QUBIX UNIVERSITY · CURRICULUM SOURCE

The Big Sheet of Graphs

Every idea in mathematics that can be reached from the origin, drawn.

Open the interactive board
681concepts
13stages
629can be drawn, 92%
493drawn so far

How much of this can be drawn?

Every concept is classified by what a picture can honestly do for it. The counts below are computed from that classification, and the build refuses to run if it names a concept the spine does not contain.

VerdictConceptsShareWhat it means
direct 467 69% The concept is a picture. Drawing it is the explanation.
frames 83 12% A process, not an object. It needs a sequence, which is what the labs in the book are for.
instance 79 12% Only a particular case can be drawn. The picture is an example of the idea, never the idea.
none 52 8% No picture is possible. It has to be argued in words or symbols.

629 of 681 concepts can be shown by some picture, and 467 of those are a picture in themselves. The remaining 52 cannot be drawn at all, and 48% of those sit in the last stage, which is the argument for having a last stage.

1

The plane itself

44 concepts · 44 drawable

By the endName a position, and say what the two numbers mean.

1
(2, 2)
(−3, 1)
(1, −3)
pointA single place, with no width and no height. Everything else on this sheet is built from these.
2
still free to slide
still free to slide
(3, 1)pinned
positionWhere something is. On a plane it takes two measurements to pin down, and neither alone is enough.
3
(3, 1)
(−2, 4)
(−4, −2)
locationThe pair of numbers that names a position. Give them to anyone with the same axes and they will find the same spot.
4
−5−4−3−2−1012345
−5−4−3−2−1012345
−5−4−3−2−1012345order is all it has
number lineA line with the numbers laid along it in order. One measurement fixes a place, because there is only one way to move.
5
−5−4−3−2−1012345
−5−4−3−2−1012345one number changed
−5−4−3−2−1012345the same one number
one dimensionOnly one way to move: forward or back. That is why a single number is enough to say where you are.
6
(1, 1)
(4, 1)moved across only
(4, −2)now down as well
two dimensionsTwo independent ways to move, so it takes two numbers. Change one and the point slides; change both and it goes anywhere.
7
(0, 0)
(3, 2)
(−2, −3)
originThe point both measurements are taken from, written (0, 0). Nothing about it is special except that everyone agrees on it.
8
axisOne of the two lines everything is measured against. Each carries its own number line.
9
(−3, 0)(2, 0)y is always 0
x-axisThe line running across, where the second measurement is zero. Every point on it has the form (something, 0).
10
(0, 3)(0, −2)x is always 0
y-axisThe line running up, where the first measurement is zero. Every point on it has the form (0, something).
11
axesThe two lines together. They cross at the origin and cut the plane into four regions.
12
(2, 3)
coordinate planeThe whole flat sheet, with axes and a grid, on which any pair of numbers has a home.
13
IIIIIIIV
geometry, as numbers
Cartesian planeThe same sheet, named after Descartes, who joined algebra to geometry by giving every point a pair of numbers.
14
(3, 1)
(1, 3)
(3, 1)(1, 3)not the same point
ordered pairTwo numbers in a fixed order, written in brackets. The order is the whole point: swap them and you have a different place.
15
a whole line of points
another whole line
(3, 1)one point
coordinateOne of the two numbers. On its own it narrows a point to a line, not to a place.
16
3
−4
x-coordinateHow far across, measured from the y-axis. Positive to the right, negative to the left.
17
2
−3
y-coordinateHow far up, measured from the x-axis. Positive above, negative below.
18
abscissa 3
abscissa −2
abscissaThe older name for the x-coordinate. You will meet it in books rather than in classrooms.
19
ordinate 2
ordinate −3
ordinateThe older name for the y-coordinate, and the one that gave "ordered pair" its name.
20
(3, 2)
plotting a pointTurning a pair of numbers into a place: go across by the first, then up by the second. Always in that order.
21
x = 3
(3, 2)
reading a pointThe reverse: drop from a marked place to each axis and read the two numbers off.
22
quadrantOne of the four regions the axes cut the plane into. Which one a point is in is decided entirely by the signs of its two numbers.
23
(2.5, 3)both positive
first quadrantTop right, where both numbers are positive. Most graphs of real quantities live here, because lengths and times are rarely negative.
24
(−2.5, 3)x negative
second quadrantTop left: x negative, y positive.
25
(−2.5, −3)both negative
third quadrantBottom left, where both numbers are negative.
26
(2.5, −3)y negative
fourth quadrantBottom right: x positive, y negative.
27
sign of a coordinateWhether each number is positive or negative. The two signs together say which quadrant you are in, without measuring anything.
28
positive directionRight along the x-axis and up the y-axis. A convention, agreed rather than discovered, but agreed everywhere.
29
negative directionLeft and down. Not smaller or lesser, just the opposite way.
30
same x, different y
gridlineA line of the grid. Every point on a vertical one shares an x-coordinate, which is what makes it useful for reading a graph.
31
(1.5, 2.5)between the dots
lattice pointA point where both numbers are whole. Easy to plot exactly, which is why tables of values tend to use them.
32
shape only
now it has size
tick markThe small strokes counting units along an axis. Without them the picture has shape but no size.
33
1 per square
10 per square, same rule
scaleHow much one step of the grid is worth. Change it and the same relationship can look steep or nearly flat.
34
2 by 2
unitOne step. Everything measured on the plane is counted in these, and the answer means nothing until you say what one is.
35
looks square
looks round
equal scalingBoth axes using the same size of step. Only then does a square look square and an angle look like itself.
36
now a strip
now an oval
distorted scalingAxes with different steps. Legal and often useful, but shape can no longer be trusted: circles turn into ovals and steepness lies.
37
of what?
timedistance
axis labelThe name of what each axis measures. Without it a graph is a shape with no subject.
38
(0, 0)
(0, 0)nothing special about it
the point (0, 0)The origin written as a pair. It is an ordinary point that happens to be where both measurements read nothing.
39
that is y = 2
that is x = 3
distance from an axisThe shortest way to an axis, which is straight at it. That distance is exactly what the other coordinate measures.
40
y > 0
y < 0
above and belowWhich side of the x-axis a point is on, which is just the sign of its second number.
41
x > 0
x < 0
left and rightWhich side of the y-axis a point is on, which is just the sign of its first number.
42
origin(3, 2)
origin(5, 3)same point, new numbers
reference frameThe origin and axes you have agreed to measure from. Move them and every coordinate changes, though nothing has actually moved.
43
(3, 1)
(3, 1)?the same pair, elsewhere
convention (input first)The agreement that the first number is measured across. Nothing forces it; everyone simply does the same thing so the numbers travel.
44
(3, 1)
(1, 3)
(3, 1)(1, 3)mirrored in y = x
the pair (3, 1) against (1, 3)Two different points from the same two numbers. This is the clearest reason the order has to be fixed.
2

