Unit FP3: Further Pure Mathematics A2 3

Syllabus
2019
Section
—
Level
A2

FP3.1 - Hyperbolic functions

Syllabus
2019
Topic
—
Level
A2

Build hyperbolic functions from exponentials

Hyperbolic functions are combinations and ratios of exe^x and e−xe^{-x}. The two basic functions aresinh⁡x=ex−e−x2,cosh⁡x=ex+e−x2.\sinh x=\frac{e^x-e^{-x}}2,\qquad \cosh x=\frac{e^x+e^{-x}}2.The other four are ratios or reciprocals of these, so their domains and asymptotes follow from where sinh⁡x\sinh x or cosh⁡x\cosh x can be zero.

Function Exponential or reciprocal definition Main graph properties
sinh⁡x\sinh x ex−e−x2\dfrac{e^x-e^{-x}}2 Odd; domain and range R\mathbb R; passes through (0,0)(0,0).
cosh⁡x\cosh x ex+e−x2\dfrac{e^x+e^{-x}}2 Even; domain R\mathbb R; range [1,∞)[1,\infty); minimum (0,1)(0,1).
tanh⁡x\tanh x sinh⁡xcosh⁡x=e2x−1e2x+1\dfrac{\sinh x}{\cosh x}=\dfrac{e^{2x}-1}{e^{2x}+1} Odd; range (−1,1)(-1,1); horizontal asymptotes y=±1y=\pm1.
cosech⁡x\operatorname{cosech}x 1/sinh⁡x1/\sinh x Odd; x≠0x\ne0; range R∖{0}\mathbb R\setminus\{0\}.
sech⁡x\operatorname{sech}x 1/cosh⁡x=2ex+e−x1/\cosh x=\dfrac2{e^x+e^{-x}} Even; range (0,1](0,1]; horizontal asymptote y=0y=0.
coth⁡x\coth x cosh⁡x/sinh⁡x\cosh x/\sinh x Odd; x≠0x\ne0; range (−∞,−1)∪(1,∞)(-\infty,-1)\cup(1,\infty).

The fundamental identity follows directly from the exponential definitions:cosh⁡2x−sinh⁡2x=(ex+e−x)2−(ex−e−x)24=1.\cosh^2x-\sinh^2x=\frac{(e^x+e^{-x})^2-(e^x-e^{-x})^2}{4}=1.Dividing by cosh⁡2x\cosh^2x gives 1−tanh⁡2x=sech⁡2x1-\tanh^2x=\operatorname{sech}^2x; dividing by sinh⁡2x\sinh^2x gives coth⁡2x−cosech⁡2x=1\coth^2x-\operatorname{cosech}^2x=1. Also, cosh⁡2x+sinh⁡2x=cosh⁡2x\cosh^2x+\sinh^2x=\cosh2x.

sinh⁡(A+B)=sinh⁡Acosh⁡B+cosh⁡Asinh⁡B,cosh⁡(A+B)=cosh⁡Acosh⁡B+sinh⁡Asinh⁡B\sinh(A+B)=\sinh A\cosh B+\cosh A\sinh B,\qquad \cosh(A+B)=\cosh A\cosh B+\sinh A\sinh B

These addition formulae are proved by replacing every hyperbolic function with its exponential definition, expanding, and collecting eA+Be^{A+B} with e−(A+B)e^{-(A+B)}. They also allow a linear combination to be written in a shifted form. For example, Psinh⁡x+Qcosh⁡x=Rsinh⁡(x+α)P\sinh x+Q\cosh x=R\sinh(x+\alpha) when Rcosh⁡α=PR\cosh\alpha=P and Rsinh⁡α=QR\sinh\alpha=Q.

A universal route for acosh⁡x+bsinh⁡x=ca\cosh x+b\sinh x=c is to set u=ex>0u=e^x>0. Multiplying the exponential form by 2u2u gives(a+b)u2−2cu+(a−b)=0.(a+b)u^2-2cu+(a-b)=0.Solve the quadratic, reject every root with u≤0u\le0, and use x=ln⁡ux=\ln u. For example, 5cosh⁡x+3sinh⁡x=75\cosh x+3\sinh x=7 gives 4u2−7u+1=04u^2-7u+1=0, sox=ln⁡7+338orx=ln⁡7−338.x=\ln\frac{7+\sqrt{33}}8\quad\text{or}\quad x=\ln\frac{7-\sqrt{33}}8.

Hyperbolic identities resemble trigonometric ones but the signs differ: the fundamental identity is cosh⁡2x−sinh⁡2x=1\cosh^2x-\sinh^2x=1. Do not confuse sech⁡x=1/cosh⁡x\operatorname{sech}x=1/\cosh x with an inverse function, and preserve excluded points where sinh⁡x=0\sinh x=0. When using u=exu=e^x, positivity is a necessary solution condition.

Derive logarithmic forms of inverse hyperbolic functions

An inverse hyperbolic function reverses a one-to-one branch of a hyperbolic function. Its graph is the reflection of that restricted branch in y=xy=x. The prefix ar⁡\operatorname{ar} means inverse function; it does not mean reciprocal.

Principal inverse Domain Range Logarithmic form
arsinh⁡x\operatorname{arsinh}x R\mathbb R R\mathbb R ln⁡ ⁣(x+x2+1)\ln\!\left(x+\sqrt{x^2+1}\right)
arcosh⁡x\operatorname{arcosh}x [1,∞)[1,\infty) [0,∞)[0,\infty) ln⁡ ⁣(x+x2−1)\ln\!\left(x+\sqrt{x^2-1}\right)
artanh⁡x\operatorname{artanh}x (−1,1)(-1,1) R\mathbb R 12ln⁡ ⁣(1+x1−x)\dfrac12\ln\!\left(\dfrac{1+x}{1-x}\right)

To prove the official example, let y=arsinh⁡xy=\operatorname{arsinh}x, so x=sinh⁡yx=\sinh y. With u=ey>0u=e^y>0,x=u−u−12⟹u2−2xu−1=0.x=\frac{u-u^{-1}}2\quad\Longrightarrow\quad u^2-2xu-1=0.Thus u=x±x2+1u=x\pm\sqrt{x^2+1}. Since x2+1>∣x∣\sqrt{x^2+1}>|x|, only u=x+x2+1u=x+\sqrt{x^2+1} is positive. Thereforey=ln⁡u=ln⁡ ⁣(x+x2+1).y=\ln u=\ln\!\left(x+\sqrt{x^2+1}\right).

The same quadratic method gives the other forms. From x=cosh⁡yx=\cosh y with the principal restriction y≥0y\ge0, choose ey=x+x2−1e^y=x+\sqrt{x^2-1}. From x=tanh⁡yx=\tanh y, rearrangement gives e2y=(1+x)/(1−x)e^{2y}=(1+x)/(1-x), hence the factor 12\tfrac12 in artanh⁡x\operatorname{artanh}x.

Branch information matters. If cosh⁡y=x\cosh y=x with x≥1x\ge1, then bothy=±arcosh⁡xy=\pm\operatorname{arcosh}xsolve the unrestricted equation. A condition y<0y<0 selectsy=−arcosh⁡x=ln⁡ ⁣(x−x2−1),y=-\operatorname{arcosh}x=\ln\!\left(x-\sqrt{x^2-1}\right),because the two positive exponential roots are reciprocals.

Because sinh⁡\sinh and tanh⁡\tanh are odd, arsinh⁡\operatorname{arsinh} and artanh⁡\operatorname{artanh} are odd. The principal arcosh⁡\operatorname{arcosh} graph begins at (1,0)(1,0) and is increasing. The logarithmic forms make exact equation solutions possible without treating inverse values as decimal approximations.

Always state the domain before using a logarithmic form: arcosh⁡x\operatorname{arcosh}x requires x≥1x\ge1, and real artanh⁡x\operatorname{artanh}x requires ∣x∣<1|x|<1. Do not write arsinh⁡x=1/sinh⁡x\operatorname{arsinh}x=1/\sinh x; the reciprocal is cosech⁡x\operatorname{cosech}x. For an unrestricted even function such as cosh⁡\cosh, include both branches unless a sign condition selects one.

FP3.2 - Further coordinate systems

Syllabus
2019
Topic
—
Level
A2

Move between equations and parameters for conics

A standard ellipse or hyperbola is centred at the origin with its transverse or major axis on the xx-axis. Assume a>0a>0 and b>0b>0. The signs in the Cartesian equation identify the curve: an ellipse has a sum equal to 11, while a hyperbola has a difference equal to 11. A parametric pair describes points on the curve using one parameter and is often the cleanest form for differentiation or moving-point problems.

Curve Cartesian equation Standard parametrisation Parameter coverage
Ellipse x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 x=acos⁡t, y=bsin⁡tx=a\cos t,\ y=b\sin t 0≤t<2π0\le t<2\pi traces the ellipse once.
Hyperbola x2a2−y2b2=1\dfrac{x^2}{a^2}-\dfrac{y^2}{b^2}=1 x=asec⁡t, y=btan⁡tx=a\sec t,\ y=b\tan t Values with cos⁡t≠0\cos t\ne0 cover both branches; different intervals select a branch.
Hyperbola, right branch x2a2−y2b2=1\dfrac{x^2}{a^2}-\dfrac{y^2}{b^2}=1 x=acosh⁡t, y=bsinh⁡tx=a\cosh t,\ y=b\sinh t t∈Rt\in\mathbb R gives x≥ax\ge a only; changing xx to −acosh⁡t-a\cosh t gives the left branch.

