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9.3 Workshop Solutions 3

True or False?

i) True, since x=r⁢cos⁡θx=r\cos\theta and y=r⁢sin⁡θy=r\sin\theta.

ii) False. The set of points given by θ=π4\theta=\frac{\pi}{4} is only half of the line y=xy=x: the points (x,x)(x,x) with x<0x<0 are given by θ=5⁢π4\theta=\frac{5\pi}{4}.

iii) False. The gradient is -fxfy-\frac{f_{x}}{f_{y}}. To see this, we differentiate f⁢(x,y)=0f(x,y)=0 with respect to xx to get fx+fy⁢d⁢yd⁢x=0f_{x}+f_{y}\frac{dy}{dx}=0, so that fy⁢d⁢yd⁢x=-fxf_{y}\frac{dy}{dx}=-f_{x} and hence d⁢yd⁢x=-fxfy\frac{dy}{dx}=-\frac{f_{x}}{f_{y}}.

iv) False: we also require fx⁢x⁢fy⁢y-fx⁢y2>0f_{xx}f_{yy}-f_{xy}^{2}>0 (see slide 4.11 in the notes).

W3.1. We have x=cosh⁡t≥0x=\cosh t\geq 0 and

x2-y2=cosh2⁡t-sinh2⁡t=1,x^{2}-y^{2}=\cosh^{2}t-\sinh^{2}t=1,

so (x,y)(x,y) lies on the right branch of the hyperbola.

(ii) d⁢xd⁢t=sinh⁡t{{dx}\over{dt}}=\sinh t and d⁢yd⁢t=cosh⁡t{{dy}\over{dt}}=\cosh t so

d⁢yd⁢x=d⁢y/d⁢td⁢x/d⁢t=cosh⁡tsinh⁡t=coth⁡t.{{dy}\over{dx}}={{dy/dt}\over{dx/dt}}={{\cosh t}\over{\sinh t}}=\coth t.

W3.2 (i) With x=a⁢t2x=at^{2} and y=2⁢a⁢ty=2at we have

y2=4⁢a2⁢t2=4⁢a⁢x,y^{2}=4a^{2}t^{2}=4ax,

so (x,y)(x,y) lies on CC.

(ii) We have

d⁢xd⁢t=2⁢a⁢t,  d⁢yd⁢t=2⁢a,{{dx}\over{dt}}=2at,\qquad{{dy}\over{dt}}=2a,

so the tangent has gradient

d⁢yd⁢x=d⁢y/d⁢td⁢x/d⁢t=1t,{{dy}\over{dx}}={{dy/dt}\over{dx/dt}}={{1}\over{t}},

and the tangent has equation

y-2⁢a⁢t=1t⁢(x-a⁢t2), or (rearranging) y=xt+a⁢t;y-2at={{1}\over{t}}(x-at^{2}),\quad{\hbox{or (rearranging)}}\quad y={{x}\over{% t}}+at;

whereas the normal has gradient

-d⁢xd⁢y=-t,-{{dx}\over{dy}}=-t,

so the normal has equation

y-2⁢a⁢t=-t⁢(x-a⁢t2).y-2at=-t(x-at^{2}).

(iii) To determine the arc length we integrate (d⁢xd⁢t)2+(d⁢yd⁢t)2\sqrt{\left(\frac{dx}{dt}\right)^{2}+\left(\frac{dy}{dt}\right)^{2}} over tt, from t=0t=0 to t=1t=1; another possibility is to integrate 1+(d⁢xd⁢y)2\sqrt{1+\left(\frac{dx}{dy}\right)^{2}} over yy, from y=0y=0 to y=2⁢ay=2a. If we try to integrate 1+(d⁢yd⁢x)2\sqrt{1+\left(\frac{dy}{dx}\right)^{2}} over xx then we obtain a slightly awkward integral of 1+ax\sqrt{1+\frac{a}{x}}, which needs a substitution.

Since d⁢xd⁢t=2⁢a⁢t\frac{dx}{dt}=2at and d⁢yd⁢t=2⁢a\frac{dy}{dt}=2a, we see that the arc length is

∫014⁢a2+4⁢a2⁢t2⁢d⁢t=2⁢a⁢∫011+t2⁢d⁢t.\int_{0}^{1}\sqrt{4a^{2}+4a^{2}t^{2}}\,dt=2a\int_{0}^{1}\sqrt{1+t^{2}}\,dt.

