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Calculus 2 Review

MAC 2312 Final Exam Study Guide


1. Velocity / Net Change Applications

Core idea: the definite integral of a rate of change gives the net change in the original quantity.

$$\int_a^b f'(t),dt = f(b)-f(a)$$

Position, Velocity, Acceleration

  • v(t) = s′(t) (velocity is derivative of position)
  • a(t) = v′(t) (acceleration is derivative of velocity)
  • $s(b)-s(a)=\displaystyle\int_a^b v(t),dt$ → this is displacement (net change in position), signed.
  • Total distance traveled (not the same as displacement when velocity changes sign): $$\text{distance}=\int_a^b |v(t)|,dt$$
    • Find where v(t) = 0 to break the interval into pieces where v doesn't change sign, integrate |v| on each piece (flip sign of the integral where v<0), and add the absolute values.
  • $v(b)-v(a)=\displaystyle\int_a^b a(t),dt$ → net change in velocity.

General Net Change Applications

If R(t) is a rate (of water flow, population growth, cost, income, etc.): $$\text{Total (net) change over }[a,b] = \int_a^b R(t),dt$$

  • If R(t) can be inflow minus outflow, or two competing rates, integrate the difference of the rates to get net change.
  • To find the amount at time b, given amount at time a: $$\text{amount}(b) = \text{amount}(a) + \int_a^b R(t),dt$$
  • Read carefully whether the problem wants net change (signed, can cancel out) or total accumulation (use |R(t)|, similar to total distance).

Common exam setup: given v(t) on [a,b], compute (i) displacement, (ii) total distance traveled — know both formulas and when each applies.


2. Volume of Solids of Revolution

Always graph the region first (and the axis of revolution) — this alone is worth points.

Disk Method

Used when the region touches the axis of revolution directly (no gap). $$V=\pi\int_a^b [R(x)]^2,dx \quad\text{(revolve about a horizontal axis)}$$ $$V=\pi\int_c^d [R(y)]^2,dy \quad\text{(revolve about a vertical axis)}$$ where R(x) (or R(y)) is the distance from the curve to the axis of revolution.

Washer Method

Used when there's a gap between the region and the axis (revolving the area between two curves). $$V=\pi\int_a^b \left([R(x)]^2-[r(x)]^2\right)dx$$

  • R(x) = outer radius (farther curve from axis), r(x) = inner radius (closer curve to axis). Outer minus inner, squared first, same order as polar area.
  • If the axis of revolution is not the x- or y-axis (e.g., y = k or x = h), adjust the radius: R(x) = f(x) − k, etc. — always distance from curve to axis, not the curve's value itself.

Shell Method

Used when it's easier to integrate along the axis parallel to the axis of revolution (avoids solving for x in terms of y, or vice versa). $$V=2\pi\int_a^b x\cdot h(x),dx \quad\text{(revolve about the y-axis, or a vertical line)}$$ $$V=2\pi\int_c^d y\cdot h(y),dy \quad\text{(revolve about the x-axis, or a horizontal line)}$$ where:

  • the factor (x or y) = radius = distance from the representative strip to the axis of revolution (adjust with ± shift if axis isn't x=0 or y=0),
  • h(x) (or h(y)) = height of the shell = length of the strip = (top curve − bottom curve), or (right curve − left curve).

Choosing disk/washer vs. shell

  1. Identify the axis of revolution and whether the region is more naturally described as a function of x or of y.
  2. If slicing perpendicular to the axis gives simple radius/radii → disk or washer.
  3. If slicing perpendicular to the axis requires solving for the "wrong" variable, or the region isn't symmetric about the axis → shell method (slice parallel to the axis instead).
  4. Either method can work for most regions — pick whichever avoids solving the curve equation for the other variable.

Steps for full credit:

  1. Sketch the region and the axis of revolution (2+ points).
  2. Identify method (disk/washer/shell) and set up radius/height expressions carefully, including any shifts for a non-standard axis.
  3. Determine correct limits of integration (intersection points of the curves).
  4. Set up and evaluate the integral.

