

For un=n!nnu_n = \dfrac{n!}{n^n}:

un+1un=(n+1)!(n+1)n+1nnn!=(n+1)nn(n+1)n+1=nn(n+1)n=(nn+1)n=1(1+1n)n.\frac{u_{n+1}}{u_n} = \frac{(n+1)!}{(n+1)^{n+1}}\cdot\frac{n^n}{n!} = \frac{(n+1)\,n^n}{(n+1)^{n+1}} = \frac{n^n}{(n+1)^n} = \Big(\frac{n}{n+1}\Big)^n = \frac{1}{\big(1+\tfrac1n\big)^n}.

As nn\to\infty, (1+1n)ne\big(1+\tfrac1n\big)^n \to e, so L=1e0.368<1.L = \dfrac1e \approx 0.368 < 1.

Since L<1L<1, the series n!nn\displaystyle\sum \frac{n!}{n^n} converges.

(b) 1/np\sum 1/n^p by the integral test

Integral test. If f(x)=1xpf(x)=\dfrac{1}{x^p} is positive, continuous and decreasing for x1x\ge1 (true for p>0p>0), then n=11np\sum_{n=1}^\infty \dfrac{1}{n^p} and 1dxxp\int_1^\infty \dfrac{dx}{x^p} converge or diverge together.

Case p1p\ne1:

1xpdx=[x1p1p]1.\int_1^\infty x^{-p}\,dx = \Big[\frac{x^{1-p}}{1-p}\Big]_1^\infty.
  • If p>1p>1: 1p<01-p<0, x1p0x^{1-p}\to0, integral =1p1=\dfrac{1}{p-1} (finite) \Rightarrow converges.
  • If p<1p<1: 1p>01-p>0, x1px^{1-p}\to\infty \Rightarrow integral diverges \Rightarrow diverges.

Case p=1p=1: 1dxx=[lnx]1=\int_1^\infty \dfrac{dx}{x} = [\ln x]_1^\infty = \infty \Rightarrow diverges (harmonic series).

Conclusion (p-series): n=11np\displaystyle\sum_{n=1}^\infty \frac{1}{n^p} converges if and only if p>1\boxed{p>1}; it diverges for p1p\le1.

infinite-seriesconvergence-tests
9short8 marks

(a) Find the equation of the plane passing through the points (1,1,0)(1, 1, 0), (2,2,1)(-2, 2, -1) and (1,2,1)(1, 2, 1). (b) Find the shortest distance between the lines

x12=y23=z34andx23=y44=z55.\frac{x-1}{2} = \frac{y-2}{3} = \frac{z-3}{4} \quad\text{and}\quad \frac{x-2}{3} = \frac{y-4}{4} = \frac{z-5}{5}.

(a) Plane through (1,1,0),(2,2,1),(1,2,1)(1,1,0),(-2,2,-1),(1,2,1)

Let P=(1,1,0)P=(1,1,0). Two in-plane vectors:

u=(2,2,1)(1,1,0)=(3,1,1),v=(1,2,1)(1,1,0)=(0,1,1).\vec{u} = (-2,2,-1)-(1,1,0) = (-3,1,-1),\quad \vec{v} = (1,2,1)-(1,1,0) = (0,1,1).

Normal n=u×v\vec n = \vec u\times\vec v:

n=i^j^k^311011=i^(11(1)1)j^((3)1(1)0)+k^((3)110)\vec n = \begin{vmatrix}\hat i&\hat j&\hat k\\-3&1&-1\\0&1&1\end{vmatrix} = \hat i(1\cdot1 -(-1)\cdot1) - \hat j((-3)\cdot1 - (-1)\cdot0) + \hat k((-3)\cdot1 - 1\cdot0) =i^(1+1)j^(3)+k^(3)=(2,3,3).= \hat i(1+1) - \hat j(-3) + \hat k(-3) = (2,\,3,\,-3).

Plane: 2(x1)+3(y1)3(z0)=02(x-1) + 3(y-1) - 3(z-0) = 0, i.e.

2x+3y3z=5.\boxed{2x + 3y - 3z = 5.}

(Check: (1,2,1):2+63=5(1,2,1):2+6-3=5 ✓.)

(b) Shortest distance between the two lines

Line 1: point A=(1,2,3)A=(1,2,3), direction d1=(2,3,4)\vec d_1=(2,3,4). Line 2: point B=(2,4,5)B=(2,4,5), direction d2=(3,4,5)\vec d_2=(3,4,5).

d1×d2=i^j^k^234345=i^(1516)j^(1012)+k^(89)=(1,2,1).\vec d_1\times\vec d_2 = \begin{vmatrix}\hat i&\hat j&\hat k\\2&3&4\\3&4&5\end{vmatrix} = \hat i(15-16) - \hat j(10-12) + \hat k(8-9) = (-1,\,2,\,-1).

d1×d2=1+4+1=6.|\vec d_1\times\vec d_2| = \sqrt{1+4+1} = \sqrt6.

AB=BA=(1,2,2).\vec{AB} = B-A = (1,2,2).