Now we make the substitution t=sinh⁡ut=\sinh u, so that 1+t2=cosh⁡u\sqrt{1+t^{2}}=\cosh u and d⁢t=cosh⁡u⁢d⁢udt=\cosh u\,du. Thus the integral becomes

2⁢a⁢∫0sinh-1⁡1cosh2⁡u⁢d⁢u=a⁢∫0sinh-1⁡1(cosh⁡2⁢u+1)⁢d⁢u=a⁢[12⁢sinh⁡2⁢u+u]0sinh-1⁡1.2a\int_{0}^{\sinh^{-1}1}\cosh^{2}u\,du=a\int_{0}^{\sinh^{-1}1}(\cosh 2u+1)\,du% =a\left[\frac{1}{2}\sinh 2u+u\right]_{0}^{\sinh^{-1}1}.

We therefore get the awkward result that the arc length is a⁢(sinh-1⁡1+12⁢sinh⁡(2⁢sinh-1⁡1))a(\sinh^{-1}1+\frac{1}{2}\sinh(2\sinh^{-1}1)), but this can be simplified somewhat. Firstly, sinh⁡(2⁢y)=2⁢sinh⁡y⁢cosh⁡y=2⁢sinh⁡y⁢1+sinh2⁡y\sinh(2y)=2\sinh y\cosh y=2\sinh y\sqrt{1+\sinh^{2}y}, so 12⁢sinh⁡(2⁢sinh-1⁡1)=2\frac{1}{2}\sinh(2\sinh^{-1}1)=\sqrt{2}. Secondly, we can express sinh-1⁡x\sinh^{-1}x uniquely in terms of xx by solving the equation ey-e-y2=x\frac{e^{y}-e^{-y}}{2}=x, so e2⁢y-2⁢x⁢ey-1=0e^{2y}-2xe^{y}-1=0, whence ey=2⁢x±4⁢x2+42e^{y}=\frac{2x\pm\sqrt{4x^{2}+4}}{2}, so y=log⁡(x+x2+1)y=\log(x+\sqrt{x^{2}+1}). In particular, sinh-1=log⁡(1+2)\sinh^{-1}=\log(1+\sqrt{2}). So the arc length from t=0t=0 to t=1t=1 is a⁢(2+log⁡(1+2))a(\sqrt{2}+\log(1+\sqrt{2})).

W3.3 (i) We let x=-cos2⁡θx=-\cos^{2}\theta and y=-sin⁡θ⁢cos2⁡θy=-\sin\theta\cos^{2}\theta, then

x2⁢(x+1)=cos4⁡θ⁢(1-cos2⁡θ)=cos4⁡θ⁢sin2⁡θ=y2;x^{2}(x+1)=\cos^{4}\theta(1-\cos^{2}\theta)=\cos^{4}\theta\sin^{2}\theta=y^{2};

hence (x,y)(x,y) lies on TT; moreover

d⁢xd⁢θ=2⁢cos⁡θ⁢sin⁡θ, d⁢yd⁢θ=-cos3⁡θ+2⁢sin2⁡θ⁢cos⁡θ;{{dx}\over{d\theta}}=2\cos\theta\sin\theta,\quad{{dy}\over{d\theta}}=-\cos^{3}% \theta+2\sin^{2}\theta\cos\theta;

so

d⁢yd⁢x=d⁢y/d⁢θd⁢x/d⁢θ=-cos3⁡θ+2⁢sin2⁡θ⁢cos⁡θ2⁢cos⁡θ⁢sin⁡θ=2⁢sin2⁡θ-cos2⁡θ2⁢sin⁡θ.{{dy}\over{dx}}={{dy/d\theta}\over{dx/d\theta}}={{-\cos^{3}\theta+2\sin^{2}% \theta\cos\theta}\over{2\cos\theta\sin\theta}}={{2\sin^{2}\theta-\cos^{2}% \theta}\over{2\sin\theta}}.