3 & 4. Integration Strategies

Decision order when you see an integral:

  1. Can you simplify algebraically first (expand, split fraction, simplify)?
  2. Is it a basic/known antiderivative?
  3. u-substitution — look for a function and its derivative (up to a constant).
  4. Integration by parts — products of unlike function types (poly × exp, poly × trig, ln, arctan, etc.)
  5. Trig integral techniques — powers of sin/cos, sec/tan, etc.
  6. Trig substitution — expressions like √(a²−x²), √(a²+x²), √(x²−a²).
  7. Partial fractions — rational function P(x)/Q(x), especially after long division if deg P ≥ deg Q.
  8. Improper integral — infinite limits or discontinuity in the interval → rewrite as a limit.

u-Substitution

Let u = inner function, du = derivative dx. Rewrite entirely in u, integrate, substitute back.

Integration by Parts

$$\int u,dv = uv - \int v,du$$ Choose u using LIATE (Logarithmic, Inverse trig, Algebraic, Trig, Exponential — pick u in that priority order, since it should get simpler when differentiated).

  • Repeated by-parts (tabular method) for x²eˣ, x²sinx, etc.
  • Circular case (eˣsinx, eˣcosx): apply by parts twice, solve algebraically for the integral.

Trig Integrals

∫sinᵐx cosⁿx dx

  • If m (power of sin) is odd: save one sinx, convert rest to cos via sin²x = 1−cos²x, let u = cosx.
  • If n (power of cos) is odd: save one cosx, convert rest to sin via cos²x = 1−sin²x, let u = sinx.
  • If both even: use power-reduction identities $$\sin^2x=\frac{1-\cos2x}{2},\qquad \cos^2x=\frac{1+\cos2x}{2}$$

∫tanᵐx secⁿx dx

  • If n (power of sec) is even: save sec²x, convert rest with sec²x = 1+tan²x, let u = tanx.
  • If m (power of tan) is odd: save secx·tanx, convert rest with tan²x = sec²x−1, let u = secx.
  • Know: ∫tanx dx = ln|secx| + C, ∫secx dx = ln|secx+tanx| + C.

Trig Substitution

Expression Substitution Identity used
√(a²−x²) x = a sinθ 1−sin²θ=cos²θ
√(a²+x²) x = a tanθ 1+tan²θ=sec²θ
√(x²−a²) x = a secθ sec²θ−1=tan²θ

After integrating, draw a right triangle from the substitution to convert θ back to x.

Partial Fractions

  1. Make sure deg(numerator) < deg(denominator); if not, do polynomial long division first.
  2. Factor the denominator completely.
  3. Set up terms:
    • Linear factor (ax+b): term A/(ax+b)
    • Repeated linear (ax+b)ⁿ: terms A₁/(ax+b) + A₂/(ax+b)² + … + Aₙ/(ax+b)ⁿ
    • Irreducible quadratic (ax²+bx+c): term (Ax+B)/(ax²+bx+c)
  4. Clear denominators, solve for constants (plug in convenient x-values or match coefficients).
  5. Integrate each simple piece (logs, arctans).

Improper Integrals

  • Infinite limit: $\int_a^\infty f,dx = \lim_{t\to\infty}\int_a^t f,dx$. Converges if the limit is finite.
  • Discontinuity at c in [a,b]: split and take one-sided limits: $\lim_{t\to c^-}\int_a^t f,dx$, etc.
  • Both pieces must converge for the whole integral to converge.
  • p-integral test: $\int_1^\infty \frac{1}{x^p}dx$ converges iff p > 1.

5. Sequences: Convergence / Divergence

A sequence {aₙ} converges to L if $\lim_{n\to\infty}a_n = L$ exists (finite); otherwise it diverges.