Verify a parametrisation by substitution. For the ellipse,(acos⁡t)2a2+(bsin⁡t)2b2=cos⁡2t+sin⁡2t=1.\frac{(a\cos t)^2}{a^2}+\frac{(b\sin t)^2}{b^2}=\cos^2t+\sin^2t=1.For the trigonometric hyperbola parametrisation, the corresponding identity is sec⁡2t−tan⁡2t=1\sec^2t-\tan^2t=1; for the hyperbolic parametrisation it is cosh⁡2t−sinh⁡2t=1\cosh^2t-\sinh^2t=1. This check also explains why the same parameter must appear in both coordinates.

To remove a parameter, first isolate functions of it and then use the matching identity. If x=4cos⁡tx=4\cos t and y=3sin⁡ty=3\sin t, then cos⁡t=x/4\cos t=x/4 and sin⁡t=y/3\sin t=y/3, sox216+y29=1.\frac{x^2}{16}+\frac{y^2}{9}=1.The coordinate bounds ∣x∣≤4|x|\le4 and ∣y∣≤3|y|\le3 follow from the parametrisation as well as from the ellipse.

A Cartesian equation is usually better for intersections. Substitute the equation of the line into the conic to obtain a quadratic in one coordinate. Its two roots represent the two intersection coordinates; their sum and product can locate a midpoint or build a symmetric expression without solving for each point separately. Return to the line equation for the other coordinate, and check that every resulting point lies on both curves.

If a conic is translated, replace xx and yy by displacements from its centre. For example,(x−h)2a2+(y−k)2b2=1\frac{(x-h)^2}{a^2}+\frac{(y-k)^2}{b^2}=1has parametrisation x=h+acos⁡tx=h+a\cos t, y=k+bsin⁡ty=k+b\sin t. Complete squares before reading a centre or semi-axis from a non-standard Cartesian equation.

Do not confuse aa and bb with their squares in the denominators. Eliminating a parameter can lose its interval restriction, so a Cartesian equation may describe more points than the original parametrisation. In particular, x=acosh⁡tx=a\cosh t, y=bsinh⁡ty=b\sinh t describes only the right branch even though its eliminated equation contains two branches.

Use focus, directrix and eccentricity

For a fixed focus SS and directrix ℓ\ell, a conic is the locus of points PP satisfyingPS=e d(P,ℓ),PS=e\,d(P,\ell),where e>0e>0 is the eccentricity and d(P,ℓ)d(P,\ell) is the perpendicular distance to the line. An ellipse has 0<e<10<e<1 and a hyperbola has e>1e>1. For the standard horizontal conics, the foci and directrices occur in symmetric pairs on the xx-axis.

Curve Relation between a,b,ea,b,e Foci Directrices
x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 b2=a2(1−e2)b^2=a^2(1-e^2), so e=1−b2/a2e=\sqrt{1-b^2/a^2} (±ae,0)(\pm ae,0) x=±a/ex=\pm a/e
x2a2−y2b2=1\dfrac{x^2}{a^2}-\dfrac{y^2}{b^2}=1 b2=a2(e2−1)b^2=a^2(e^2-1), so e=1+b2/a2e=\sqrt{1+b^2/a^2} (±ae,0)(\pm ae,0) x=±a/ex=\pm a/e

The focus is farther from the centre than the corresponding vertex for a hyperbola because e>1e>1, but nearer for an ellipse because e<1e<1. Thus the quantities aeae and a/ea/e switch their relative sizes: for an ellipse ae<a<a/eae<a<a/e, whereas for a hyperbola a/e<a<aea/e<a<ae. This is a useful geometric check on calculated coordinates and directrices.

The ellipse relation can be recovered from the locus definition. Use the right focus S=(ae,0)S=(ae,0) and right directrix x=a/ex=a/e. For P=(x,y)P=(x,y) on the appropriate side of that directrix,(x−ae)2+y2=e2(x−ae)2.(x-ae)^2+y^2=e^2\left(x-\frac ae\right)^2.Expansion cancels the linear terms and gives(1−e2)x2+y2=a2(1−e2).(1-e^2)x^2+y^2=a^2(1-e^2).Dividing through and comparing with x2/a2+y2/b2=1x^2/a^2+y^2/b^2=1 yields b2=a2(1−e2)b^2=a^2(1-e^2). The same distance principle, with e>1e>1, gives the hyperbola relation.

Given any two compatible focus-directrix quantities, solve systematically. If a hyperbola has focus distance ae=10ae=10 and directrix distance a/e=5/2a/e=5/2, then a2=(ae)(a/e)=25a^2=(ae)(a/e)=25, so a=5a=5, e=2e=2, andb2=a2(e2−1)=75.b^2=a^2(e^2-1)=75.Its standard equation is therefore x2/25−y2/75=1x^2/25-y^2/75=1. The positive square root is used because eccentricity and semi-axis length are positive.

These displayed formulae assume a horizontal major or transverse axis. For a vertical conic, the roles of xx and yy swap: the foci lie at (0,±ae)(0,\pm ae) and the directrices are y=±a/ey=\pm a/e. Identify the axis from the equation before applying a memorised coordinate pattern.

Do not use the ellipse sign in the eccentricity relation for a hyperbola, and do not report e=±⋯e=\pm\sqrt{\cdots}: eccentricity is positive. The focus-directrix definition uses perpendicular distance, which is non-negative; squaring an equation of distances may introduce points on the wrong side unless the relevant branch or region is checked.

Find tangents and normals to ellipses and hyperbolas

A tangent has the curve's instantaneous gradient at the point of contact; a normal is perpendicular to it. There are two complementary routes. Use differentiation when the contact point is known or parametrised. Use a repeated-root condition when a line y=mx+cy=mx+c is required to touch a conic at exactly one point.

Curve and point Tangent equation
Ellipse at (acos⁡t,bsin⁡t)(a\cos t,b\sin t) xcos⁡ta+ysin⁡tb=1\dfrac{x\cos t}{a}+\dfrac{y\sin t}{b}=1
Hyperbola at (asec⁡t,btan⁡t)(a\sec t,b\tan t) xsec⁡ta−ytan⁡tb=1\dfrac{x\sec t}{a}-\dfrac{y\tan t}{b}=1
Hyperbola at (acosh⁡t,bsinh⁡t)(a\cosh t,b\sinh t) xcosh⁡ta−ysinh⁡tb=1\dfrac{x\cosh t}{a}-\dfrac{y\sinh t}{b}=1

For the ellipse x2/a2+y2/b2=1x^2/a^2+y^2/b^2=1, implicit differentiation givesdydx=−b2xa2y.\frac{dy}{dx}=-\frac{b^2x}{a^2y}.At (acos⁡t,bsin⁡t)(a\cos t,b\sin t) this is −bcos⁡t/(asin⁡t)-b\cos t/(a\sin t). Substitution in point-gradient form and simplification produces the tangent in the table. The normal gradient is the negative reciprocal, asin⁡t/(bcos⁡t)a\sin t/(b\cos t), provided neither relevant gradient is vertical.

Parametric differentiation gives the same result without first eliminating tt:dydx=dy/dtdx/dt.\frac{dy}{dx}=\frac{dy/dt}{dx/dt}.For x=asec⁡tx=a\sec t, y=btan⁡ty=b\tan t, this gives dy/dx=bsec⁡2t/(asec⁡ttan⁡t)dy/dx=b\sec^2t/(a\sec t\tan t). Keep the contact point attached to the same parameter value when writing the line through it.

ellipse: c2=a2m2+b2,hyperbola: c2=a2m2−b2\text{ellipse: }c^2=a^2m^2+b^2,\qquad \text{hyperbola: }c^2=a^2m^2-b^2

These conditions for y=mx+cy=mx+c come from substituting the line into the Cartesian conic and setting the resulting quadratic discriminant to zero. For example, tangents of slope 3/43/4 to x2/16+y2/9=1x^2/16+y^2/9=1 satisfyc2=16(34)2+9=18,c^2=16\left(\frac34\right)^2+9=18,so the two parallel tangents are y=34x±32y=\tfrac34x\pm3\sqrt2. A line through a specified external point supplies a second equation relating mm and cc.

After finding a tangent, recover its contact point by solving the line and conic simultaneously. Because the intersection is a repeated root, the quadratic should have one repeated coordinate; substitution gives the other coordinate. This is also a check that the proposed line really touches rather than cuts the curve.

The family y=mx+cy=mx+c does not include vertical tangents, such as x=±ax=\pm a at the horizontal vertices. A zero tangent gradient gives a vertical normal, so the negative-reciprocal rule must be interpreted geometrically rather than used as division by zero. The hyperbola tangent condition can have no real cc for some slopes; require a2m2−b2≥0a^2m^2-b^2\ge0.

