Unit FP2: Further Pure Mathematics A2 2
- Syllabus
- 2019
- Section
- —
- Level
- A2
An algebraic inequality is solved by finding every point where its truth value can change, then determining which intervals satisfy the original relation. Denominator zeros and modulus boundaries must be recorded before simplifying.
| Form | Safe algebraic route |
|---|---|
| rational inequality | Move all terms to one side, combine them into N(x)/D(x), and mark zeros of both N and D. Test the sign on each resulting interval. |
| ∣F(x)∣<G(x) | Require G(x)>0, then solve −G(x)<F(x)<G(x). For ≤, require G(x)≥0. |
| ∣F(x)∣>G(x) | Where G(x)<0 the inequality is automatic; where G(x)≥0, solve F(x)>G(x) or F(x)<−G(x). Use the analogous inclusive conditions for ≥. |
| piecewise modulus | Alternatively split at every zero of the expression inside ∣ ∣, replace it by the correct signed expression on each interval, and intersect each result with that interval. |
For example, x−11>x+2x⟺(x−1)(x+2)−x2+2x+2>0. The numerator is zero at x=1±3; the denominator is zero at x=−2,1. A sign chart across these four ordered critical points gives −2<x<1−3or1<x<1+3. The denominator points are excluded even though they separate sign intervals.
For the official model inequality ∣x2−1∣>2(x+1), the right side is negative when x<−1, so that whole interval works automatically. For x≥−1, solve x2−1>2(x+1)orx2−1<−2(x+1). These become (x−3)(x+1)>0 or (x+1)2<0, giving x>3. Hence the full solution is x<−1orx>3.
Never multiply an inequality by an expression whose sign is unknown: the inequality direction might need to reverse. Keep exact critical values, test every interval, exclude every point where the original expression is undefined, and include a numerator or equality boundary only when the original inequality permits equality.
The method of differences rewrites each term as a difference of shifted expressions. When consecutive terms are displayed, the interior contributions cancel and only a small number of boundary terms remain.
| Step | Purpose |
|---|---|
| Decompose the summand | Use partial fractions, or a supplied identity, to write the term as shifted copies such as ur−ur+m. |
| Verify the identity | Recombine the parts before summing so that constants, signs and shifts are correct. |
| Display boundary terms | Write enough terms from the beginning and end to show exactly what cancels. |
| Collect survivors | Keep the first m positive terms and the final m negative terms, then simplify. |
r=p∑q(ur−ur+m)=j=0∑m−1up+j−j=1∑muq+j
For the official model, partial fractions give r(r+1)1=r1−r+11. Therefore r=1∑nr(r+1)1=(1−21)+(21−31)+⋯+(n1−n+11). Every interior fraction cancels, leaving 1−n+11=n+1n.
If a closed form S(n)=∑r=pnf(r) is already known, a later finite block is found by subtraction: r=a∑bf(r)=S(b)−S(a−1). This preserves the correct first included term r=a.
Do not claim cancellation without showing the shifted terms, and do not discard every middle-looking term when the shift is m>1: exactly m terms survive at each boundary. Check the starting index before using partial fractions whose denominators could be zero. This objective concerns finite series; an infinite limit requires separate convergence justification and is not asserted here.
Euler's relation represents a rotation through a real angle θ as a complex exponential: eiθ=cosθ+isinθ. Its real and imaginary parts are the coordinates of the corresponding point on the unit circle.
eiθ=cosθ+isinθ,e−iθ=cosθ−isinθ
The second relation is obtained by replacing θ with −θ and using that cosine is even while sine is odd. Adding the two equations eliminates the imaginary terms; subtracting them eliminates the cosine terms.
cosθ=2eiθ+e−iθ,sinθ=2ieiθ−e−iθ
For example, e3iθ+e−3iθ=2cos3θ, while e3iθ−e−3iθ=2isin3θ. These conversions let a trigonometric expression be handled with laws of indices and then converted back.
Keep the minus sign in e−iθ and the factor i in the sine denominator. The quotient is real because the numerator eiθ−e−iθ is purely imaginary. Euler's relation here concerns complex exponentials; it does not say that eiθ is a real exponential.
De Moivre's theorem says that multiplying a complex number in polar form n times multiplies its argument by n and raises its modulus to the power n. For every integer n,(cosθ+isinθ)n=cos(nθ)+isin(nθ).More generally, [r(cosθ+isinθ)]n=rn[cos(nθ)+isin(nθ)].