(ii) Now let x=tan2⁡θx=\tan^{2}\theta and y=sec⁢θ⁢tan2⁡θy={\hbox{sec}}\,\theta\tan^{2}\theta; then

x2⁢(x+1)=tan4⁡θ⁢(tan2⁡θ+1)=tan4⁡θ⁢sec2⁢θ=y2;x^{2}(x+1)=\tan^{4}\theta(\tan^{2}\theta+1)=\tan^{4}\theta{\hbox{sec}}^{2}% \theta=y^{2};

hence (x,y)(x,y) lies on TT; moreover,

d⁢xd⁢θ=2⁢tan⁡θ⁢sec2⁢θ, d⁢yd⁢θ=sec⁢θ⁢tan3⁡θ+2⁢tan⁡θ⁢sec3⁢θ;{{dx}\over{d\theta}}=2\tan\theta{\hbox{sec}}^{2}\theta,\quad{{dy}\over{d\theta% }}={\hbox{sec}}\theta\tan^{3}\theta+2\tan\theta{\hbox{sec}}^{3}\theta;

so

d⁢yd⁢x=d⁢y/d⁢θd⁢x/d⁢θ=sec⁢θ⁢tan3⁡θ+2⁢tan⁡θ⁢sec3⁢θ2⁢tan⁡θ⁢sec2⁢θ=tan2⁡θ+2⁢sec2⁡θ2⁢sec⁢θ.{{dy}\over{dx}}={{dy/d\theta}\over{dx/d\theta}}={{{\hbox{sec}}\theta\tan^{3}% \theta+2\tan\theta{\hbox{sec}}^{3}\theta}\over{2\tan\theta{\hbox{sec}}^{2}% \theta}}={{\tan^{2}\theta+2\sec^{2}\theta}\over{2{\hbox{sec}}\,\theta}}.

W3.4. (i) We observe that x3=t6=y2x^{3}=t^{6}=y^{2}, so (x,y)(x,y) lies on CC, and x,y≥0x,y\geq 0, so the point is in the first quadrant.

(ii) We calculate

d⁢xd⁢t=2⁢t,  d⁢yd⁢t=3⁢t2,{{dx}\over{dt}}=2t,\qquad{{dy}\over{dt}}=3t^{2},

so arclength is given by

(d⁢sd⁢t)2=(d⁢xd⁢t)2+(d⁢yd⁢t)2=4⁢t2+9⁢t4\Bigl({{ds}\over{dt}}\Bigr)^{2}=\Bigl({{dx}\over{dt}}\Bigr)^{2}+\Bigl({{dy}% \over{dt}}\Bigr)^{2}=4t^{2}+9t^{4}

so

La=∫0ad⁢sd⁢t⁢d⁢t=∫0at⁢4+9⁢t2⁢d⁢tL_{a}=\int_{0}^{a}{{ds}\over{dt}}dt=\int_{0}^{a}t\sqrt{4+9t^{2}}\,dt

so we substitute t2=ut^{2}=u and d⁢u/d⁢t=2⁢tdu/dt=2t, so get

La=12⁢∫0a24+9⁢u⁢d⁢u=12⁢[23⋅9⁢(4+9⁢u)3/2]0a2=127⁢((4+9⁢a2)3/2-43/2).L_{a}={{1}\over{2}}\int_{0}^{a^{2}}\sqrt{4+9u}\,du={{1}\over{2}}\Bigl[{{2}% \over{3\cdot 9}}\bigl(4+9u\bigr)^{3/2}\Bigr]_{0}^{a^{2}}={{1}\over{27}}\Bigl(% \bigl(4+9a^{2})^{3/2}-4^{3/2}\Bigr).

This calculation was first carried out by Neil, and the simple form of the answer caused much surprise at the time.

(iii) When a=1a=1, the precise value of LaL_{a} is 133/2-827\frac{13^{3/2}-8}{27}, which is 1.4401.440 to three decimal places. To apply Simpson’s rule to the integral ∫01t⁢4+9⁢t2⁢d⁢t\int_{0}^{1}t\sqrt{4+9t^{2}}\,dt, we first have to evaluate the function t⁢4+9⁢t2t\sqrt{4+9t^{2}} at the three points t=0t=0, t=12t=\frac{1}{2} and t=1t=1. The respective values are 00, 12⁢4+94=54\frac{1}{2}\sqrt{4+\frac{9}{4}}=\frac{5}{4}, and 13\sqrt{13}. Thus Simpson’s rule produces an estimate of

1-06⁢(1.0+4.⁢54+1.⁢13)=5+136.\frac{1-0}{6}\left(1.0+4.\frac{5}{4}+1.\sqrt{13}\right)=\frac{5+\sqrt{13}}{6}.

This gives us a value of 1.4341.434, less than 1⁢%1\% from the precise value.