Eliminate a parameter to determine a locus

A locus records every position a moving point can occupy. In a coordinate problem, first express the moving point as (x(t),y(t))(x(t),y(t)) from the geometry; then eliminate tt to obtain a Cartesian relation. The relation is not the whole answer until restrictions inherited from the parameter and construction have been checked.

Step Question to answer
1. Coordinate What are xx and yy in terms of the same parameter?
2. Isolate Which simple expressions in the parameter equal functions of xx and yy?
3. Eliminate Which identity or algebraic relation removes the parameter?
4. Simplify Can the result be written as a recognisable conic or requested polynomial form?
5. Restrict and verify Does the construction trace the whole curve, one branch, one arc, or omit points?

Suppose a moving midpoint has coordinatesx=2+3cos⁡t,y=−1+2sin⁡t.x=2+3\cos t,\qquad y=-1+2\sin t.Then cos⁡t=(x−2)/3\cos t=(x-2)/3 and sin⁡t=(y+1)/2\sin t=(y+1)/2. Using cos⁡2t+sin⁡2t=1\cos^2t+\sin^2t=1 gives the locus(x−2)29+(y+1)24=1.\frac{(x-2)^2}{9}+\frac{(y+1)^2}{4}=1.If tt ranges through a full 2π2\pi interval, the whole ellipse is traced; a smaller interval would select only part of it.

When coordinates are rational functions of a parameter, avoid solving unnecessarily complicated equations. Ifx=6uu2+1,y=3(1−u2)u2+1,x=\frac{6u}{u^2+1},\qquad y=\frac{3(1-u^2)}{u^2+1},then direct calculation gives x2/9+y2/9=1x^2/9+y^2/9=1. The missing or repeated points must still be checked from the original expressions; algebraic elimination alone does not record how the curve is traced.

Points created from intersections, midpoints or perpendicular lines should be built in layers. Find the defining lines or intersection coordinates first; use root sums for a midpoint when two intersections are roots of one quadratic; then eliminate the moving parameter. This keeps each geometric condition visible and prevents an unexplained leap to the final equation.

After elimination, complete squares and normalise to recognise the curve. For example,4x2+9y2+18y=274x^2+9y^2+18y=27becomesx29+(y+1)24=1.\frac{x^2}{9}+\frac{(y+1)^2}{4}=1.A correct locus equation should be tested by substituting the original parametric coordinates back into it identically.

Squaring, dividing by an expression that may be zero, or using a many-to-one trigonometric identity can add or remove solutions. Record parameter intervals, denominator exclusions and sign conditions before elimination, then test boundary values separately. A Cartesian equation with no restriction can overstate the locus.

FP3.3 - Differentiation

Syllabus
2019
Topic
—
Level
A2

Differentiate hyperbolic functions and combinations

Hyperbolic derivatives follow from the exponential definitions and then obey the usual chain, product, quotient and reciprocal rules. The key pair mirrors differentiation of exe^x:ddxsinh⁡x=cosh⁡x,ddxcosh⁡x=sinh⁡x.\frac{d}{dx}\sinh x=\cosh x,\qquad \frac{d}{dx}\cosh x=\sinh x.Unlike trigonometric differentiation, differentiating cosh⁡x\cosh x does not introduce a minus sign.

f(u)f(u) ddxf(u)\dfrac{d}{dx}f(u), where u=u(x)u=u(x)
sinh⁡u\sinh u u′cosh⁡uu'\cosh u
cosh⁡u\cosh u u′sinh⁡uu'\sinh u
tanh⁡u\tanh u u′sech⁡2uu'\operatorname{sech}^2u
coth⁡u\coth u −u′cosech⁡2u-u'\operatorname{cosech}^2u
sech⁡u\operatorname{sech}u −u′sech⁡utanh⁡u-u'\operatorname{sech}u\tanh u
cosech⁡u\operatorname{cosech}u −u′cosech⁡ucoth⁡u-u'\operatorname{cosech}u\coth u

For example, the quotient rule and cosh⁡2u−sinh⁡2u=1\cosh^2u-\sinh^2u=1 giveddutanh⁡u=cosh⁡2u−sinh⁡2ucosh⁡2u=sech⁡2u.\frac{d}{du}\tanh u=\frac{\cosh^2u-\sinh^2u}{\cosh^2u}=\operatorname{sech}^2u.The reciprocal rule then gives the negative sign in d(sech⁡u)/du=−sech⁡utanh⁡ud(\operatorname{sech}u)/du=-\operatorname{sech}u\tanh u. These derivations are safer than importing trigonometric signs by memory.

Differentiate the outside function, keep its argument, then multiply by the derivative of that argument. Thusddxtanh⁡(5x−1)=5sech⁡2(5x−1),\frac{d}{dx}\tanh(5x-1)=5\operatorname{sech}^2(5x-1),andddxsech⁡(x2)=−2xsech⁡(x2)tanh⁡(x2).\frac{d}{dx}\operatorname{sech}(x^2)=-2x\operatorname{sech}(x^2)\tanh(x^2).Every nested layer contributes a factor.

For a product such as y=xsinh⁡2xy=x\sinh^2x, keep both product-rule terms and apply a second chain rule to the square:dydx=sinh⁡2x+2xsinh⁡xcosh⁡x=sinh⁡2x+xsinh⁡2x.\frac{dy}{dx}=\sinh^2x+2x\sinh x\cosh x=\sinh^2x+x\sinh2x.The identity 2sinh⁡xcosh⁡x=sinh⁡2x2\sinh x\cosh x=\sinh2x is an optional final simplification, not a replacement for the differentiation steps.

Write powers explicitly before differentiating a quotient. Ify=cosh⁡2xx+1=cosh⁡(2x)(x+1)−1/2,x>−1,y=\frac{\cosh2x}{\sqrt{x+1}}=\cosh(2x)(x+1)^{-1/2},\qquad x>-1,thendydx=2sinh⁡(2x)(x+1)−1/2−12cosh⁡(2x)(x+1)−3/2.\frac{dy}{dx}=2\sinh(2x)(x+1)^{-1/2}-\frac12\cosh(2x)(x+1)^{-3/2}.A common denominator may be formed only after both terms are correct.

Do not copy the circular-function pattern d(cos⁡x)/dx=−sin⁡xd(\cos x)/dx=-\sin x onto cosh⁡x\cosh x. Distinguish sinh⁡2x=(sinh⁡x)2\sinh^2x=(\sinh x)^2 from sinh⁡(x2)\sinh(x^2), and do not omit the inner derivative. Retain any domain restriction created by denominators, square roots, coth⁡\coth or cosech⁡\operatorname{cosech}.

Differentiate inverse trigonometric and hyperbolic functions

If y=f−1(x)y=f^{-1}(x) on a one-to-one branch of ff, then x=f(y)x=f(y) and implicit differentiation givesdydx=1f′(y).\frac{dy}{dx}=\frac{1}{f'(y)}.Rewrite the result in terms of xx using the defining identity and the principal range. The branch and domain are part of the derivative formula, especially when a square root appears.

Function of u=u(x)u=u(x) Derivative Real differentiability condition
arcsin⁡u\arcsin u u′1−u2\dfrac{u'}{\sqrt{1-u^2}} ∣u∣<1|u|<1
arccos⁡u\arccos u −u′1−u2-\dfrac{u'}{\sqrt{1-u^2}} ∣u∣<1|u|<1
arctan⁡u\arctan u u′1+u2\dfrac{u'}{1+u^2} all real uu
arsinh⁡u\operatorname{arsinh}u u′1+u2\dfrac{u'}{\sqrt{1+u^2}} all real uu
arcosh⁡u\operatorname{arcosh}u u′u2−1\dfrac{u'}{\sqrt{u^2-1}} u>1u>1
artanh⁡u\operatorname{artanh}u u′1−u2\dfrac{u'}{1-u^2} ∣u∣<1|u|<1

To derive the inverse-sinh result, let y=arsinh⁡xy=\operatorname{arsinh}x, so x=sinh⁡yx=\sinh y. Then1=cosh⁡ydydx⟹dydx=1cosh⁡y.1=\cosh y\frac{dy}{dx}\quad\Longrightarrow\quad\frac{dy}{dx}=\frac1{\cosh y}.Because cosh⁡y>0\cosh y>0 and cosh⁡2y=1+sinh⁡2y\cosh^2y=1+\sinh^2y, this becomesddxarsinh⁡x=11+x2.\frac{d}{dx}\operatorname{arsinh}x=\frac1{\sqrt{1+x^2}}.The positive square root is justified by the principal range, not chosen arbitrarily.

For a composite inverse function, differentiate the complete inner expression. For example, if y=arcosh⁡(2x+3)y=\operatorname{arcosh}(2x+3) and x>−1x>-1, thendydx=2(2x+3)2−1.\frac{dy}{dx}=\frac{2}{\sqrt{(2x+3)^2-1}}.The stricter condition 2x+3>12x+3>1 ensures the derivative is finite; the function itself is defined at the endpoint where 2x+3=12x+3=1, but its derivative formula is singular there.