For positive integers, the result follows by induction. The case n=1 is immediate. If it holds for n=k, multiplication by cosθ+isinθ and the angle-addition formulae give cos((k+1)θ)+isin((k+1)θ). For n=0, both sides equal 1. For negative n, take the reciprocal of the positive-power result; the reciprocal of cosϕ+isinϕ is cosϕ−isinϕ. This proves the theorem for every integer n.
| Required use | Teaching move |
|---|---|
| Multiple-angle identity | Expand (cosθ+isinθ)n, then equate real parts for cosine or imaginary parts for sine. |
| Power reduction | Write powers using eiθ and e−iθ, expand, then pair conjugate exponentials as cosines. |
| Roots of a complex number | Include every argument ϕ+2kπ before dividing by the root number. |
For instance, equating imaginary parts when n=3 gives sin3θ=3sinθcos2θ−sin3θ=3sinθ−4sin3θ. In the reverse direction, Euler's forms give cos2θ=21+cos2θ. Thus the same theorem connects multiple angles with powers in both directions.
zm=R(cosϕ+isinϕ) ⟹ zk=R1/m(cosmϕ+2kπ+isinmϕ+2kπ),k=0,1,…,m−1
The m values have equal modulus R1/m and arguments separated by 2π/m, so they form a regular m-gon centred at the origin. Substitute one root into the original equation to check the modulus and multiplied argument.
De Moivre's theorem in this objective is proved for integer powers. When finding roots, do not use only one principal argument: the 2kπ term is what produces all distinct roots. When equating parts, retain only terms with the correct real or imaginary parity and use one consistent angle unit.
On an Argand diagram, ∣z−a∣ is the distance from the point z to the fixed point a, while arg(z−a) is the directed angle of the displacement from a to z. Translate each complex condition into distance or angle geometry before sketching.
| Complex condition | Geometric locus or region |
|---|---|
| ∣z−a∣=b, b>0 | Circle with centre a and radius b. |
| ∣z−a∣=k∣z−b∣, k>0 | Fixed ratio of distances: an Apollonius circle if k=1; the perpendicular bisector of ab if k=1. |
| arg(z−a)=β | Ray from a in direction β; the point a is excluded because its argument is undefined. |
| arg(z−bz−a)=β | Points from which the segment joining a and b subtends the fixed directed angle β; normally an arc through a and b, with both endpoints excluded. |
| ∣z−a∣≤∣z−b∣ | The half-plane at least as close to a as to b, including the perpendicular-bisector boundary. |
| ∣z−a∣≤b | The closed disc with centre a and radius b. |
For an exact equation, set z=x+iy and write each modulus as a squared distance. For example, ∣z∣=2∣z−3∣ becomes x2+y2=4[(x−3)2+y2], so (x−4)2+y2=4. The locus is therefore the circle with centre (4,0) and radius 2.
For an inequality, first draw its equality boundary, test a point not on that boundary to choose the correct side, and use a solid boundary for ≤ or ≥. For an argument condition, also respect the stated argument range so that the correct ray or arc is selected.
A modulus is a non-negative distance, not the complex number itself. Squaring a modulus equation is safe when both sides are non-negative, but expand coordinates before completing the square. An argument condition gives a directed angle and excludes every point that makes its numerator or denominator zero; do not replace a ray by a full straight line.
A transformation assigns each permitted point z in the source plane a point w in the image plane. To find the image of a locus, connect z=x+iy and w=u+iv through the transformation, substitute into the source condition, and simplify until the result is a condition on u and v.
| Transformation | Reliable route |
|---|---|
| w=z2 | Use u=x2−y2 and v=2xy, or use ∣w∣=∣z∣2 and argw=2argz. Remember that z and −z have the same image. |
| w=cz+daz+b | Rearrange to z=cw−ab−dw when the inverse is defined, then impose the original locus condition. |
| Cartesian source condition | Put w=u+iv, rationalise any denominator, equate real and imaginary parts, and complete the square or collect line terms. |
For example, let w=z+1z−1,z=−1. If z lies on the imaginary axis, then z=iy for real y, so ∣w∣=∣iy+1∣∣iy−1∣=1. The image lies on the unit circle. Solving z=(1+w)/(1−w) shows that w=1 has no finite preimage, so the image is the unit circle with that point excluded.
For a non-degenerate fractional linear transformation, ad−bc=0. If c=0, the source value z=−d/c is a pole and is excluded; the inverse also reveals any missing image value. Lines and circles commonly map to lines or circles, but the algebra and exclusions decide which one in a particular problem.