W3.5. Let f⁢(x,y)=4⁢x2+x⁢y+6⁢y2-4f(x,y)=4x^{2}+xy+6y^{2}-4; so that f⁢(x,y)=0f(x,y)=0 gives the equation for the ellipse and defines yy implicitly as a function of xx. To find d⁢yd⁢x\frac{dy}{dx} we can either use the formula d⁢yd⁢x=-fxfy\frac{dy}{dx}=-\frac{f_{x}}{f_{y}}, or we can differentiate the equation f⁢(x,y)=0f(x,y)=0 with respect to xx. The second approach is more instructive, so this is how we’ll do it here. (However, both methods amount to the same thing.)

Since 4⁢x2+x⁢y+6⁢y2-4=04x^{2}+xy+6y^{2}-4=0, when we differentiate with respect to xx we get:

8⁢x+y+x⁢d⁢yd⁢x+12⁢y⁢d⁢yd⁢x=0.8x+y+x\frac{dy}{dx}+12y\frac{dy}{dx}=0.

Now we collect terms together, so that

(x+12⁢y)⁢d⁢yd⁢x=-8⁢x-y, hence⁢d⁢yd⁢x=-8⁢x+yx+12⁢y.(x+12y)\frac{dy}{dx}=-8x-y,\;\;\mbox{hence}\;\;\frac{dy}{dx}=-\frac{8x+y}{x+12% y}.

(Note that fx=8⁢x+yf_{x}=8x+y and fy=x+12⁢yf_{y}=x+12y, which tallies with d⁢yd⁢x=-fxfy\frac{dy}{dx}=-\frac{f_{x}}{f_{y}}.)

W3.6. (i) We suppose that the formula

x+y=tan-1⁡yx+y=\tan^{-1}y

defines yy implicitly as a function of xx, and we differentiate to obtain

1+d⁢yd⁢x=11+y2⁢d⁢yd⁢x,1+{{dy}\over{dx}}={{1}\over{1+y^{2}}}{{dy}\over{dx}},

so that

(1+y2)+(1+y2)⁢d⁢yd⁢x=d⁢yd⁢x,(1+y^{2})+(1+y^{2}){{dy}\over{dx}}={{dy}\over{dx}},

and hence

1+y2+y2⁢d⁢yd⁢x=0.1+y^{2}+y^{2}{{dy}\over{dx}}=0.

Alternatively, let f⁢(x,y)=x+y+tan-1⁡yf(x,y)=x+y+\tan^{-1}y with first-order partial derivatives

∂⁡f∂⁡x=1, ∂⁡f∂⁡y=1-11+y2=y21+y2.{{\partial f}\over{\partial x}}=1,\quad{{\partial f}\over{\partial y}}=1-{{1}% \over{1+y^{2}}}={{y^{2}}\over{1+y^{2}}}.

Then the required derivative is

d⁢yd⁢x=-∂⁡f/∂⁡x∂⁡f/∂⁡y=-1+y2y2.{{dy}\over{dx}}=-{{\partial f/\partial x}\over{\partial f/\partial y}}=-{{1+y^% {2}}\over{y^{2}}}.

(ii) We can differentiate the formula

tan-1⁡yx=12⁢log⁡(x2+y2)\tan^{-1}{{y}\over{x}}={{1}\over{2}}\log\bigl(x^{2}+y^{2}\bigr)

with respect to xx, and obtain by the chain rule

11+y2/x2⁢dd⁢x⁢yx=12⁢1x2+y2⁢dd⁢x⁢(x2+y2){{1}\over{1+y^{2}/x^{2}}}{{d}\over{dx}}{{y}\over{x}}={{1}\over{2}}{{1}\over{x^% {2}+y^{2}}}{{d}\over{dx}}\bigl(x^{2}+y^{2}\bigr)
11+y2/x2⁢x⁢d⁢yd⁢x-yx2=1x2+y2⁢(x+y⁢d⁢yd⁢x){{1}\over{1+y^{2}/x^{2}}}{{x{{dy}\over{dx}}-y}\over{x^{2}}}={{1}\over{x^{2}+y^% {2}}}\Bigl(x+y{{dy}\over{dx}}\Bigr)

which reduces, when we multiply by x2+y2x^{2}+y^{2}, to

x⁢d⁢yd⁢x-y=x+y⁢d⁢yd⁢x,x{{dy}\over{dx}}-y=x+y{{dy}\over{dx}},
d⁢yd⁢x=x+yx-y.{{dy}\over{dx}}={{x+y}\over{x-y}}.