Useful simplification often appears only after applying the rule. Fory=arcsin⁡x+x1−x2,∣x∣<1,y=\arcsin x+x\sqrt{1-x^2},\qquad |x|<1,the product and chain rules givedydx=11−x2+1−x2−x21−x2=21−x2.\frac{dy}{dx}=\frac1{\sqrt{1-x^2}}+\sqrt{1-x^2}-\frac{x^2}{\sqrt{1-x^2}}=2\sqrt{1-x^2}.Keeping a common radical visible makes the cancellation reliable.

When simplifying radicals, use x2=∣x∣\sqrt{x^2}=|x|, not automatically xx. For example,ddxarsinh⁡ ⁣(4x2−1)=2x∣x∣4x2−1,∣x∣>12.\frac{d}{dx}\operatorname{arsinh}\!\left(\sqrt{4x^2-1}\right)=\frac{2x}{|x|\sqrt{4x^2-1}},\qquad |x|>\frac12.This equals 2/4x2−12/\sqrt{4x^2-1} for x>1/2x>1/2 but −2/4x2−1-2/\sqrt{4x^2-1} for x<−1/2x<-1/2. A stated domain decides the sign.

After differentiating a combination, solve f′(x)=0f'(x)=0 within the original domain. If clearing radicals requires squaring, the resulting equation is only a candidate equation: substitute each candidate back into the unsquared derivative equation and reject values outside the inverse-function or radical domain.

The prefix ar⁡\operatorname{ar} denotes an inverse function, not a reciprocal. Do not confuse arsinh⁡x\operatorname{arsinh}x with cosech⁡x\operatorname{cosech}x, or artanh⁡x\operatorname{artanh}x with 1/tanh⁡x1/\tanh x. State the real domain before simplifying roots or solving stationary-point equations, and remember the inner derivative in every composite.

FP3.4 - Integration

Syllabus
2019
Topic
—
Level
A2

Integrate hyperbolic functions and expressions

Hyperbolic antiderivatives reverse the derivative patterns from FP3.3. First recognise whether the integrand contains a function together with the derivative of its argument; then account for any constant chain factor. Always add CC to an indefinite integral.

Integrand pattern, u=u(x)u=u(x) Antiderivative
u′sinh⁡uu'\sinh u cosh⁡u+C\cosh u+C
u′cosh⁡uu'\cosh u sinh⁡u+C\sinh u+C
u′sech⁡2uu'\operatorname{sech}^2u tanh⁡u+C\tanh u+C
u′cosech⁡2uu'\operatorname{cosech}^2u −coth⁡u+C-\coth u+C
u′sech⁡utanh⁡uu'\operatorname{sech}u\tanh u −sech⁡u+C-\operatorname{sech}u+C
u′cosech⁡ucoth⁡uu'\operatorname{cosech}u\coth u −cosech⁡u+C-\operatorname{cosech}u+C

Ratios lead to logarithms because d(ln⁡∣f∣)/dx=f′/fd(\ln|f|)/dx=f'/f:∫tanh⁡x dx=ln⁡(cosh⁡x)+C,\int\tanh x\,dx=\ln(\cosh x)+C,∫coth⁡x dx=ln⁡∣sinh⁡x∣+C.\int\coth x\,dx=\ln|\sinh x|+C.The absolute value is needed in the second result because sinh⁡x\sinh x may be negative; cosh⁡x\cosh x is always positive.

Two useful single-function forms follow by differentiating the inverse expression:∫sech⁡x dx=arctan⁡(sinh⁡x)+C,\int\operatorname{sech}x\,dx=\arctan(\sinh x)+C,∫cosech⁡x dx=ln⁡∣tanh⁡x2∣+C.\int\operatorname{cosech}x\,dx=\ln\left|\tanh\frac{x}{2}\right|+C.These apply only on intervals where the integrand is defined.

For∫(3cosh⁡(3x)−2sech⁡2(2x))dx,\int\left(3\cosh(3x)-2\operatorname{sech}^2(2x)\right)dx,each inner derivative is already present, so the result issinh⁡(3x)−tanh⁡(2x)+C.\sinh(3x)-\tanh(2x)+C.Differentiate the result: 3cosh⁡(3x)−2sech⁡2(2x)3\cosh(3x)-2\operatorname{sech}^2(2x) is recovered exactly.

Expressions involving powers may need an identity before integration. For example,cosh⁡2x=1+cosh⁡2x2,sinh⁡2x=cosh⁡2x−12.\cosh^2x=\frac{1+\cosh2x}{2},\qquad \sinh^2x=\frac{\cosh2x-1}{2}.Thus ∫cosh⁡2x dx=x/2+sinh⁡2x/4+C\int\cosh^2x\,dx=x/2+\sinh2x/4+C. Choose an identity that turns the integrand into direct patterns rather than expanding exponentials unnecessarily.

Do not integrate tanh⁡x\tanh x as ln⁡∣sinh⁡x∣\ln|\sinh x|; its numerator is the derivative of cosh⁡x\cosh x, not sinh⁡x\sinh x. Preserve negative signs in reciprocal-function patterns, divide by constant inner derivatives when they are absent, and keep singular points of coth⁡\coth and cosech⁡\operatorname{cosech} outside the interval.

Integrate inverse trigonometric and hyperbolic functions

An inverse trigonometric or inverse hyperbolic function is usually integrated by parts. Choose the inverse function as the part to differentiate and 11 as the part to integrate:u=f−1(x),dv=dx.u=f^{-1}(x),\qquad dv=dx.Its derivative becomes an algebraic expression that can be simplified or integrated directly.

Integral Result
∫arcsin⁡x dx\int\arcsin x\,dx xarcsin⁡x+1−x2+Cx\arcsin x+\sqrt{1-x^2}+C
∫arctan⁡x dx\int\arctan x\,dx xarctan⁡x−12ln⁡(1+x2)+Cx\arctan x-\tfrac12\ln(1+x^2)+C
∫arsinh⁡x dx\int\operatorname{arsinh}x\,dx xarsinh⁡x−1+x2+Cx\operatorname{arsinh}x-\sqrt{1+x^2}+C
∫arcosh⁡x dx\int\operatorname{arcosh}x\,dx xarcosh⁡x−x2−1+Cx\operatorname{arcosh}x-\sqrt{x^2-1}+C, x≥1x\ge1
∫artanh⁡x dx\int\operatorname{artanh}x\,dx xartanh⁡x+12ln⁡(1−x2)+Cx\operatorname{artanh}x+\tfrac12\ln(1-x^2)+C, ∣x∣<1|x|<1

For example,∫arsinh⁡x dx=xarsinh⁡x−∫x1+x2 dx.\int\operatorname{arsinh}x\,dx=x\operatorname{arsinh}x-\int\frac{x}{\sqrt{1+x^2}}\,dx.With w=1+x2w=1+x^2, the remaining integral is 1+x2\sqrt{1+x^2}, givingxarsinh⁡x−1+x2+C.x\operatorname{arsinh}x-\sqrt{1+x^2}+C.Differentiating this result makes the two x/1+x2x/\sqrt{1+x^2} terms cancel.

For a scaled argument, substitute first or apply integration by parts with the full argument. If a>0a>0, then∫arctan⁡(xa)dx=xarctan⁡(xa)−a2ln⁡(a2+x2)+C.\int\arctan\left(\frac{x}{a}\right)dx=x\arctan\left(\frac{x}{a}\right)-\frac a2\ln(a^2+x^2)+C.Terms differing only by a constant inside a logarithm are absorbed into CC.

For a definite integral, use one antiderivative consistently and retain exact principal inverse values. Check that the complete interval lies in the real domain: [−1,1][-1,1] for arcsin⁡x\arcsin x, [1,∞)[1,\infty) for arcosh⁡x\operatorname{arcosh}x, and (−1,1)(-1,1) for artanh⁡x\operatorname{artanh}x.

The superscript notation sinh⁡−1x\sinh^{-1}x means the inverse function here, not 1/sinh⁡x1/\sinh x. Do not omit the xf−1(x)x f^{-1}(x) term produced by integration by parts, and do not discard the domain merely because the final algebraic expression contains familiar logarithms or roots.

Choose trigonometric or hyperbolic substitutions

A substitution is chosen so that a standard identity removes a quadratic expression. Assume a>0a>0. Trigonometric substitutions are natural for a2−x2a^2-x^2 and a2+x2a^2+x^2; hyperbolic substitutions give equally direct forms for positive sums and differences. Transform the differential and limits as well as the integrand.

Target form Useful substitution Identity used Standard antiderivative
1a2+x2\dfrac1{a^2+x^2} x=atan⁡θx=a\tan\theta 1+tan⁡2θ=sec⁡2θ1+\tan^2\theta=\sec^2\theta 1aarctan⁡(x/a)+C\dfrac1a\arctan(x/a)+C
1a2−x2\dfrac1{\sqrt{a^2-x^2}} x=asin⁡θx=a\sin\theta 1−sin⁡2θ=cos⁡2θ1-\sin^2\theta=\cos^2\theta arcsin⁡(x/a)+C\arcsin(x/a)+C
1a2+x2\dfrac1{\sqrt{a^2+x^2}} x=asinh⁡tx=a\sinh t 1+sinh⁡2t=cosh⁡2t1+\sinh^2t=\cosh^2t arsinh⁡(x/a)+C\operatorname{arsinh}(x/a)+C
1x2−a2\dfrac1{\sqrt{x^2-a^2}} x=acosh⁡tx=a\cosh t for x≥ax\ge a cosh⁡2t−1=sinh⁡2t\cosh^2t-1=\sinh^2t arcosh⁡(x/a)+C\operatorname{arcosh}(x/a)+C

Use the same four moves each time: choose the identity-matching substitution; calculate dxdx; replace every occurrence of xx; simplify the square root with the parameter range that fixes its sign. For a definite integral, convert both bounds immediately and evaluate in the new variable without back-substituting.