Techniques:

  • Treat n as continuous x, use standard limit laws / L'Hôpital's rule (valid since if the continuous limit exists, the sequence limit equals it).
  • Squeeze Theorem: if bₙ ≤ aₙ ≤ cₙ and bₙ, cₙ → L, then aₙ → L. Useful for sequences with sin, cos, or (−1)ⁿ factors.
  • Key limit: $\lim_{n\to\infty} r^n = 0$ if |r| < 1; diverges if |r| > 1 (or r = −1, oscillates); = 1 if r = 1.
  • $\lim_{n\to\infty}\left(1+\frac{k}{n}\right)^n = e^k$
  • Factorial/exponential growth: $\lim \frac{n!}{n^n}=0$, and n! grows faster than any exponential aⁿ.
  • Absolute Value Theorem: if $\lim |a_n| = 0$ then $\lim a_n = 0$ (handles alternating sequences).
  • Monotonic Sequence Theorem: a bounded, monotonic (always increasing or always decreasing) sequence converges. Useful for recursively defined sequences: show monotonic + bounded ⇒ converges, then take limit of both sides of the recursion to solve for L.

Common divergence indicators: dominant term grows without bound, oscillation without approaching a single value (e.g., (−1)ⁿ, sin(n) without decay), or the sequence is unbounded.


6. Taylor / Maclaurin Series

Taylor series of f(x) centered at a: $$f(x) = \sum_{n=0}^{\infty} \frac{f^{(n)}(a)}{n!}(x-a)^n$$

Maclaurin series = Taylor series centered at a = 0: $$f(x) = \sum_{n=0}^{\infty}\frac{f^{(n)}(0)}{n!}x^n$$

Process:

  1. Compute f(a), f′(a), f″(a), f‴(a), … and find the pattern.
  2. Write general term $\dfrac{f^{(n)}(a)}{n!}(x-a)^n$ in summation notation.
  3. Find radius of convergence R using the Ratio Test: $L=\lim_{n\to\infty}\left|\frac{a_{n+1}}{a_n}\right|$; series converges absolutely when L < 1.
  4. Check the endpoints x = a±R separately (plug in, test with an appropriate series test) to determine the exact interval of convergence (open, half-open, or closed).

Memorize these Maclaurin series (centered at 0), all valid for all x unless noted:

$$e^x = \sum_{n=0}^\infty \frac{x^n}{n!}=1+x+\frac{x^2}{2!}+\cdots$$ $$\sin x = \sum_{n=0}^\infty \frac{(-1)^n x^{2n+1}}{(2n+1)!}=x-\frac{x^3}{3!}+\frac{x^5}{5!}-\cdots$$ $$\cos x = \sum_{n=0}^\infty \frac{(-1)^n x^{2n}}{(2n)!}=1-\frac{x^2}{2!}+\frac{x^4}{4!}-\cdots$$ $$\frac{1}{1-x}=\sum_{n=0}^\infty x^n,\quad |x|<1$$ $$\ln(1+x)=\sum_{n=1}^\infty \frac{(-1)^{n-1}x^n}{n},\quad -1<x\le1$$ $$\arctan x = \sum_{n=0}^\infty \frac{(-1)^n x^{2n+1}}{2n+1},\quad -1\le x\le1$$ $$(1+x)^k=\sum_{n=0}^\infty \binom{k}{n}x^n\ \text{(binomial series)},\quad |x|<1$$

Shortcut: for many problems it is far faster to take a known series and substitute, differentiate, integrate, or multiply by xⁿ rather than compute derivatives directly — check whether the function is a disguised version of one above.


7. Power Series Representations of Functions

Build from the geometric series: $$\frac{1}{1-x}=\sum_{n=0}^\infty x^n,\qquad |x|&lt;1$$

Common manipulations:

  • Substitution: replace x with an expression. E.g. $\frac{1}{1+x^2}=\frac{1}{1-(-x^2)}=\sum_{n=0}^\infty(-1)^n x^{2n}$.
  • Multiplying by a power of x: $\frac{x}{1-x}= \sum_{n=0}^\infty x^{n+1}$.
  • Differentiating term-by-term: if $f(x)=\sum a_n x^n$, then $f'(x)=\sum n,a_n x^{n-1}$ (same radius of convergence, endpoints re-checked).
  • Integrating term-by-term: $\int f(x),dx = \sum \frac{a_n}{n+1}x^{n+1}+C$.
  • Partial fractions first, then apply geometric series to each piece, if the denominator factors.