Alternatively, we can introduce

f⁢(x,y)=tan-1⁡(y/x)-12⁢log⁡(x2+y2)-1f(x,y)=\tan^{-1}(y/x)-{{1}\over{2}}\log(x^{2}+y^{2})-1

and calculate the first-order partial derivatives

fx=11+y2/x2⁢(-y/x)-xx2+y2=-y+xx2+y2,f_{x}={{1}\over{1+y^{2}/x^{2}}}\bigl(-y/x\bigr)-{{x}\over{x^{2}+y^{2}}}=-{{y+x% }\over{x^{2}+y^{2}}},
fy=11+y2/x2⁢(1/x)-yx2+y2=x-yx2+y2;f_{y}={{1}\over{1+y^{2}/x^{2}}}\bigl(1/x\bigr)-{{y}\over{x^{2}+y^{2}}}={{x-y}% \over{x^{2}+y^{2}}};

hence

d⁢yd⁢x=-fxfy=x+yx-y.{{dy}\over{dx}}=-{{f_{x}}\over{f_{y}}}={{x+y}\over{x-y}}.

W3.7.(i) When x=1x=1, we have 8⁢y2=28y^{2}=2; so that y=±1/2y=\pm 1/2.

(ii) We assume that yy is defined implicitly as a function of xx and we differentiate the relation

8⁢y2=x2⁢(x+1)8y^{2}=x^{2}(x+1)

to obtain

16⁢y⁢d⁢yd⁢x=2⁢x⁢(x+1)+x2=3⁢x2+2⁢x;16y{{dy}\over{dx}}=2x(x+1)+x^{2}=3x^{2}+2x;

hence

d⁢yd⁢x=3⁢x2+2⁢x16⁢y.{{dy}\over{dx}}={{3x^{2}+2x}\over{16y}}.

Alternatively, let f⁢(x,y)=8⁢y2-x2⁢(x+1)f(x,y)=8y^{2}-x^{2}(x+1) so that fx=-2⁢x⁢(x+1)-x2f_{x}=-2x(x+1)-x^{2} and fy=16⁢yf_{y}=16y; then

d⁢yd⁢x=-fxfy=3⁢x2+2⁢x16⁢y.{{dy}\over{dx}}=-{{f_{x}}\over{f_{y}}}={{3x^{2}+2x}\over{16y}}.

From the formula above, we see that the tangents to the curve have gradients

d⁢yd⁢x={5/8,a⁢t⁢(1,1/2);-5/8,a⁢t⁢(1,-1/2).{{dy}\over{dx}}=\begin{cases}5/8,&at$(1,1/2)$;\cr-5/8,&at$(1,-1/2)$.\cr\end{cases}

For the equations of the tangents, we have:

y-12=58⁢(x-1)⁢and⁢y-(-12)=-58⁢(x-1)y-\frac{1}{2}=\frac{5}{8}\left(x-1\right)\;\;\mbox{and}\;\;y-(-\frac{1}{2})=-% \frac{5}{8}\left(x-1\right)

so we get the two lines y=±(58⁢x-18)y=\pm\left(\frac{5}{8}x-\frac{1}{8}\right) at the respective points (1,±12)(1,\pm\frac{1}{2}).

W3.8. (i) We calculate the first-order partial derivatives of g⁢(x,y)=x2-2⁢x⁢y+y3g(x,y)=x^{2}-2xy+y^{3} to be

∂⁡g∂⁡x=2⁢x-2⁢y, ∂⁡g∂⁡y=-2⁢x+3⁢y2;{{\partial g}\over{\partial x}}=2x-2y,\quad{{\partial g}\over{\partial y}}=-2x% +3y^{2};

the second-order partial derivatives are

gx⁢x=2, gy⁢y=6⁢y, gx⁢y=-2.g_{xx}=2,\quad g_{yy}=6y,\quad g_{xy}=-2.

(ii) The stationary points occur where

2⁢x-2⁢y=0 and -2⁢x+3⁢y2=0.2x-2y=0\quad{\hbox{and}}\quad-2x+3y^{2}=0.

From the first equation, we deduce that x=yx=y, so the second equation becomes -2⁢x+3⁢x2=0-2x+3x^{2}=0, or x⁢(-2+3⁢x)=0x(-2+3x)=0, with roots x=0x=0 and x=2/3x=2/3; hence the stationary points are

(0,0) and (2/3,2/3).(0,0)\quad{\hbox{and}}\quad(2/3,2/3).