For 0<b<a0<b<a,∫0bdx(a2−x2)3/2\int_0^b\frac{dx}{(a^2-x^2)^{3/2}}uses x=asin⁡θx=a\sin\theta, dx=acos⁡θ dθdx=a\cos\theta\,d\theta, with 0≤θ<π/20\le\theta<\pi/2. Since (a2−x2)3/2=a3cos⁡3θ(a^2-x^2)^{3/2}=a^3\cos^3\theta, the integral becomes1a2∫0arcsin⁡(b/a)sec⁡2θ dθ=ba2a2−b2.\frac1{a^2}\int_0^{\arcsin(b/a)}\sec^2\theta\,d\theta=\frac{b}{a^2\sqrt{a^2-b^2}}.The range justifies replacing cos⁡2θ\sqrt{\cos^2\theta} by cos⁡θ\cos\theta.

A hyperbolic substitution can be especially clean when a2+x2\sqrt{a^2+x^2} or x2−a2\sqrt{x^2-a^2} appears because the radical becomes acosh⁡ta\cosh t or asinh⁡ta\sinh t. A trigonometric route may instead be preferable when exact angle values make definite limits simple. The valid method is the one whose identity matches the sign pattern and whose range is controlled.

Do not transform only the radical: dxdx and all limits must change too. The equality a2cos⁡2θ=acos⁡θ\sqrt{a^2\cos^2\theta}=a\cos\theta requires a range with cos⁡θ≥0\cos\theta\ge0; otherwise it is a∣cos⁡θ∣a|\cos\theta|. Check the original radical domain before choosing or evaluating bounds.

Use substitution with quadratic surds

For an integral involving Ax2+Bx+C\sqrt{Ax^2+Bx+C}, expose the quadratic's geometry before substituting. Complete the square, factor out any positive constant, and identify one of the patterns a2−u2a^2-u^2, a2+u2a^2+u^2 or u2−a2u^2-a^2. In more complicated cases the required substitution may be supplied, but every algebraic change must still be shown.

Step Required action
1. Normalise Complete the square and factor constants from the surd.
2. Choose Match the sign pattern to u=asin⁡θu=a\sin\theta, u=asinh⁡tu=a\sinh t, u=atan⁡θu=a\tan\theta or u=acosh⁡tu=a\cosh t.
3. Transform Find dudu or dxdx and rewrite the entire integrand.
4. Integrate Simplify using the matching identity and integrate in the new variable.
5. Return/check Back-substitute, or transform bounds for a definite integral; differentiate to verify.

Consider∫dxx2+6x+13.\int\frac{dx}{\sqrt{x^2+6x+13}}.Completing the square gives (x+3)2+4(x+3)^2+4. Put x+3=2sinh⁡tx+3=2\sinh t, so dx=2cosh⁡t dtdx=2\cosh t\,dt and the denominator is 2cosh⁡t2\cosh t. The integral is ∫dt\int dt, hencearsinh⁡(x+32)+C.\operatorname{arsinh}\left(\frac{x+3}{2}\right)+C.Differentiation recovers the original integrand.

If the numerator contains the derivative 2Ax+B2Ax+B of the quadratic, try the direct substitution u=Ax2+Bx+Cu=Ax^2+Bx+C before a trigonometric or hyperbolic substitution. For example,∫2x+4x2+4x+7 dx=2x2+4x+7+C.\int\frac{2x+4}{\sqrt{x^2+4x+7}}\,dx=2\sqrt{x^2+4x+7}+C.This is shorter because the numerator already supplies dudu.

When a non-obvious substitution is given, derive its consequences rather than guessing the target. Calculate dxdx, rewrite the surd, state the parameter range needed for its sign, and simplify systematically. For definite integrals, translate endpoints before cancellation so that orientation and sign remain visible.

Completing the square changes form, not domain. Never replace u2\sqrt{u^2} by uu without a range or sign statement, and do not divide by a substituted factor that may be zero. This objective covers substitution for quadratic surds; unrelated rational substitutions and numerical integration are outside this card.

Derive and use reduction formulae

A reduction formula rewrites an integral indexed by nn in terms of the same family with a smaller index. It is derived from the definition of the indexed integral, usually by integration by parts and an identity. State the definition, restrictions and base cases before using the recurrence.

LetIn=∫0π/2sin⁡nx dx.I_n=\int_0^{\pi/2}\sin^n x\,dx.For n≥2n\ge2, write sin⁡nx=sin⁡n−1xsin⁡x\sin^n x=\sin^{n-1}x\sin x and integrate by parts with u=sin⁡n−1xu=\sin^{n-1}x, dv=sin⁡x dxdv=\sin x\,dx. The boundary term [−sin⁡n−1xcos⁡x]0π/2[-\sin^{n-1}x\cos x]_0^{\pi/2} is zero.

The remaining integral is(n−1)∫0π/2sin⁡n−2xcos⁡2x dx=(n−1)(In−2−In).(n-1)\int_0^{\pi/2}\sin^{n-2}x\cos^2x\,dx=(n-1)(I_{n-2}-I_n).ThereforenIn=(n−1)In−2,n≥2.nI_n=(n-1)I_{n-2},\qquad n\ge2.Use I0=π/2I_0=\pi/2 for even powers and I1=1I_1=1 for odd powers. For instance, I4=(3/4)I2=(3/4)(1/2)I0=3π/16I_4=(3/4)I_2=(3/4)(1/2)I_0=3\pi/16.

A different family needs a different derivation. IfJn=∫sin⁡nxsin⁡x dx,n>0,J_n=\int\frac{\sin nx}{\sin x}\,dx,\qquad n>0,then sin⁡((n+2)x)−sin⁡(nx)=2cos⁡((n+1)x)sin⁡x\sin((n+2)x)-\sin(nx)=2\cos((n+1)x)\sin x. Dividing by sin⁡x\sin x and integrating givesJn+2=2sin⁡((n+1)x)n+1+Jn.J_{n+2}=\frac{2\sin((n+1)x)}{n+1}+J_n.This is an indefinite relation, so use a consistent arbitrary constant convention.

For an unfamiliar indexed family, choose integration by parts so that one factor differentiates toward the lower-index integrand. Rewrite leftover powers using an identity, isolate every occurrence of the original InI_n, and only then divide to obtain the recurrence. To evaluate, step down repeatedly until a directly calculable base integral is reached.

A recurrence is not valid outside the stated index range, and even/odd chains can have different base cases. Do not use a printed formula without matching its definition and limits. In a derivation, include the boundary term and justify why it vanishes; in an indefinite recurrence, remember that constants of integration are not independent at each line.

Calculate arc length and surfaces of revolution

Arc length adds infinitesimal distances dsds along a curve. A surface of revolution adds circumference times arc length, so the radius is the perpendicular distance from the curve to the axis. The specification covers Cartesian and parametric curves, not polar forms.

Situation Formula on the stated interval
Cartesian y=f(x)y=f(x) s=∫ab1+(dy/dx)2 dxs=\int_a^b\sqrt{1+(dy/dx)^2}\,dx
Cartesian x=g(y)x=g(y) s=∫cd1+(dx/dy)2 dys=\int_c^d\sqrt{1+(dx/dy)^2}\,dy
Parametric (x(t),y(t))(x(t),y(t)) s=∫αβ(dx/dt)2+(dy/dt)2 dts=\int_\alpha^\beta\sqrt{(dx/dt)^2+(dy/dt)^2}\,dt
Curved surface about the xx-axis S=2π∫∣y∣ dsS=2\pi\int |y|\,ds
Curved surface about the yy-axis S=2π∫∣x∣ dsS=2\pi\int |x|\,ds

First differentiate and simplify the speed factor under the square root. Then determine the radius and parameter interval. Use absolute values or split the interval if the signed coordinate crosses the axis. The square root denotes non-negative speed, so h(t)2=∣h(t)∣\sqrt{h(t)^2}=|h(t)| unless its sign is established.

Forx=t−t33,y=t2,0≤t≤1,x=t-\frac{t^3}{3},\qquad y=t^2,\qquad 0\le t\le1,we have dx/dt=1−t2dx/dt=1-t^2 and dy/dt=2tdy/dt=2t, sodsdt=(1−t2)2+4t2=1+t2.\frac{ds}{dt}=\sqrt{(1-t^2)^2+4t^2}=1+t^2.Hence the arc length is [t+t3/3]01=4/3[t+t^3/3]_0^1=4/3. Rotating the curve about the xx-axis gives curved area$2\pi\int_0^1t^2(1+t^2)dt=\frac{16\pi}{15}.

The formula 2π∫r ds2\pi\int r\,ds gives only the curved surface swept out by the curve. If a solid's total surface area is requested and the endpoints generate circular end faces, add the appropriate disc or annulus areas separately. Read the geometry and endpoint radii before deciding whether end faces exist.