After obtaining the image equation, check it with one easy source point: transform that point directly and verify that its w-coordinates satisfy the new equation. This catches sign errors introduced while rationalising or completing the square.
Do not transform only the equation and forget the domain. A denominator-zero source point is not mapped, and an inverse denominator can identify a point absent from the image. Under w=z2, doubling an argument may require reduction to the required argument interval, and the mapping is two-to-one away from the origin.
A first-order equation is separable when it can be written as dxdy=g(x)h(y), so every factor involving y can be placed with dy and every factor involving x with dx. The constant of integration produces a family of solution curves; an initial condition selects one member.
| Step | Reason |
|---|---|
| Form the equation | Translate a rate statement into dy/dx and define every variable and constant. |
| Record equilibrium solutions | If h(y)=0, constant curves may solve the equation and would be lost by division. |
| Separate and integrate | Write h(y)1dy=g(x)dx, then include one arbitrary constant. |
| Apply the condition | Substitute the given (x,y) pair to obtain the particular solution. |
| Analyse before sketching | Find the domain, asymptotes and stationary points; use the sign of dy/dx for increasing or decreasing branches. |
For dxdy=x(1+y),y(0)=0, first record the equilibrium solution y=−1. For the other solutions,∫1+y1dy=∫xdx,so ln∣1+y∣=2x2+C⟹y=Aex2/2−1.The condition y(0)=0 gives A=1, hence y=ex2/2−1.
For the full family y=Aex2/2−1, every curve is symmetric about the y-axis and has dy/dx=0 at x=0. Curves with A>0 lie above the equilibrium and have a minimum at x=0; curves with A<0 lie below it and have a maximum there. This qualitative information should agree with any plotted member.
Do not divide by a function of y before checking where it is zero, because this can discard equilibrium solutions. Keep the integration constant until an initial or boundary condition is applied, and state the interval on which logarithms, denominators and the explicit solution are defined. A sketch must follow the solved curve and the differential equation's gradient signs, not a generic shape.
A first-order linear equation must first be written in the standard form dxdy+P(x)y=Q(x). Its integrating factor is μ(x)=e∫P(x)dx. Because μ′=Pμ, multiplying by μ turns the entire left side into the product derivative dxd(μy).
dxd(μy)=μQ⟹y=μ(x)∫μ(x)Q(x)dx+C
| Step | Check |
|---|---|
| Normalise | Divide by the coefficient of dy/dx; identify P and Q only afterwards. |
| Build μ | Integrate P with the correct sign; a non-zero constant factor in μ is immaterial. |
| Multiply every term | Verify that the left side equals (μy)′. |
| Integrate once | Integrate μQ, add C, then divide by μ. |
| Particularise and verify | Apply the condition, then substitute or differentiate to check the result. |
For dxdy−2y=x, we have P=−2 and μ=e−2x. Thus (e−2xy)′=xe−2x.Integration by parts gives e−2xy=−e−2x(2x+41)+C, so y=−2x−41+Ce2x. If y(0)=43, then C=1.
The term containing C is the homogeneous part of the family, while the remaining terms form one particular response to Q(x). Their sum is still a solution because the equation is linear.
The integrating-factor formula applies after the equation is in standard linear form; P and Q may be functions of x but not of y. Multiplying only some terms, using eP instead of e∫Pdx, or forgetting to divide the final expression by μ breaks the product-derivative identity. Preserve the stated x-domain when division or logarithms are involved.
A given substitution is useful when it converts a non-standard first-order equation into either a separable equation or a linear equation. The essential move is to differentiate the substitution with the chain rule, replace every occurrence of the old dependent variable consistently, and solve the resulting equation in the new variable.
| Given form | Differentiate as |
|---|---|
| v=y−g(x) | dxdv=dxdy−g′(x) |
| v=yn | dxdv=nyn−1dxdy |
| v=y−n | dxdv=−ny−n−1dxdy |
| y=F(v) | dxdy=F′(v)dxdv |
After differentiating, substitute into the original equation and simplify until only x, v and dv/dx remain. Identify the transformed equation as separable or linear, solve it by the corresponding earlier method, restore the integration constant, and finally replace v to express the result in the requested variable and form.
