Skills

Math you need: the one-page sheet

Functions and Their Graphs

A function sends each input to one output. Read it from a formula (substitute with parentheses), a graph (heights, filled and open dots) or a table. Know the domain, write lines in point-slope form, compose functions inside first, move graphs with f(x − h) + k , and find vertical asymptotes where a denominator is 0.

  • A function gives one output for each input. Substitute with parentheses: if f(x)=x2−3xf(x) = x^2 - 3x, then f(a+1)f(a + 1)=(a+1)2−3(a+1)= (a + 1)^2 - 3(a + 1).
  • The domain is every input the rule accepts; the range is every output it produces. Rule out zero denominators and square roots of negatives.
  • On a graph, a filled dot is on the graph and an open circle is not. f(a)f(a) is the height of the graph at x=ax = a.
  • A line through (x1,y1)(x_1, y_1) with slope mm is y−y1=m(x−x1)y - y_1 = m(x - x_1) (point-slope form). Slope is rise over run.
  • f(g(x))f(g(x)) means gg first, then ff. Order matters: usually f(g(x))≠g(f(x))f(g(x)) \ne g(f(x)).
  • A rational function has a vertical asymptote where the denominator is 0 and the numerator is not.

f(3) names one number: the height of the graph above x = 3 those inputs are left out of the domain f(g(x)) means: do g first, then f moves the whole graph h units right and k units up

function
A rule that assigns exactly one output to each input. f(3)f(3) is the output when the input is 3.
domain
The set of inputs a function accepts. The range is the set of outputs it produces.
graph of a function
All points (x,f(x))(x, f(x)) for xx in the domain. The height of the graph above x=ax = a is f(a)f(a); a filled dot is on the graph, an open circle is not.
slope
Rise over run: for a line through (x1,y1)(x_1, y_1) and (x2,y2)(x_2, y_2), mm=y2−y1x2−x1= \frac{y_2 - y_1}{x_2 - x_1}.
point-slope form
The point-slope form of a line with slope mm through (x1,y1)(x_1, y_1): y−y1=m(x−x1)y - y_1 = m(x - x_1). Slope-intercept form is y=mx+by = mx + b.
piecewise function
A function defined by different formulas on different parts of its domain, such as f(x)=x2f(x) = x^2 for x<2x < 2 and f(x)=3x−1f(x) = 3x - 1 for x≥2x \ge 2.
composite function
A composite function feeds one output into another function: f(g(x))f(g(x)) applies gg first, then ff.
graph transformation
A change that moves or reshapes a graph: f(x−h)+kf(x - h) + k shifts it hh right and kk up; −f(x)-f(x) flips it over the xx-axis; af(x)a f(x) stretches it vertically.
rational function
A quotient of two polynomials, such as 2x+1x−4\frac{2x + 1}{x - 4}. A polynomial is a sum of terms axna x^n with whole-number powers nn.
asymptote
A line the graph approaches. A rational function has a vertical asymptote x=ax = a where its denominator is 0 and its numerator is not; a horizontal asymptote is a height the outputs settle toward as |x||x| grows large.

Exponent Rules and Rewriting Powers

Exponent rules let you write every root and fraction as a power: 1/(x^n) = x^(−n) and n√(x^m) = x^(m/n) . Add exponents to multiply, subtract to divide, multiply for a power of a power, and remember an exponent applies only to the base it touches and never splits over a sum.

  • Multiply powers of the same base: add exponents. Divide: subtract. Power of a power: multiply.
  • x−n=1xnx^{-n} = \frac{1}{x^n}. A negative exponent means reciprocal, never a negative number.
  • xm/n=(xn)mx^{m/n} = \left(\sqrt[n]{x}\right)^m. Take the root first to keep numbers small: 82/3=22=48^{2/3} = 2^2 = 4.
  • An exponent applies only to what it touches: 3x−2=3x23x^{-2} = \frac{3}{x^2}, but (3x)−2=19x2(3x)^{-2} = \frac{1}{9x^2}.
  • Exponents do not split over sums: (x+3)−1≠x−1+3−1(x + 3)^{-1} \ne x^{-1} + 3^{-1} and x2+9≠x+3\sqrt{x^2 + 9} \ne x + 3.

so x^m⋅x^n = x^(m + n) , and (x^m)/(x^n) = x^(m − n) a negative exponent is a reciprocal: x^(−n) = 1/(x^n) a fractional exponent is a root: x^(1/2) = √x and x^(m/n) = (n√x)^m expressions like 3/x² + 2√x become 3x⁻² + 2x^(1/2) , ready for calculus

exponent rules
The laws for powers of one base: xmxn=xm+nx^m x^n = x^{m+n}, xmxn=xm−n\frac{x^m}{x^n} = x^{m-n}, (xm)n=xmn(x^m)^n = x^{mn}, x0=1x^0 = 1. A negative exponent is a reciprocal (x−n=1xnx^{-n} = \frac{1}{x^n}); a fractional exponent is a root (xm/n=(xn)mx^{m/n} = (\sqrt[n]{x})^m).