Length has units of length and surface area has squared units. Both must be non-negative. For a definite calculation, verify that the parameter traces the intended piece once; retracing a segment would count its length or swept area again.

Do not confuse arc length with area under a curve, and do not omit the speed factor in a surface integral. The radius is ∣y∣|y| about the xx-axis and ∣x∣|x| about the yy-axis. Polar arc length and polar surfaces are explicitly outside this FP3 requirement.

FP3.5 - Vectors

Syllabus
2019
Topic
—
Level
A2

Use vector products for perpendiculars, areas and volumes

The vector product a×b\mathbf a\times\mathbf b is a vector perpendicular to both a\mathbf a and b\mathbf b. Its direction follows the right-hand orientation, while its magnitude records the area scale generated by the two vectors:∣a×b∣=∣a∣ ∣b∣sin⁡θ,|\mathbf a\times\mathbf b|=|\mathbf a|\,|\mathbf b|\sin\theta,where 0≤θ≤π0\le\theta\le\pi is the angle between them.

a×b=(a2b3−a3b2a3b1−a1b3a1b2−a2b1)\mathbf a\times\mathbf b=\begin{pmatrix}a_2b_3-a_3b_2\\a_3b_1-a_1b_3\\a_1b_2-a_2b_1\end{pmatrix}

Quantity Vector expression Geometric meaning
a×b\mathbf a\times\mathbf b component formula above Perpendicular vector; reversing order reverses its direction.
∣a×b∣|\mathbf a\times\mathbf b| magnitude of the cross product Area of the parallelogram on a,b\mathbf a,\mathbf b.
12∣a×b∣\tfrac12|\mathbf a\times\mathbf b| half the magnitude Area of the triangle on the same two sides.
a⋅(b×c)\mathbf a\cdot(\mathbf b\times\mathbf c) scalar triple product Signed volume scale of a parallelepiped.
∣a⋅(b×c)∣|\mathbf a\cdot(\mathbf b\times\mathbf c)| absolute triple product Volume of the parallelepiped; divide by 66 for the corresponding tetrahedron.

Order matters: b×a=−(a×b)\mathbf b\times\mathbf a=-(\mathbf a\times\mathbf b), whereas cyclic changes leave a scalar triple product unchanged. A zero cross product means the two non-zero vectors are parallel. A zero scalar triple product means the three vectors are coplanar, because the third vector has no component perpendicular to the plane of the first two.

Let a=(1,2,−1)\mathbf a=(1,2,-1) and b=(3,0,2)\mathbf b=(3,0,2). Thena×b=(4,−5,−6),∣a×b∣=77.\mathbf a\times\mathbf b=(4,-5,-6),\qquad |\mathbf a\times\mathbf b|=\sqrt{77}.The triangle with adjacent sides a\mathbf a and b\mathbf b has area 77/2\sqrt{77}/2. If c=(0,1,1)\mathbf c=(0,1,1), then(a×b)⋅c=−11,(\mathbf a\times\mathbf b)\cdot\mathbf c=-11,so the parallelepiped volume is 1111; the sign records orientation, not a negative physical volume.

A calculated cross product should satisfy (a×b)⋅a=0(\mathbf a\times\mathbf b)\cdot\mathbf a=0 and (a×b)⋅b=0(\mathbf a\times\mathbf b)\cdot\mathbf b=0. These two dot-product checks catch most component or sign errors before the result is used as a normal or area vector.

Do not treat the cross product as commutative, and do not use the signed scalar triple product directly as a volume. For a triangle use half the parallelogram area; for a tetrahedron use one sixth of the parallelepiped volume. Cross products here are three-dimensional.

Solve line, plane and shortest-distance problems

A vector equation separates position from direction. A line through the point with position vector a\mathbf a and non-zero direction b\mathbf b may be writtenr=a+λb\mathbf r=\mathbf a+\lambda\mathbf bor equivalently(r−a)×b=0.(\mathbf r-\mathbf a)\times\mathbf b=\mathbf0.The second form says exactly that the displacement from the fixed point is parallel to the line direction.

Problem Construction
Distance from point PP to plane through AA with normal n\mathbf n d=∣AP→⋅n∣∣n∣d=\dfrac{|\overrightarrow{AP}\cdot\mathbf n|}{|\mathbf n|}
Line of intersection of non-parallel planes Direction n1×n2\mathbf n_1\times\mathbf n_2; find one point satisfying both plane equations.
Shortest distance between skew lines r=a1+λb1\mathbf r=\mathbf a_1+\lambda\mathbf b_1 and r=a2+μb2\mathbf r=\mathbf a_2+\mu\mathbf b_2 d=∣(a2−a1)⋅(b1×b2)∣∣b1×b2∣d=\dfrac{|(\mathbf a_2-\mathbf a_1)\cdot(\mathbf b_1\times\mathbf b_2)|}{|\mathbf b_1\times\mathbf b_2|}
Distance between parallel lines with common direction b\mathbf b d=∣(a2−a1)×b∣∣b∣d=\dfrac{|(\mathbf a_2-\mathbf a_1)\times\mathbf b|}{|\mathbf b|}

Each distance formula is a projection. For a point and plane, the displacement is projected onto the unit normal. For skew lines, b1×b2\mathbf b_1\times\mathbf b_2 is perpendicular to both directions, so projecting any joining displacement onto this common normal gives the fixed perpendicular separation.

For the plane 2x−y+2z=62x-y+2z=6 and point P=(1,1,1)P=(1,1,1), the normal is n=(2,−1,2)\mathbf n=(2,-1,2). Substitution gives the signed residual 2−1+2−6=−32-1+2-6=-3, sod=∣−3∣22+(−1)2+22=1.d=\frac{|-3|}{\sqrt{2^2+(-1)^2+2^2}}=1.The absolute value is essential because distance is non-negative.

Forℓ1:r=λ(1,0,1),ℓ2:r=(0,1,0)+μ(0,1,1),\ell_1:\mathbf r=\lambda(1,0,1),\qquad \ell_2:\mathbf r=(0,1,0)+\mu(0,1,1),the common normal is (1,0,1)×(0,1,1)=(−1,−1,1)(1,0,1)\times(0,1,1)=(-1,-1,1). With joining vector (0,1,0)(0,1,0),d=∣(0,1,0)⋅(−1,−1,1)∣3=13.d=\frac{|(0,1,0)\cdot(-1,-1,1)|}{\sqrt3}=\frac1{\sqrt3}.Solving the coordinate equations confirms the lines do not intersect, so the skew formula applies.

For two plane equations, first cross their normals to obtain the intersection-line direction. Then choose one coordinate conveniently and solve the two simultaneous linear equations for a point. Substitute the final parametric line into both plane equations: both identities must hold for every parameter value.

The skew-line denominator is zero for parallel directions, so use the parallel-line formula instead. A zero scalar triple product gives zero separation but does not by itself distinguish intersecting from coincident/parallel cases; classify the directions and solve for intersection. Direction vectors and normals may be rescaled by any non-zero constant without changing the geometry.

Move between equations of a plane

A plane is fixed by one point and two independent in-plane directions, or by one point and a non-zero normal. These descriptions produce equivalent parametric, vector-normal and Cartesian equations; converting between them reveals the geometry needed for intersections and angles.

Form Equation Meaning
Parametric r=a+sb+tc\mathbf r=\mathbf a+s\mathbf b+t\mathbf c Point a\mathbf a plus two non-parallel directions in the plane.
Normal r⋅n=p\mathbf r\cdot\mathbf n=p n\mathbf n is perpendicular to the plane and p=a⋅np=\mathbf a\cdot\mathbf n.
Point-normal (r−a)⋅n=0(\mathbf r-\mathbf a)\cdot\mathbf n=0 Every in-plane displacement from AA is perpendicular to n\mathbf n.
Cartesian Ax+By+Cz=DAx+By+Cz=D Normal n=(A,B,C)\mathbf n=(A,B,C) and D=pD=p.

From a parametric form, calculate n=b×c\mathbf n=\mathbf b\times\mathbf c and then p=a⋅np=\mathbf a\cdot\mathbf n. From a Cartesian form, read off the normal and find any convenient point satisfying the equation; two independent vectors perpendicular to the normal may then serve as parametric directions.

A plane through A=(1,−1,2)A=(1,-1,2) with directions b=(1,2,0)\mathbf b=(1,2,0) and c=(0,1,1)\mathbf c=(0,1,1) hasn=b×c=(2,−1,1).\mathbf n=\mathbf b\times\mathbf c=(2,-1,1).Since a⋅n=2+1+2=5\mathbf a\cdot\mathbf n=2+1+2=5, its normal and Cartesian forms arer⋅(2,−1,1)=5,qquad2x−y+z=5.\mathbf r\cdot(2,-1,1)=5,qquad 2x-y+z=5.Substituting AA and both direction displacements verifies the conversion.

If three non-collinear points A,B,CA,B,C define a plane, use AB→\overrightarrow{AB} and AC→\overrightarrow{AC} as the two directions. Their cross product is a normal. If the cross product is zero, the points are collinear and do not determine a unique plane.