(d1×d2)AB=(1)(1)+2(2)+(1)(2)=1+42=1.(\vec d_1\times\vec d_2)\cdot\vec{AB} = (-1)(1) + 2(2) + (-1)(2) = -1+4-2 = 1.

Shortest distance:

d=(d1×d2)ABd1×d2=16=160.408 units.d = \frac{|(\vec d_1\times\vec d_2)\cdot\vec{AB}|}{|\vec d_1\times\vec d_2|} = \frac{1}{\sqrt6} = \boxed{\frac{1}{\sqrt6}\approx 0.408 \text{ units.}}
lines-and-planes-3dshortest-distance
10short8 marks

Compute the work done by the force field F=(3x2+6y)i^14yzj^+20xz2k^\vec{F} = (3x^2 + 6y)\hat{i} - 14yz\,\hat{j} + 20xz^2\,\hat{k} in moving a particle from the point (0,0,0)(0,0,0) to the point (1,1,1)(1,1,1) along the curve x=tx = t, y=t2y = t^2, z=t3z = t^3.

Work done by F\vec F along x=t, y=t2, z=t3x=t,\ y=t^2,\ z=t^3

F=(3x2+6y)i^14yzj^+20xz2k^.\vec F = (3x^2+6y)\hat i - 14yz\,\hat j + 20xz^2\,\hat k. Work =CFdr.= \displaystyle\int_C \vec F\cdot d\vec r.

Parametrize, t:01t:0\to1 (since (0,0,0)(1,1,1)(0,0,0)\to(1,1,1)):

x=t, y=t2, z=t3,dx=dt, dy=2tdt, dz=3t2dt.x=t,\ y=t^2,\ z=t^3,\qquad dx=dt,\ dy=2t\,dt,\ dz=3t^2\,dt.

Components in tt:

  • 3x2+6y=3t2+6t2=9t2.3x^2+6y = 3t^2 + 6t^2 = 9t^2.
  • 14yz=14t2t3=14t5.-14yz = -14\,t^2 t^3 = -14t^5.
  • 20xz2=20t(t3)2=20t7.20xz^2 = 20\,t\,(t^3)^2 = 20t^7.
Fdr=(9t2)(dt)+(14t5)(2tdt)+(20t7)(3t2dt)=(9t228t6+60t9)dt.\vec F\cdot d\vec r = (9t^2)(dt) + (-14t^5)(2t\,dt) + (20t^7)(3t^2\,dt) = \big(9t^2 - 28t^6 + 60t^9\big)dt.

Integrate:

W=01(9t228t6+60t9)dt=[3t34t7+6t10]01=34+6=5 units of work.W = \int_0^1 (9t^2 - 28t^6 + 60t^9)\,dt = \Big[3t^3 - 4t^7 + 6t^{10}\Big]_0^1 = 3 - 4 + 6 = \boxed{5 \text{ units of work.}}
vector-calculusline-integralwork-done
11short8 marks

By changing to polar coordinates, evaluate 00e(x2+y2)dxdy\displaystyle\int_0^{\infty}\int_0^{\infty} e^{-(x^2 + y^2)}\, dx\, dy and hence deduce the value of 0ex2dx\displaystyle\int_0^{\infty} e^{-x^2}\, dx.

Gaussian integral via polar coordinates

Let I=00e(x2+y2)dxdy.I = \displaystyle\int_0^\infty\int_0^\infty e^{-(x^2+y^2)}\,dx\,dy. The region is the first quadrant x0, y0x\ge0,\ y\ge0.

Switch to polar coordinates x=rcosθ, y=rsinθ, dxdy=rdrdθx=r\cos\theta,\ y=r\sin\theta,\ dx\,dy = r\,dr\,d\theta. The first quadrant corresponds to 0θπ2, 0r<0\le\theta\le\tfrac\pi2,\ 0\le r<\infty, and x2+y2=r2x^2+y^2 = r^2:

I=0π/20er2rdrdθ.I = \int_0^{\pi/2}\int_0^\infty e^{-r^2}\,r\,dr\,d\theta.

Inner integral: let u=r2, du=2rdru=r^2,\ du=2r\,dr:

0er2rdr=120eudu=12.\int_0^\infty e^{-r^2} r\,dr = \tfrac12\int_0^\infty e^{-u}\,du = \tfrac12.

Outer: 0π/2dθ=π2.\int_0^{\pi/2} d\theta = \tfrac\pi2. Hence

I=π212=π4.I = \frac\pi2\cdot\frac12 = \boxed{\frac{\pi}{4}}.

Deducing 0ex2dx\int_0^\infty e^{-x^2}\,dx

Because the integrand separates, II also factors:

I=(0ex2dx)(0ey2dy)=(0ex2dx)2.I = \left(\int_0^\infty e^{-x^2}\,dx\right)\left(\int_0^\infty e^{-y^2}\,dy\right) = \left(\int_0^\infty e^{-x^2}\,dx\right)^2.

Let J=0ex2dx.J = \int_0^\infty e^{-x^2}\,dx. Then J2=π4J^2 = \dfrac\pi4, so

0ex2dx=π2.\boxed{\int_0^\infty e^{-x^2}\,dx = \frac{\sqrt\pi}{2}.}
multiple-integralspolar-coordinates

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