Algebra for Limits: Factoring and Rationalizing

Limits that give zero over zero are settled with precalculus algebra: factor and cancel a common factor, multiply by a conjugate to clear a square root, or combine a complex fraction into one. Cancel factors, never terms, and expand powers in full. The simplified expression agrees with the original everywhere except the troublesome point.

  • Factoring toolkit: common factor; difference of squares a2−b2=(a−b)(a+b)a^2 - b^2 = (a - b)(a + b); trinomials (with the acac method when the leading coefficient is not 1); cubes a3±b3a^3 \pm b^3=(a±b)(a2∓ab+b2)= (a \pm b)(a^2 \mp ab + b^2).
  • Cancel factors, never terms: x(x−4)(x−4)(x+4)\frac{x(x - 4)}{(x - 4)(x + 4)}=xx+4= \frac{x}{x + 4}, but x2+4x+2\frac{x^2 + 4}{x + 2} does not simplify.
  • Rationalizing: multiply top and bottom by the conjugate (A−B\sqrt{A} - B and A+B\sqrt{A} + B form a pair). Their product is A−B2A - B^2. Leave the other factor unmultiplied.
  • A complex fraction becomes one fraction with a common denominator; then divide.
  • Expand powers fully: (a+h)2=a2+2ah+h2(a + h)^2 = a^2 + 2ah + h^2. The middle term is the one that matters.

factor top and bottom so that factor is visible gives a simpler expression equal to the original for every x ≠ a multiplying by the conjugate √x + 2 turns it into x − 4 , which can cancel a common denominator turns the complex fraction into one fraction you can simplify

factoring
Writing an expression as a product, such as x2−9=(x−3)(x+3)x^2 - 9 = (x - 3)(x + 3) (a difference of squares). A factored form shows which factors can cancel.
rationalizing
Removing a square root from part of a fraction by multiplying top and bottom by the conjugate: A−B\sqrt{A} - B and A+B\sqrt{A} + B are conjugates, and (A−B)(A+B)(\sqrt{A} - B)(\sqrt{A} + B)=A−B2= A - B^2.
complex fraction
A fraction whose top or bottom contains fractions, such as 1x+2−12x\frac{\frac{1}{x + 2} - \frac{1}{2}}{x}. Combine the inner fractions over a common denominator to simplify it.

Trigonometry and the Unit Circle

Radians measure angles by arc length on the unit circle, where the point at angle θ is (cos θ, sin θ) . Exact values come from the first-quadrant special angles plus the quadrant signs. Tangent, secant, cosecant and cotangent are ratios of sine and cosine, and sin² x + cos² x = 1 links them. Keep calculators in radian mode.

  • Radians: π\pi radians =180∘= 180^{\circ}. To convert degrees to radians, multiply by π180\frac{\pi}{180}. Calculus always uses radians, including on the calculator.
  • On the unit circle, the point at angle θ\theta is (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta): cosine is the xx-coordinate, sine the yy-coordinate.
  • Know the first-quadrant values at π6,π4,π3\frac{\pi}{6}, \frac{\pi}{4}, \frac{\pi}{3}: 12,22,32\frac{1}{2}, \frac{\sqrt{2}}{2}, \frac{\sqrt{3}}{2}. Other quadrants use a reference angle and a sign.
  • sec⁡=1cos⁡\sec = \frac{1}{\cos}, csc⁡=1sin⁡\csc = \frac{1}{\sin}, cot⁡=cos⁡sin⁡\cot = \frac{\cos}{\sin}. sin2⁡x\sin^2 x means (sin⁡x)2(\sin x)^2.
  • Pythagorean identity: sin2⁡x+cos2⁡x=1\sin^2 x + \cos^2 x = 1; also 1+tan2⁡x=sec2⁡x1 + \tan^2 x = \sec^2 x and sin⁡2x=2sin⁡xcos⁡x\sin 2x = 2\sin x\cos x.