The acute angle θ\theta between two planes is the acute angle between their normals:cos⁡θ=∣n1⋅n2∣∣n1∣ ∣n2∣,0≤θ≤π2.\cos\theta=\frac{|\mathbf n_1\cdot\mathbf n_2|}{|\mathbf n_1|\,|\mathbf n_2|},\qquad 0\le\theta\le\frac\pi2.The absolute value selects the acute angle because reversing a normal does not change its plane.

In r⋅n=p\mathbf r\cdot\mathbf n=p, pp is a scalar, not necessarily the perpendicular distance from the origin; that distance is ∣p∣/∣n∣|p|/|\mathbf n|. The two parametric directions must be independent. Equivalent plane equations may differ by any non-zero scalar multiple, so compare all coefficients together rather than term by term.

FP3.6 - Further matrix algebra

Syllabus
2019
Topic
—
Level
A2

Represent linear transformations with matrices

A matrix represents a linear transformation by multiplying a column vector. If T:Rn→RmT:\mathbb R^n\to\mathbb R^m has matrix AA, thenT(x)=Ax.T(\mathbf x)=A\mathbf x.Linearity means T(u+v)=T(u)+T(v)T(\mathbf u+\mathbf v)=T(\mathbf u)+T(\mathbf v) and T(ku)=kT(u)T(k\mathbf u)=kT(\mathbf u), so the origin maps to the origin.

The columns of AA are the images of the standard basis vectors. In three dimensions,A=(∣∣∣T(e1)T(e2)T(e3)∣∣∣).A=\begin{pmatrix}|&|&|\\T(\mathbf e_1)&T(\mathbf e_2)&T(\mathbf e_3)\\|&|&|\end{pmatrix}.This gives the matrix immediately when the action on i,j,k\mathbf i,\mathbf j,\mathbf k is known, and explains why matrix multiplication forms the correct linear combination of those images.

Transformation Matrix size Multiplication
R2→R2\mathbb R^2\to\mathbb R^2 2×22\times2 two-component output from a two-component input
R3→R3\mathbb R^3\to\mathbb R^3 3×33\times3 three-component output from a three-component input
Rn→Rm\mathbb R^n\to\mathbb R^m m×nm\times n mm rows determine output components; nn columns match inputs

LetA=(1020−11210).A=\begin{pmatrix}1&0&2\\0&-1&1\\2&1&0\end{pmatrix}.Its columns show T(e1)=(1,0,2)TT(\mathbf e_1)=(1,0,2)^T, T(e2)=(0,−1,1)TT(\mathbf e_2)=(0,-1,1)^T and T(e3)=(2,1,0)TT(\mathbf e_3)=(2,1,0)^T. HenceT(1,2,−1)T=A(12−1)=(−1−34).T(1,2,-1)^T=A\begin{pmatrix}1\\2\\-1\end{pmatrix}=\begin{pmatrix}-1\\-3\\4\end{pmatrix}.The same result is the linear combination T(e1)+2T(e2)−T(e3)T(\mathbf e_1)+2T(\mathbf e_2)-T(\mathbf e_3).

If images of enough independent vectors are supplied instead of basis vectors, put the input vectors as columns of a matrix XX and their images as columns of YY. The unknown transformation matrix satisfies AX=YAX=Y; when XX is invertible, A=YX−1A=YX^{-1}. Verify every supplied mapping after solving.

A matrix represents a linear transformation only when the coordinate conventions and vector order are fixed. Do not place basis images in rows, and do not include a translation term in a purely linear matrix transformation. A map that sends the zero vector to a non-zero vector is affine, not linear.

Compose transformations in the correct order

Matrix products encode successive transformations, but the rightmost matrix acts first. If BB is followed by AA, thenx↦BBx↦AA(Bx)=(AB)x.\mathbf x\xmapsto{B}B\mathbf x\xmapsto{A}A(B\mathbf x)=(AB)\mathbf x.This is why the product ABAB represents BB followed by AA.

A product ABAB exists when the number of columns of AA equals the number of rows of BB. The result has the rows of AA and columns of BB. Each entry is a row-column dot product; dimension compatibility must be checked before interpreting a composition.

LetA=(100−1),B=(1201).A=\begin{pmatrix}1&0\\0&-1\end{pmatrix},\qquad B=\begin{pmatrix}1&2\\0&1\end{pmatrix}.ThenAB=(120−1)AB=\begin{pmatrix}1&2\\0&-1\end{pmatrix}represents the shear BB followed by reflection AA. For (1,1)T(1,1)^T, BB gives (3,1)T(3,1)^T and AA gives (3,−1)T(3,-1)^T, matching AB(1,1)TAB(1,1)^T.

Reversing the order givesBA=(1−20−1),BA=\begin{pmatrix}1&-2\\0&-1\end{pmatrix},which sends (1,1)T(1,1)^T to (−1,−1)T(-1,-1)^T. Thus AB≠BAAB\ne BA in general. A quick test vector can reveal an order error even before the full product is interpreted.

The identity matrix II leaves every vector unchanged, so AI=IA=AAI=IA=A. If two successive transformations undo one another, their product is II in the appropriate order; this becomes the basis of inverse transformations later in the Topic.

Read a written sequence from the action on the vector, not from left to right in the matrix product. Matrix multiplication is associative, so parentheses may move in ABCABC, but it is not generally commutative, so factors may not be reordered.

Transpose matrices and reverse product order

The transpose ATA^{\mathsf T} is formed by exchanging rows and columns: its (i,j)(i,j) entry is the (j,i)(j,i) entry of AA. Therefore an m×nm\times n matrix becomes an n×mn\times m matrix, and (AT)T=A(A^{\mathsf T})^{\mathsf T}=A.

Operation Transpose rule
Sum (A+B)T=AT+BT(A+B)^{\mathsf T}=A^{\mathsf T}+B^{\mathsf T}
Scalar multiple (kA)T=kAT(kA)^{\mathsf T}=kA^{\mathsf T}
Product (AB)T=BTAT(AB)^{\mathsf T}=B^{\mathsf T}A^{\mathsf T}
Inverse, when it exists (A−1)T=(AT)−1(A^{-1})^{\mathsf T}=(A^{\mathsf T})^{-1}
Symmetric matrix AT=AA^{\mathsf T}=A

The product order reverses because(AB)ijT=(AB)ji=∑kAjkBki=∑k(BT)ik(AT)kj.(AB)^{\mathsf T}_{ij}=(AB)_{ji}=\sum_k A_{jk}B_{ki}=\sum_k(B^{\mathsf T})_{ik}(A^{\mathsf T})_{kj}.So the row-column pairing becomes BTATB^{\mathsf T}A^{\mathsf T}, not ATBTA^{\mathsf T}B^{\mathsf T}.

ForA=(120−1),B=(3124),A=\begin{pmatrix}1&2\\0&-1\end{pmatrix},\qquad B=\begin{pmatrix}3&1\\2&4\end{pmatrix},we have AB=(79−2−4)AB=\begin{pmatrix}7&9\\-2&-4\end{pmatrix} and(AB)T=(7−29−4)=BTAT.(AB)^{\mathsf T}=\begin{pmatrix}7&-2\\9&-4\end{pmatrix}=B^{\mathsf T}A^{\mathsf T}.Direct multiplication confirms both the entries and reversed order.

Transposes convert column information into row information and are central to dot products and orthogonality. If a square matrix PP has orthonormal columns, then PTP=IP^{\mathsf T}P=I, so P−1=PTP^{-1}=P^{\mathsf T}; this is used when symmetric matrices are diagonalised.

Transposition does not reverse entries within each row; it swaps the row and column indices. Do not distribute it over a product without reversing factor order. A symmetric matrix must be square, and matching diagonal entries alone is not enough: every off-diagonal pair must also agree.

Evaluate 3 by 3 determinants and test singularity

The determinant of a square matrix is a scalar that measures signed scale under its transformation. For a 3×33\times3 matrix, expand along any row or column using signed 2×22\times2 minors. A matrix is singular exactly when its determinant is zero; otherwise it is non-singular and has an inverse.

det⁡ ⁣(abcdefghi)=a(ei−fh)−b(di−fg)+c(dh−eg)\det\!\begin{pmatrix}a&b&c\\d&e&f\\g&h&i\end{pmatrix}=a(ei-fh)-b(di-fg)+c(dh-eg)

Determinant condition Algebraic consequence Transformation consequence
det⁡A≠0\det A\ne0 Unique inverse A−1A^{-1} exists No dimension is collapsed; volume scale is ∣det⁡A∣|\det A|.
det⁡A=0\det A=0 AA is singular; no inverse Some non-zero direction is collapsed; transformed volume is zero.
det⁡A<0\det A<0 Still invertible if non-zero Orientation is reversed; physical volume uses ∣det⁡A∣|\det A|.

ForM=(210−132041),M=\begin{pmatrix}2&1&0\\-1&3&2\\0&4&1\end{pmatrix},expansion along the first row givesdet⁡M=2(3⋅1−2⋅4)−1((−1)⋅1−2⋅0)=−10+1=−9.\det M=2(3\cdot1-2\cdot4)-1((-1)\cdot1-2\cdot0)=-10+1=-9.Thus MM is non-singular and multiplies volumes by 99, while reversing orientation.