(iii) The Hessian discriminant is

Δ=gx⁢x⁢gy⁢y-gx⁢y2=12⁢y-4.\Delta=g_{xx}g_{yy}-g_{xy}^{2}=12y-4.

The stationary points are classified in the following table.

stationary pointΔgx⁢xnature(0,0)-4<0*saddle(2/3,2/3)42>0local minimum\begin{matrix}{\hbox{stationary point}}&\Delta&g_{xx}&{\hbox{nature}}\cr(0,0)&% -4<0&*&{\hbox{saddle}}\cr(2/3,2/3)&4&2>0&{\hbox{local minimum}}\cr\end{matrix}

W3.9. (i) We have fx=1-y⁢exf_{x}=1-ye^{x} and fy=3⁢y2-exf_{y}=3y^{2}-e^{x}, so both partial derivatives are zero exactly when y=e-xy=e^{-x} and 3⁢y2=ex3y^{2}=e^{x}. Multiplying, we obtain: y⁢.3⁢y2=e-x.ex=1y.3y^{2}=e^{-x}.e^{x}=1, hence y=133y=\frac{1}{\sqrt[3]{3}}. It follows that ex=3332=33e^{x}=\frac{3}{\sqrt[3]{3}^{2}}=\sqrt[3]{3}, so x=13⁢log⁡3x=\frac{1}{3}\log 3. Thus there is one stationary point (13⁢log⁡3,133)(\frac{1}{3}\log 3,\frac{1}{\sqrt[3]{3}}).

(ii) Here gx=y3-1(x+y)2g_{x}=y^{3}-\frac{1}{(x+y)^{2}} and gy=3⁢x⁢y2-1(x+y)2g_{y}=3xy^{2}-\frac{1}{(x+y)^{2}}, so if both partial derivatives are zero we must have y3=1(x+y)2=3⁢x⁢y2y^{3}=\frac{1}{(x+y)^{2}}=3xy^{2}, so y=3⁢xy=3x. Substituting back into the equation y3=1(x+y)2y^{3}=\frac{1}{(x+y)^{2}}, we get 27⁢x3=1(4⁢x)227x^{3}=\frac{1}{(4x)^{2}}, so x5=127.16=1432x^{5}=\frac{1}{27.16}=\frac{1}{432}. Over ℝ{\mathbb{R}}, there is only one solution here: x=14325x=\frac{1}{\sqrt[5]{432}}, and so y=34325=9165y=\frac{3}{\sqrt[5]{432}}=\sqrt[5]{\frac{9}{16}}. Thus there is one turning point 14325⁢(1,3)\frac{1}{\sqrt[5]{432}}(1,3).

(iii) Here hx=3⁢x2-3⁢y4h_{x}=3x^{2}-3y^{4} and hy=12⁢y3-12⁢x⁢y3=12⁢y3⁢(1-x)h_{y}=12y^{3}-12xy^{3}=12y^{3}(1-x). Thus if hy=0h_{y}=0 then either y=0y=0 or x=1x=1; if hx=0h_{x}=0 then x2=y4x^{2}=y^{4}, so x=±y2x=\pm y^{2}. Combining these, if y=0y=0 and x2=y4x^{2}=y^{4} then x=y=0x=y=0; if x=1x=1 and x=±y2x=\pm y^{2} then y=±1y=\pm 1. Thus there are three stationary points: (0,0)(0,0), (1,1)(1,1) and (1,-1)(1,-1).

Showing existence of saddle points

i) In this case we have fx⁢x=-y⁢exf_{xx}=-ye^{x}, fx⁢y=-exf_{xy}=-e^{x} and fy⁢y=6⁢yf_{yy}=6y so that Δ=fx⁢x⁢fy⁢y-fx⁢y2=-6⁢y2⁢ex-e2⁢x\Delta=f_{xx}f_{yy}-f_{xy}^{2}=-6y^{2}e^{x}-e^{2x}. This is clearly negative for all values of x,yx,y so that any stationary point is a saddle point. (It only remains to recall that we found one stationary point for f⁢(x,y)f(x,y).)