radians: a half turn is π , a full turn 2π the point reached is (cos θ, sin θ) , and tan θ = (sin θ)/(cos θ) sin² θ + cos² θ = 1 , the Pythagorean identity gives the exact value at any special angle

radian
A measure of angle: the length of the arc the angle cuts on a circle of radius 1. A full turn is 2π2\pi radians, so π\pi radians =180∘= 180^{\circ}.
unit circle
The circle of radius 1 centered at the origin, x2+y2=1x^2 + y^2 = 1. The point at angle θ\theta (measured counterclockwise from (1,0)(1, 0)) is (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta).
sine
Sine and cosine give the coordinates of the point at angle θ\theta on the unit circle: (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta). The others are ratios: tan⁡θ=sin⁡θcos⁡θ\tan\theta = \frac{\sin\theta}{\cos\theta}, sec⁡θ=1cos⁡θ\sec\theta = \frac{1}{\cos\theta}, csc⁡θ=1sin⁡θ\csc\theta = \frac{1}{\sin\theta}, cot⁡θ=cos⁡θsin⁡θ\cot\theta = \frac{\cos\theta}{\sin\theta}.
Pythagorean identity
An equation true for every angle. The Pythagorean identity sin2⁡θ+cos2⁡θ=1\sin^2\theta + \cos^2\theta = 1 comes from the unit circle; dividing by cos2⁡θ\cos^2\theta gives tan2⁡θ+1=sec2⁡θ\tan^2\theta + 1 = \sec^2\theta.

Exponentials and Logarithms

e^x is the exponential function calculus uses; it is always positive and passes through (0, 1) . ln x , defined for x > 0 , undoes it: e^(ln x) = x and ln (e^x) = x . Logs turn products into sums, quotients into differences and powers into multipliers, which is how you solve for a variable in an exponent.

  • ex>0e^x > 0 for every xx; e0=1e^0 = 1. The graph rises steeply to the right and approaches the xx-axis to the left.
  • ln⁡x\ln x is defined only for x>0x > 0; ln⁡1=0\ln 1 = 0, ln⁡e=1\ln e = 1. Its graph is the graph of exe^x reflected across y=xy = x.
  • Log rules: ln⁡(ab)=ln⁡a+ln⁡b\ln(ab) = \ln a + \ln b, ln⁡ab=ln⁡a−ln⁡b\ln\frac{a}{b} = \ln a - \ln b, ln⁡(ap)=pln⁡a\ln(a^p) = p\ln a. There is no rule for ln⁡(a+b)\ln(a + b).
  • ee and ln⁡\ln cancel: eln⁡x=xe^{\ln x} = x (x>0x > 0) and ln⁡(ex)=x\ln(e^x) = x. Use them to solve equations.
  • AektA e^{kt} grows when k>0k > 0 and decays when k<0k < 0; the time to double is ln⁡2k\frac{\ln 2}{k}.

it models growth by a fixed percentage; the base e ≈ 2.718 is the one calculus prefers e^(ln x) = x for x > 0 and ln (e^x) = x for every x give the log rules: ln (ab) = ln a + ln b , ln a/b = ln a − ln b , ln a^p = pln a take ln of both sides to bring it down: 2x = ln 9

exponential function
A function bxb^x with a fixed positive base b≠1b \ne 1; it changes by the same factor over equal steps in xx. The natural exponential exe^x uses e≈2.71828e \approx 2.71828. AektA e^{kt} shows exponential growth when k>0k > 0 and exponential decay when k<0k < 0.
natural logarithm
ln⁡x\ln x is the power of ee that gives xx: ln⁡x=y\ln x = y means ey=xe^y = x. It is defined for x>0x > 0. Log rules: ln⁡(ab)=ln⁡a+ln⁡b\ln(ab) = \ln a + \ln b, ln⁡ab=ln⁡a−ln⁡b\ln\frac{a}{b} = \ln a - \ln b, ln⁡ap=pln⁡a\ln a^p = p\ln a.

Inverse Functions

An inverse function runs a one-to-one function backward: f⁻¹(b) = a exactly when f(a) = b . Its graph is the reflection of f across y = x , so points swap coordinates and slopes become reciprocals. Find a formula by solving x = f(y) for y . The inverse trig functions use restricted ranges, and f⁻¹ never means 1/f .