For a matrix containing a parameter, calculate and factor the determinant, then solve det⁡A=0\det A=0 to find exactly the singular values. Any later inverse formula must explicitly exclude those values. Substitute a candidate back into the determinant as a check.

Swapping two rows changes the determinant's sign; multiplying one row by kk multiplies the determinant by kk; adding a multiple of one row to another leaves it unchanged. These rules can simplify an evaluation, but every operation's effect must be tracked.

The cofactor signs alternate +,−,++,-,+ across the first row. Do not confuse a negative determinant with singularity: only zero is singular. When determinant magnitude is used as an area or volume scale, take the absolute value.

Find inverses of 3 by 3 matrices

A square matrix AA has an inverse only when det⁡A≠0\det A\ne0. The inverse satisfiesAA−1=A−1A=IAA^{-1}=A^{-1}A=Iand can be calculated from cofactors:A−1=1det⁡Aadj⁡A.A^{-1}=\frac1{\det A}\operatorname{adj}A.The adjugate is the transpose of the cofactor matrix.

Step Action
1. Determinant Calculate det⁡A\det A and state any excluded parameter values.
2. Minors Delete row ii and column jj to form each 2×22\times2 minor.
3. Cofactors Apply signs (+−+−+−+−+)\begin{pmatrix}+&-&+\\-&+&-\\+&-&+\end{pmatrix}.
4. Adjugate Transpose the cofactor matrix.
5. Divide/check Divide by det⁡A\det A and verify a product with AA gives II.

ForA=(110011001),det⁡A=1,A=\begin{pmatrix}1&1&0\\0&1&1\\0&0&1\end{pmatrix},\qquad \det A=1,the inverse isA−1=(1−1101−1001).A^{-1}=\begin{pmatrix}1&-1&1\\0&1&-1\\0&0&1\end{pmatrix}.Multiplying AA−1AA^{-1} gives II, including the cancellation 1−1=01-1=0 and 1−1=01-1=0 in the upper off-diagonal entries.

For invertible AA and BB,(AB)−1=B−1A−1.(AB)^{-1}=B^{-1}A^{-1}.Indeed, (AB)(B−1A−1)=AIA−1=I(AB)(B^{-1}A^{-1})=AIA^{-1}=I. The order reverses because the most recently applied transformation must be undone first.

The equation Ax=bA\mathbf x=\mathbf b has the unique solution x=A−1b\mathbf x=A^{-1}\mathbf b when AA is non-singular. In exact work, retain fractions and parameter restrictions until the final result, then verify by substitution.

Do not call the cofactor matrix the adjugate before transposing it, and do not divide by a determinant that may be zero. Taking reciprocals of individual entries does not form a matrix inverse. Both left and right identity products are valid checks for a square inverse.

Reverse transformations and their combinations

If a transformation sends x\mathbf x to y=Ax\mathbf y=A\mathbf x and AA is non-singular, its inverse sends the image back to the original vector:x=A−1y.\mathbf x=A^{-1}\mathbf y.No inverse transformation exists when AA is singular because distinct inputs have been collapsed to the same output.

If BB acts first and AA second, the combined matrix is ABAB. To reverse the combination, undo AA first and then BB:y=ABx⟹x=B−1A−1y.\mathbf y=AB\mathbf x\quad\Longrightarrow\quad \mathbf x=B^{-1}A^{-1}\mathbf y.Thus (AB)−1=B−1A−1(AB)^{-1}=B^{-1}A^{-1} is both an algebraic and procedural rule.

A linear transformation maps every point and direction vector of a line. To find the preimage of an image liney=p+λd,\mathbf y=\mathbf p+\lambda\mathbf d,apply A−1A^{-1} to both fixed vectors:x=A−1p+λA−1d.\mathbf x=A^{-1}\mathbf p+\lambda A^{-1}\mathbf d.The same parameter remains because matrix multiplication is linear.

LetA=diag⁡(2,−1,12)A=\operatorname{diag}\left(2,-1,\frac12\right)and suppose the image line isy=(4,1,3)T+λ(2,−2,1)T.\mathbf y=(4,1,3)^T+\lambda(2,-2,1)^T.Since A−1=diag⁡(1/2,−1,2)A^{-1}=\operatorname{diag}(1/2,-1,2), the original line isx=(2,−1,6)T+λ(1,2,2)T.\mathbf x=(2,-1,6)^T+\lambda(1,2,2)^T.Applying AA to its point and direction recovers the image line.

Check an inverse transformation in both directions on a general vector or on the defining point/direction data. For a combination, multiply the proposed inverse by the combined matrix in the correct order and require the identity matrix.

An inverse matrix reverses a transformation; it is not the transpose unless the matrix is orthogonal. Do not reverse a product without reversing factor order, and do not attempt an inverse transformation before checking that the determinant is non-zero.

Find and normalise eigenvectors

A non-zero vector v\mathbf v is an eigenvector of AA when the transformation changes only its scale (and possibly direction):Av=λv.A\mathbf v=\lambda\mathbf v.The scalar λ\lambda is the corresponding eigenvalue. The zero vector is never an eigenvector.

Stage Calculation
Find eigenvalues Solve det⁡(A−λI)=0\det(A-\lambda I)=0.
Find an eigenvector For each λ\lambda, solve (A−λI)v=0(A-\lambda I)\mathbf v=\mathbf0 for a non-zero vector.
Check Verify Av=λvA\mathbf v=\lambda\mathbf v.
Normalise if required Replace v\mathbf v by v/∣v∣\mathbf v/|\mathbf v|; its negative is equally valid.

ForA=(4123),A=\begin{pmatrix}4&1\\2&3\end{pmatrix},the characteristic equation is(4−λ)(3−λ)−2=λ2−7λ+10=0,(4-\lambda)(3-\lambda)-2=\lambda^2-7\lambda+10=0,so λ=5\lambda=5 or 22.

For λ=5\lambda=5, (A−5I)v=0(A-5I)\mathbf v=0 gives y=xy=x, so one eigenvector is (1,1)T(1,1)^T and a normalised choice is (1,1)T/2(1,1)^T/\sqrt2. For λ=2\lambda=2, the equation gives y=−2xy=-2x, so a normalised choice is (1,−2)T/5(1,-2)^T/\sqrt5. Direct multiplication verifies both pairs.

If a vector is supplied, multiply it by AA and compare corresponding non-zero components. It is an eigenvector only if one common scalar λ\lambda works in every component, including components that are zero. If an eigenvalue is supplied, substitute it into the nullspace equations rather than recomputing every root.

The same method applies to 3×33\times3 matrices: the characteristic determinant is cubic and each eigenvector comes from a homogeneous three-variable system. Row-reduce without forcing the free parameter to zero, then choose a convenient non-zero scale before normalising.

Solving only det⁡(A−λI)=0\det(A-\lambda I)=0 finds eigenvalues, not eigenvectors. Eigenvectors are non-zero and are not unique: every non-zero scalar multiple represents the same eigendirection. Normalising changes length to 11 but does not determine a unique sign.

Orthogonally diagonalise a symmetric matrix

A real symmetric matrix A=ATA=A^{\mathsf T} has an orthonormal basis of eigenvectors. Put those unit eigenvectors into the columns of an orthogonal matrix PP. ThenPTP=I,P−1=PT,D=PTAPP^{\mathsf T}P=I,\qquad P^{-1}=P^{\mathsf T},\qquad D=P^{\mathsf T}APis diagonal.

Step Required consistency
1. Eigenvalues Find all eigenvalues of AA.
2. Eigenvectors Find a basis for each eigenspace.
3. Orthonormalise Normalise mutually perpendicular eigenvectors; within a repeated eigenspace choose an orthonormal basis.
4. Assemble PP Place the unit eigenvectors as columns.
5. Assemble DD Put the matching eigenvalues on the diagonal in the same column order.

Writing the column equations together gives AP=PDAP=PD. Multiplying on the left by PT=P−1P^{\mathsf T}=P^{-1} yields PTAP=DP^{\mathsf T}AP=D. Orthogonality is what makes the change of coordinates preserve lengths and turns the inverse into a transpose.

ForA=(2112),A=\begin{pmatrix}2&1\\1&2\end{pmatrix},the eigenvalue 33 has unit eigenvector (1,1)T/2(1,1)^T/\sqrt2, and eigenvalue 11 has unit eigenvector (1,−1)T/2(1,-1)^T/\sqrt2. ThereforeP=12(111−1),D=(3001),P=\frac1{\sqrt2}\begin{pmatrix}1&1\\1&-1\end{pmatrix},\qquad D=\begin{pmatrix}3&0\\0&1\end{pmatrix},and direct multiplication gives PTAP=DP^{\mathsf T}AP=D.

Permuting the columns of PP is allowed only when the diagonal entries of DD are permuted in exactly the same way. Changing the sign of any eigenvector column leaves orthogonality and the resulting diagonal entry unchanged.

Diagonalisation by an orthogonal PP is guaranteed here because AA is real and symmetric; do not assume every matrix has an orthogonal eigenbasis. Columns of PP must be unit and mutually perpendicular, and their order must match the eigenvalues in DD.