Consider dxdy+2y=xy3 with the given substitution v=y−2. Since dxdv=−2y−3dxdy, multiplying the original equation by −2y−3 gives dxdv−4v=−2x.This is linear. With integrating factor e−4x,ve−4x=∫−2xe−4xdx=e−4x(2x+81)+C,so v=2x+81+Ce4x,y2=2x+81+Ce4x1.
The substitution may impose restrictions. Here v=y−2 assumes y=0, so the original equation must be checked separately: y=0 is also a solution and was excluded during the transformation. Do not stop at the equation in v unless that is what was requested, and do not confuse this first-order reduction with the separate second-order workflow in FP2.5.
For a constant-coefficient equation adx2d2y+bdxdy+cy=f(x),a=0, the general solution is the sum of the complementary function (CF), which solves the homogeneous equation, and one particular integral (PI), which accounts for f(x): y=CF+PI.
| Roots of am2+bm+c=0 | Complementary function |
|---|---|
| Distinct real m1,m2 | Aem1x+Bem2x |
| Repeated real m | (A+Bx)emx |
| Complex α±iβ | eαx(Acosβx+Bsinβx) |
The auxiliary equation comes from trying y=emx in the homogeneous equation. Each independent root solution contributes an arbitrary constant, so a second-order equation has two constants before conditions are imposed.
| Form of f(x) | Trial form for the PI |
|---|---|
| kepx | λepx |
| A+Bx | λx+μ |
| p+qx+cx2 | λx2+μx+ν |
| mcosωx+nsinωx | λcosωx+μsinωx |
Differentiate the trial, substitute it into the full equation and compare coefficients to determine its unknowns. If any part of the trial is already in the CF, multiply the whole trial by x; use another factor of x if the overlap is repeated.
For the official resonance model y′′+4y=sin2x, the auxiliary roots are ±2i, so CF=Acos2x+Bsin2x. A trial Ccos2x+Dsin2x duplicates the CF and contributes zero. Use an x factor instead: yp=Kxcos2x. Since (xcos2x)′′+4xcos2x=−4sin2x, K=−41. Hence y=Acos2x+Bsin2x−41xcos2x.
Apply values of y and y′ only after CF and PI have been combined, producing two simultaneous equations for A and B. A final substitution into the differential equation checks both the PI coefficients and any resonance factor.
Do not use the auxiliary equation on the non-homogeneous right side, and do not call the CF alone the general solution when f(x)=0. A repeated root requires the factor x in the CF; overlap between the PI trial and the CF also requires an extra factor x. Keep the frequency ω, exponential rate p and all derivative signs exact.
A given substitution can turn a variable-coefficient second-order equation into the constant-coefficient type just solved. The decisive step is to transform both derivatives with the chain rule before simplifying; every derivative must be taken with respect to the variable displayed in its denominator.
| Given substitution | Required derivative relations |
|---|---|
| t=g(x) | dxdy=dtdyg′(x) and dx2d2y=dt2d2y[g′(x)]2+dtdyg′′(x) |
| x=h(t) | dxdy=dx/dtdy/dt and dx2d2y=(xt)3yttxt−ytxtt |
| y=q(x)v(x) | y′=q′v+qv′ and y′′=q′′v+2q′v′+qv′′ |
Differentiate the supplied relation, replace y′, y′′ and every explicit occurrence of the old variable, then cancel common non-zero factors using the stated domain. Check that the resulting equation is exactly the claimed constant-coefficient form. Solve it as CF + PI in the new variable, and finally back-substitute both the variable and any dependent-variable relation.
For x2y′′+3xy′−3y=2lnx,x>0, take the given substitution t=lnx. Then y′=x1yt,y′′=x21(ytt−yt), so the equation becomes ytt+2yt−3y=2t. Its auxiliary roots are 1 and −3. A PI at+b gives a=−32 and b=−94, hence y=Aet+Be−3t−32t−94. Returning to x gives y=Ax+Bx−3−32lnx−94,x>0.
The transformed equation and the final answer can be checked independently: substitute the derivative relations into the original equation for the first check, then replace the final y and its x-derivatives in the original equation for the second.
Do not replace x in the coefficients while leaving derivatives in the old variable. For t=lnx the condition x>0 is essential; for a square-root substitution, track the stated branch and domain. Constants A and B remain arbitrary through back-substitution, but the same letter must not be used ambiguously for both a coefficient and a new variable.