  • f−1(b)=af^{-1}(b) = a means f(a)=bf(a) = b. So f(f−1(x))=xf(f^{-1}(x)) = x and f−1(f(x))=xf^{-1}(f(x)) = x on the right domains.
  • f−1(x)f^{-1}(x) is not 1f(x)\frac{1}{f(x)}. The −1-1 means "undo", not "reciprocal".
  • Only a one-to-one function (each output from one input; passes the horizontal line test) has an inverse. Restrict the domain if needed.
  • To find a formula: write x=f(y)x = f(y) and solve for yy.
  • arcsin⁡x\arcsin x and arctan⁡x\arctan x return angles in [−π2,π2]\left[-\frac{\pi}{2}, \frac{\pi}{2}\right]; arccos⁡x\arccos x returns angles in [0,π][0, \pi].

the inverse function f⁻¹ sends b back to a : f⁻¹(b) = a exactly when f(a) = b swaps the coordinates of every point, reflecting the graph across y = x slopes at matching points are reciprocals their inverses use restricted ranges: arcsine and arctangent give angles from −π/2 to π/2, arccosine from 0 to π

inverse function
For a one-to-one function ff, the function f−1f^{-1} that undoes it: f−1(b)=af^{-1}(b) = a exactly when f(a)=bf(a) = b. Its graph is the reflection of the graph of ff across y=xy = x. A function is one-to-one when no two inputs share an output.
inverse trigonometric function
arcsin⁡x\arcsin x, arccos⁡x\arccos x and arctan⁡x\arctan x (also written sin−1⁡x\sin^{-1} x, ...) give the angle with a given sine, cosine or tangent, from a restricted range: [−π2,π2]\left[-\frac{\pi}{2}, \frac{\pi}{2}\right] for arcsine, [0,π][0, \pi] for arccosine, (−π2,π2)\left(-\frac{\pi}{2}, \frac{\pi}{2}\right) for arctangent.

Geometry for Calculus

Calculus word problems start with a geometric equation. Right angles call for the Pythagorean theorem; nested triangles call for similar triangles and a ratio; shapes call for their area or volume formulas. Label changing quantities with letters, fixed ones with numbers, and use a ratio to reduce a formula to one variable.

  • Pythagorean theorem: in a right triangle with legs aa, bb and hypotenuse cc, a2+b2=c2a^2 + b^2 = c^2. The hypotenuse is opposite the right angle.
  • Similar triangles have equal angles, so their sides are in proportion: ab=AB\frac{a}{b} = \frac{A}{B}. Look for a small triangle inside a big one.
  • Know the area and volume formulas: circle πr2\pi r^2, semicircle 12πr2\frac{1}{2}\pi r^2, trapezoid b1+b22h\frac{b_1 + b_2}{2}h, cylinder πr2h\pi r^2 h, cone 13πr2h\frac{1}{3}\pi r^2 h, sphere 43πr3\frac{4}{3}\pi r^3.
  • Draw the picture, label what changes with letters and what is fixed with numbers, then write one equation.

the Pythagorean theorem links the sides: x² + y² = z² similar triangles: corresponding sides are in the same ratio, such as r/h = 4/10 a formula like V = 1/3 πr²h becomes a function of one variable, V = 4π/75 h³

similar triangles
Triangles with the same three angles. Their corresponding sides are in the same ratio, so rh=RH\frac{r}{h} = \frac{R}{H} for matching sides.
Pythagorean theorem
In a right triangle with legs aa and bb and hypotenuse cc: a2+b2=c2a^2 + b^2 = c^2.
volume of a cone
Volume of a cone 13πr2h\frac{1}{3}\pi r^2 h, of a cylinder πr2h\pi r^2 h, of a sphere 43πr3\frac{4}{3}\pi r^3; area of a trapezoid b1+b22h\frac{b_1 + b_2}{2}h, of a semicircle 12πr2\frac{1}{2}\pi r^2.

Parametric Equations and Vectors

Parametric equations describe a path by giving x and y as functions of a parameter t ; increasing t traces the path in a direction. Eliminating t shows the shape but loses the direction. A vector ⟨a, b⟩ records a change in position, from start to end; its magnitude is √(a² + b²) , and vectors add and scale component by component.

  • Parametric equations x=x(t)x = x(t), y=y(t)y = y(t) give a point for each tt. Make a table of tt, xx, yy, plot the points in order of tt, and draw arrows for the direction.
  • Eliminate the parameter to see the shape: solve a linear equation for tt and substitute, or square and add sines and cosines. The direction and the timing are lost when you do.
  • x=rcos⁡tx = r\cos t, y=rsin⁡ty = r\sin t is a circle of radius rr traced counterclockwise from (r,0)(r, 0); swapping sine and cosine starts at the top and goes clockwise.
  • A vector ⟨a,b⟩\left\langle a, b \right\rangle is a change: aa across and bb up. From PP to QQ it is end minus start; its magnitude is a2+b2\sqrt{a^2 + b^2}. Add vectors and multiply by numbers one component at a time.