Finding interval of convergence: apply the Ratio Test to the general term, solve |x−a| < R for R, then test both endpoints individually in the original series (don't assume from the open interval).


8. Parametric Equations → Cartesian

Eliminating the parameter t:

  • Solve one equation for t, substitute into the other, or
  • Use an identity: if x = a cos t, y = b sin t → (x/a)² + (y/b)² = 1 (ellipse), using cos²t + sin²t = 1.
  • Watch the domain/range restrictions on t — they restrict the resulting curve (e.g., only part of the ellipse, direction of tracing).

Slope of tangent line (no need to eliminate t): $$\frac{dy}{dx}=\frac{dy/dt}{dx/dt}$$

Second derivative: $$\frac{d^2y}{dx^2}=\frac{d}{dx}\left(\frac{dy}{dx}\right)=\frac{\dfrac{d}{dt}\left(\dfrac{dy}{dx}\right)}{dx/dt}$$

Identifying the curve: after eliminating t, recognize standard forms:

  • Line, parabola, circle, ellipse, hyperbola (see conic forms in section 9 below).
  • Note orientation/direction of tracing from increasing t, and any restricted domain (arrows on the graph).

Graphing: plot a table of (x,y) points for increasing t values, connect in order, and mark the direction of motion with an arrow.


9. Polar ⟷ Cartesian Conversions

Conversion formulas: $$x=r\cos\theta,\qquad y=r\sin\theta$$ $$r^2=x^2+y^2,\qquad \tan\theta=\frac{y}{x}$$

Polar → Cartesian: substitute the above directly into the polar equation, then complete the square if needed to identify the curve.

Cartesian → Polar: substitute x = r cosθ, y = r sinθ into the Cartesian equation and simplify for r (or r²).

Common polar curves to recognize:

Polar equation Cartesian form Curve
r = a x² + y² = a² circle, center origin
r = a cosθ (x − a/2)² + y² = (a/2)² circle through origin, on x-axis
r = a sinθ x² + (y − a/2)² = (a/2)² circle through origin, on y-axis
θ = c y = (tan c)x line through origin
r = a + b cosθ (or sinθ), a=b cardioid heart shape, cusp at origin
r = a + b cosθ, a<b limaçon with inner loop
r = a + b cosθ, a>b dimpled/convex limaçon
r² = a² cos2θ lemniscate figure-eight
r = a cos(nθ) or a sin(nθ) rose curve n petals if n odd, 2n petals if n even

10. Graphing Polar Curves & Area of Polar Regions

Graphing: Make a table of θ vs r over one full period (usually 0 to 2π, or 0 to π for some roses), plot points, and connect smoothly. Pay attention to:

  • Symmetry (about polar axis if r(−θ)=r(θ); about the pole if r(θ+π)=r(θ); about θ=π/2 if r(π−θ)=r(θ)).
  • Where r = 0 (curve passes through the pole) and where r is maximum.

Area of a polar region: $$A=\int_\alpha^\beta \frac{1}{2}\left[r(\theta)\right]^2 d\theta$$

Steps:

  1. Identify the correct bounds α, β where the curve traces the desired region exactly once (find intersection angles by setting r-values equal, or find where r = 0).
  2. Area between two curves: $A = \int_\alpha^\beta \frac{1}{2}\left([r_{outer}]^2-[r_{inner}]^2\right)d\theta$ — always outer minus inner, squared first.
  3. Area of a single inner loop of a limaçon: find the θ-values where r = 0 bounding that loop, integrate only over that range.
  4. Watch for symmetry to simplify: often easier to integrate over half the region and double it.
  5. Simplify the integrand with power-reduction identities ($\cos^2\theta=\frac{1+\cos2\theta}{2}$, etc.) before integrating.

11. Conics in Standard (Cartesian) Form

General strategy: complete the square in x and y to get the standard form, then read off center, a, b (or c), and classify.

Parabola

$$(y-k)^2 = 4p(x-h) \quad\text{or}\quad (x-h)^2=4p(y-k)$$

  • Vertex (h,k). Opens toward the sign of p.
  • Focus is p units from vertex along axis of symmetry; directrix is p units on the opposite side.