The nth derivative of y=f(x) is written f(n)(x) or dxndny. Higher derivatives are found by differentiating successively, but patterns, recurrences and a derivative table prevent repeated algebra from becoming unmanageable.
| Function | Useful nth derivative pattern |
|---|---|
| ekx | knekx |
| sin(kx) | knsin(kx+2nπ) |
| (ax+b)p | anp(p−1)⋯(p−n+1)(ax+b)p−n |
| ln(ax+b), n≥1 | (ax+b)n(−1)n−1(n−1)!an |
For y=ln(2+x),y′=2+x1,y′′=−(2+x)21,y′′′=(2+x)32.The powers, alternating signs and factorial factors give y(n)=(2+x)n(−1)n−1(n−1)!,n≥1. Substituting n=1,2,3 checks the general expression.
When a function satisfies a differential relation, differentiating that relation can be shorter than starting again from the original function. Keep every product-rule term: differentiating x,y′′ gives y′′+x,y′′′. Values of lower derivatives at a point can then determine a required higher derivative there.
The order belongs to the whole derivative: d3y/dx3 is not (dy/dx)3. Reapply product and chain rules at every stage, simplify before looking for a pattern, and verify a claimed nth-derivative formula against the first two or three cases. State any restriction inherited from logarithms or denominators.
A Maclaurin series is a Taylor series centred at 0. Its coefficients are chosen so that the polynomial and the function have the same successive derivatives at x=0:f(x)=f(0)+f′(0)x+2!f′′(0)x2+⋯+n!f(n)(0)xn+⋯.
If f(x)=a0+a1x+a2x2+⋯, then setting x=0 gives a0=f(0). Differentiate once and set x=0 to get a1=f′(0); differentiating r times gives f(r)(0)=r!ar. Hence ar=f(r)(0)/r!.
| Function | Maclaurin expansion |
|---|---|
| ex | 1+x+2!x2+3!x3+⋯ |
| sinx | x−3!x3+5!x5−⋯ |
| cosx | 1−2!x2+4!x4−⋯ |
| ln(1+x) | x−2x2+3x3−4x4+⋯, for ∣x∣<1 |
The logarithmic expansion follows because for r≥1, dxrdrln(1+x)x=0=(−1)r−1(r−1)!. Standard series may then be adapted and combined. For example,ln1−x1+x=ln(1+x)−ln(1−x)=2x+32x3+O(x5). Even powers cancel, so only the needed terms should be retained.
Divide each derivative value by the matching factorial, write terms in ascending powers, and distinguish the number of non-zero terms from the highest power requested. A truncated series is a local approximation, not an identity for every x; preserve the relevant domain, especially ∣x∣<1 for the displayed logarithmic series.
A Taylor series expands f(x) about a chosen centre x=a in powers of the displacement h=x−a:f(x)=f(a)+f′(a)h+2!f′′(a)h2+3!f′′′(a)h3+⋯.The coefficients therefore describe the function's value and successive local changes at a, not at 0.
| Step | Action |
|---|---|
| Set the centre | Write h=x−a and keep all final powers in h. |
| Build a derivative table | Evaluate f(a),f′(a),…,f(n)(a) through the requested power. |
| Insert factorials | Use f(r)(a)hr/r! for each term. |
| Simplify and truncate | Give ascending powers through the stated order and use an ellipsis or remainder notation. |
For the official example f(x)=sinx about a=π, let h=x−π. The derivative values aref(π)=0,f′(π)=−1,f′′(π)=0,f′′′(π)=1.Therefore, up to and including h3,sinx=−(x−π)+6(x−π)3+O((x−π)4). Directly using sin(π+h)=−sinh confirms the signs.
Do not insert derivatives evaluated at 0 unless the centre is 0. The coefficient of (x−a)r is f(r)(a)/r!, not merely the derivative value. If a question asks through (x−a)3, include zero coefficients only when they clarify the structure, and do not replace the requested shifted powers by expanded powers of x.
The Taylor-series method solves a differential equation locally by using the equation and its derivatives to generate y(a),y′(a),y′′(a),… at the expansion centre. A term through (x−a)n requires derivative values through y(n)(a).
| Step | Purpose |
|---|---|
| Use the given conditions | Record y(a) and the supplied lower derivatives. |
| Evaluate the equation at a | Solve for the next derivative value. |
| Differentiate the equation | Generate each further derivative, keeping all product-rule terms. |
| Evaluate again at a | Substitute values already found before moving to the next order. |
| Assemble the Taylor polynomial | Use y(r)(a)(x−a)r/r! and stop at the requested power. |
For the official modely′′+xy′+y=0,y(0)=1,y′(0)=0,the original equation at 0 gives y′′(0)=−1. Differentiating once givesy′′′+2y′+xy′′=0,so y′′′(0)=0. Differentiating again givesy′′′′+3y′′+xy′′′=0,so y′′′′(0)=3. Hence, through x4,y=1-rac{x^2}{2!}+\frac{3x^4}{4!}+O(x^5)=1-\frac{x^2}{2}+\frac{x^4}{8}+O(x^5).