each t gives one point (x(t), y(t)) , and together the points trace a path the path gets a direction (its orientation), which an equation in x and y cannot show eliminating t gives the shape of the path as an equation in x and y a vector, whose length √((Δx)² + (Δy)²) comes from the Pythagorean theorem

parametric equations
A pair of equations x=x(t)x = x(t), y=y(t)y = y(t) that give both coordinates of a point in terms of a third variable tt, the parameter (often time). As tt increases, the point traces a path in a direction; eliminating tt can give an equation in xx and yy, but it loses the direction and the timing.
vector
A quantity with a size and a direction, written by its components as ⟨a,b⟩\left\langle a, b \right\rangle: aa across and bb up. The vector from (x1,y1)(x_1, y_1) to (x2,y2)(x_2, y_2) is ⟨x2−x1,y2−y1⟩\left\langle x_2 - x_1, y_2 - y_1 \right\rangle; its magnitude (length) is a2+b2\sqrt{a^2 + b^2}. Vectors add and scale component by component.

Polar Coordinates and Polar Graphs

Polar coordinates name a point by an angle θ and a signed distance r . Convert with x = rcos θ and y = rsin θ . A polar curve r = f(θ) is plotted from a table of θ and r ; watch for r = 0 (the curve meets the pole) and r < 0 (the point is on the opposite ray).

  • A polar point (r,θ)(r, \theta): turn to the ray at angle θ\theta, then go rr units. A negative rr goes backward, through the pole, onto the opposite ray.
  • x=rcos⁡θx = r\cos\theta, y=rsin⁡θy = r\sin\theta, r2=x2+y2r^2 = x^2 + y^2. These connect every polar question to rectangular ones.
  • A polar curve r=f(θ)r = f(\theta) is a parametric curve with parameter θ\theta: x=f(θ)cos⁡θx = f(\theta)\cos\theta, y=f(θ)sin⁡θy = f(\theta)\sin\theta.
  • Shapes to know: r=ar = a (circle), θ=c\theta = c (line through the pole), r=acos⁡θr = a\cos\theta and r=asin⁡θr = a\sin\theta (circles through the pole), r=a+bcos⁡θr = a + b\cos\theta (limaçons, cardioid when a=ba = b), r=asin⁡(nθ)r = a\sin(n\theta) (roses).

you reach the point (r, θ) x = rcos θ and y = rsin θ as θ turns, the point traces a polar curve you see where r = 0 (the pole) and where r < 0 (the opposite ray)

polar coordinates
A way to name a point by (r,θ)(r, \theta): turn to the ray at angle θ\theta from the positive xx-axis, then go a signed distance rr along it. They convert by x=rcos⁡θx = r\cos\theta, y=rsin⁡θy = r\sin\theta and r2=x2+y2r^2 = x^2 + y^2; a curve r=f(θ)r = f(\theta) is a polar curve.

Sequences, Sigma Notation and Factorials

An infinite sequence lists a term a_n for each n . It converges if its terms approach one number and diverges otherwise; find the limit as for functions at infinity. Simplify factorial ratios by expanding the larger factorial, and read sigma notation from its starting index.

  • A sequence is a function whose inputs are n=1,2,3,…n = 1, 2, 3, \ldots Its limit is found with the tools for limx→∞f(x)\lim_{x \to \infty} f(x): leading terms, L'Hospital's rule, the squeeze theorem.
  • n!=n(n−1)(n−2)⋯2⋅1n! = n(n - 1)(n - 2) \cdots 2 \cdot 1, with 0!=10! = 1. Simplify ratios by writing the larger factorial down to the smaller: (n+1)!=(n+1)n!(n + 1)! = (n + 1)\,n!.
  • Sigma notation ∑k=1mak\sum_{k=1}^{m} a_k adds the terms from k=1k = 1 to k=mk = m. Check the starting index: it decides the first term.

an infinite sequence a_1, a_2, a_3, … , a function of n the terms settle to one number (the sequence converges) or they do not (it diverges) lim as n → ∞, a_n comes from lim as x → ∞, f(x) when that limit exists the common factorial cancels, leaving a few factors

infinite sequence
A list of numbers a1,a2,a3,…a_1, a_2, a_3, \ldots with one term for each counting number nn; a function of nn. It converges to LL if limn→∞an=L\lim_{n \to \infty} a_n = L, and diverges if its terms do not approach one number.
factorial
For a positive integer nn, n!=n(n−1)⋯2⋅1n! = n(n - 1)\cdots 2 \cdot 1; also 0!=10! = 1. Ratios simplify by expanding the larger factorial: (n+1)!=(n+1)n!(n + 1)! = (n + 1)\,n!.