ii) We recall that g⁢(x,y)g(x,y) has one stationary point 14325⁢(1,3)\frac{1}{\sqrt[5]{432}}(1,3). In particular, y=3⁢xy=3x at the stationary point. Now gx⁢x=2(x+y)3g_{xx}=\frac{2}{(x+y)^{3}}, gx⁢y=3⁢y2+2(x+y)3g_{xy}=3y^{2}+\frac{2}{(x+y)^{3}}, gy⁢y=6⁢x⁢y+2(x+y)3g_{yy}=6xy+\frac{2}{(x+y)^{3}}. If y=3⁢xy=3x then we have gx⁢x=264⁢x3=132⁢x3g_{xx}=\frac{2}{64x^{3}}=\frac{1}{32x^{3}}, gx⁢y=27⁢x2+132⁢x3g_{xy}=27x^{2}+\frac{1}{32x^{3}} and gy⁢y=18⁢x2+132⁢x3g_{yy}=18x^{2}+\frac{1}{32x^{3}}. Then

Δ=gx⁢x⁢gy⁢y-gx⁢y2=132⁢x3⁢(18⁢x2+132⁢x3)-(27⁢x2+132⁢x3)2=-729⁢x4-98⁢x.\Delta=g_{xx}g_{yy}-g_{xy}^{2}=\frac{1}{32x^{3}}(18x^{2}+\frac{1}{32x^{3}})-(2% 7x^{2}+\frac{1}{32x^{3}})^{2}=-729x^{4}-\frac{9}{8x}.

Thus Δ<0\Delta<0 for all x>0x>0, and in particular for the unique stationary point. Hence 14325⁢(1,3)\frac{1}{\sqrt[5]{432}}(1,3) is a saddle point for g⁢(x,y)g(x,y).

iii) Recall that h⁢(x,y)h(x,y) has three stationary points: (0,0)(0,0), (1,1)(1,1) and (1,-1)(1,-1). We have hx⁢x=6⁢xh_{xx}=6x, hx⁢y=-12⁢y3h_{xy}=-12y^{3} and hy⁢y=36⁢y2⁢(1-x)h_{yy}=36y^{2}(1-x). Therefore Δ=hx⁢x⁢hy⁢y-hx⁢y2=216⁢x⁢y2⁢(1-x)-144⁢y6\Delta=h_{xx}h_{yy}-h_{xy}^{2}=216xy^{2}(1-x)-144y^{6}. We have Δ=-144\Delta=-144 at the points (1,±1)(1,\pm 1) so that both of these are saddle points. (We have Δ=0\Delta=0 at the point (0,0)(0,0) (so that our existing methods do not allow us to determine the nature of this stationary point.)

W3.10. To find stationary points, we first look for simultaneous solutions of the equations fx=0f_{x}=0, fy=0f_{y}=0. Since

∂⁡f∂⁡x=4⁢x3-4⁢y,  and⁢∂⁡f∂⁡y=4⁢y3-4⁢x\frac{\partial f}{\partial x}=4x^{3}-4y,\;\;\;\mbox{and}\;\;\;\frac{\partial f% }{\partial y}=4y^{3}-4x

the stationary points are the points (x,y)(x,y) satisfying x3=yx^{3}=y and y3=xy^{3}=x. Then y=x3=(y3)3=y9y=x^{3}=(y^{3})^{3}=y^{9}, so y=0,1y=0,1 or -1-1. Then in these three cases we have x=y3=0,1x=y^{3}=0,1 or -1-1. So there are three stationary points: (0,0)(0,0), (1,1)(1,1) and (-1,-1)(-1,-1). To determine what types these points are, we calculate the second order partial derivatives: we have

∂2⁡f∂⁡x2=12⁢x2,  ∂2⁡f∂⁡x⁢∂⁡y=-4⁢and⁢∂2⁡f∂⁡y2=12⁢y2.\frac{\partial^{2}f}{\partial x^{2}}=12x^{2},\;\;\;\frac{\partial^{2}f}{% \partial x\partial y}=-4\;\;\;\mbox{and}\;\;\;\frac{\partial^{2}f}{\partial y^% {2}}=12y^{2}.

Thus Δ=144⁢x2⁢y2-16\Delta=144x^{2}y^{2}-16. In particular, at the points (1,1)(1,1) and (-1,-1)(-1,-1), Δ\Delta and fx⁢xf_{xx} are positive; at (0,0)(0,0), Δ\Delta is negative. So (1,1)(1,1) and (-1,-1)(-1,-1) are local minima, while (0,0)(0,0) is a saddle point.