Equivalently, substitute y=a0+a1x+a2x2+⋯ and its differentiated series into the equation, then equate coefficients. The derivative-at-the-centre method is usually shorter when initial values are supplied explicitly.
Each differentiation changes product terms: for example, (xy′)′=y′+xy′′. Do not stop after finding derivatives; factorial denominators are still required when forming the series. The truncated polynomial is a local series solution to the requested order, not a claim that the omitted remainder is zero.
A polar point (r,θ) lies a distance r≥0 from the pole in the direction measured by θ from the initial line. Cartesian and polar descriptions are connected byx=rcosθ,y=rsinθ,r2=x2+y2.At the pole r=0, the angle is not unique.
| Polar equation | Structure to recognise |
|---|---|
| θ=α | Ray from the pole at angle α when r≥0. |
| r=psec(α−θ) | Straight line xcosα+ysinα=p. |
| r=a | Circle centred at the pole, radius a. |
| r=2acosθ | Circle centre (a,0), radius a. |
| r=kθ | Spiral whose radius changes linearly with angle. |
| r=a(1±cosθ) | Cardioid; the sign determines its orientation. |
| r=a(3+2cosθ) | Limacon with a≤r≤5a when a>0. |
| r=acos2θ | Rose-type curve; locate permitted intervals, zeros and extrema. |
| r2=a2cos2θ | Lemniscate; real points require cos2θ≥0. |
To sketch reliably, first state the permitted θ interval. Test symmetry by replacing θ with −θ or π−θ, solve r=0 for passages through the pole, find maximum and minimum r, and calculate a small table at exact angles. Plot in increasing θ so the order of loops or arcs is clear.
Cartesian conversion can confirm the shape. For example,r=2acosθ⟹r2=2arcosθ,so x2+y2=2ax⟹(x−a)2+y2=a2.This proves that the polar curve is the circle described in the table.
Curves drawn over the same ray intersect where their admissible radii are equal. Solve r1(θ)=r2(θ), retain angles in the stated range, and substitute back for the exact radius. The pole may be a shared point even when it arises from different angle values.
Under the stated convention r≥0, discard angle intervals that make an unsquared radius negative unless the question explicitly defines a signed-radius plotting convention. Do not treat tanθ=y/x alone as a quadrant check, and do not assume one period traces every curve exactly once; use symmetry, zeros and the supplied interval.
A narrow polar sector of angle dθ has area approximately 21r2dθ. Therefore the area swept once as θ runs from α to β isA=21∫αβr2dθ.The limits must describe the actual boundary rays or curve intersections of the required region.
| Step | Check |
|---|---|
| Find boundary angles | Solve intersections or use the stated rays; keep only admissible values. |
| Identify the swept region | Check whether one integral gives it directly or whether a second polar area or a triangle must be subtracted. |
| Square before integrating | Expand r2 and use exact trigonometric identities. |
| Evaluate in radians | Retain exact values of π and radicals until the end. |
For the upper half of the cardioid r=a(1+cosθ), 0≤θ≤π,A=2a2∫0π(1+2cosθ+cos2θ)dθ.Using cos2θ=21(1+cos2θ) givesA=2a2(π+2π)=43πa2.
dθdx=r′cosθ−rsinθ,dθdy=r′sinθ+rcosθ,dxdy=dx/dθdy/dθ
| Required tangent | Condition |
|---|---|
| Parallel to the initial line | dy/dθ=0 and dx/dθ=0. |
| At right angles to the initial line | dx/dθ=0 and dy/dθ=0. |
For r=2acosθ, at θ=π/4 we have r=2a. Alsodθdy=2acos2θ=0,dθdx=−2asin2θ=−2a=0.Thus the tangent is parallel to the initial line at (r,θ)=(2a,π/4), the top point (a,a) of the circle.
The area formula counts a region once only when the chosen interval traces its boundary once. If dx/dθ and dy/dθ are both zero, the simple horizontal/vertical test is inconclusive and the local curve needs separate analysis. Never divide by dx/dθ before checking whether it is zero, and use radians in integration.