Ellipse

$$\frac{(x-h)^2}{a^2}+\frac{(y-k)^2}{b^2}=1$$

  • Center (h,k). a > b: major axis horizontal (if a² is under the x-term); a < b: major axis vertical.
  • $c^2 = a^2 - b^2$ (a is always the larger denominator's square root).
  • Vertices: (h±a, k) or (h, k±a) along major axis. Foci: (h±c, k) or (h, k±c).

Hyperbola

$$\frac{(x-h)^2}{a^2}-\frac{(y-k)^2}{b^2}=1\quad\text{(opens left/right)}$$ $$\frac{(y-k)^2}{a^2}-\frac{(x-h)^2}{b^2}=1\quad\text{(opens up/down)}$$

  • Center (h,k). $c^2 = a^2+b^2$.
  • Vertices: a units from center along the transverse axis. Foci: c units from center, same axis.
  • Asymptotes: through the center with slopes ±b/a (horizontal transverse axis) or ±a/b (vertical transverse axis): $$y-k=\pm\frac{b}{a}(x-h)\quad\text{or}\quad y-k=\pm\frac{a}{b}(x-h)$$

Graphing tip: plot center first, then vertices, then sketch the guiding box (using a, b) for ellipses/hyperbolas, draw asymptotes as dashed lines for hyperbolas before sketching the curve.


12. Conics in Polar Form

Standard polar conic equations (focus at the pole): $$r=\frac{ed}{1\pm e\cos\theta}\qquad r=\frac{ed}{1\pm e\sin\theta}$$

  • e = eccentricity, d = distance from focus (pole) to the directrix.
  • Denominator with cosθ → directrix is vertical (x = ±d); denominator with sinθ → directrix is horizontal (y = ±d).
  • + sign → directrix to the right/above the pole; − sign → directrix to the left/below the pole.

Classify by eccentricity:

e value Conic
e = 1 Parabola
0 < e < 1 Ellipse
e > 1 Hyperbola

Finding key features:

  1. Get the equation into the exact form above (divide numerator and denominator so the constant term in the denominator is 1).
  2. Read off e directly (coefficient of cosθ or sinθ) and solve for d.
  3. Vertices: plug in the θ-values that point along the axis of symmetry (θ = 0, π for cosθ-form; θ = π/2, 3π/2 for sinθ-form) to get r, then convert (r,θ) to Cartesian points.
  4. Focus: always at the pole (origin) for this standard form.
  5. Directrix: the line x = d or y = d (with appropriate sign) as determined above.
  6. Asymptotes (hyperbola only, e>1): find where r → ∞, i.e., where the denominator = 0; those θ-values give the asymptote directions from the pole (lines through the origin at those angles), or convert the Cartesian form (after multiplying out) to extract slopes.
  7. Graphing: plot the vertex/vertices found in step 3, note the pole is a focus, and sketch consistent with the eccentricity (nearly circular for small e, elongated for e close to 1, two open branches for e>1).

Quick Reference: General Problem-Solving Checklist

  • Velocity/net change: decide if the problem wants signed net change (just integrate) or total accumulation/distance (integrate |rate|, splitting at sign changes).
  • Volumes: graph the region AND the axis of revolution first (guaranteed points); choose disk/washer vs. shell based on which needs fewer variable-swaps; always outer² − inner² for washers.
  • Integrals: identify structure first → pick the right technique → simplify before integrating when possible → don't forget +C for indefinite integrals.
  • Sequences: find the limit as n→∞; use L'Hôpital, squeeze theorem, or monotonic/bounded argument as needed.
  • Series: know your 6 memorized Maclaurin series cold; always find R with Ratio Test, then check both endpoints separately.
  • Parametric/Polar/Conics: always convert carefully, complete the square when needed, and double check by identifying key features (vertices, foci, center, asymptotes, directrix) before graphing.
  • Polar area: always graph first (4 pts), correctly identify bounds α, β (8 pts) — this is the #1 place points are lost.
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