Straight lines and segments

50 concepts · 50 drawable

By the endMeasure a line: how long, how steep, where it crosses.

45
still going
straight lineThe path that never turns. It carries on past the edge of any picture of it, which is why a drawn line is always a sample of one.
46
same direction, less of it
line segmentA piece of a line with two ends. Unlike a line it has a length you can measure.
47
same start, opposite direction
rayHalf a line: one end, and no other. A beam of light is the usual picture.
48
endend
endendthe other stays
endpointWhere a segment stops. Two of them, and between them everything belongs to the segment.
49
inside
not insidean endpoint is not interior
interior pointA point on a segment that is not an end. Between, strictly.
50
ABC
ABCno longer between
betweennessOne point lying on the segment joining two others. It is the idea that lets a line be ordered.
51
4 across, 3 up
5
length of a segmentHow far apart the two ends are. Drop the horizontal and vertical legs and it is the hypotenuse of a right triangle.
52
Δx = 4Δy = 3
√(16 + 9) = 5
distance formulaPythagoras written for two coordinate pairs: square the two differences, add, take the root.
53
gives 5
gives 13
Pythagoras in the planeThe rule that makes distance measurable at all. Every length on this sheet is an application of it.
54
midpoint
midpointit follows
midpointThe point exactly halfway. Its two coordinates are the averages of the two ends.
55
(−3 + 3) ÷ 2 = 0
(−2 + 2) ÷ 2 = 0
(0, 0)
midpoint formulaAverage each coordinate separately. There is nothing more to it than that.
56
section formulaThe midpoint generalised: a point dividing a segment in any stated ratio, not just in half.
57
ABP
ABP
internal divisionA dividing point that lies inside the segment. Both parts point the same way.
58
ABP
ABP
external divisionA dividing point beyond one end. The ratio is signed, and one part now runs backwards.
59
ratio along a segmentHow the two parts compare. It fixes a point without ever mentioning a length.
60
the third is off it
collinear pointsPoints that all sit on one line. Three points are collinear when the slope between any two of them is the same.
61
y is always 2
horizontal lineA line of constant height. Its equation names only y, because x is free to be anything.
62
x is always 2
vertical lineA line of constant position across. Its equation names only x, and it is the one kind of line that is not a function.
63
oblique lineAny line that is neither flat nor upright. Both coordinates change as you move along it.
64
2 up per 4 across
4 up per 4 across
4 up per 2 across
slopeHow much the line climbs for each step across. One number that describes the whole line, because a line never changes its mind.
65
gradientThe same number as slope, under the name used in British schools and in physics.
66
+3
−3
riseThe vertical part of a step along the line. Negative if the line is going down.
67
4
2same line, smaller step
runThe horizontal part of the same step. Usually taken as positive, so the sign of the answer comes from the rise.
68
3 ÷ 4 = 0.75
1.5 ÷ 2 = 0.75
rise over runDivide one by the other and the size of the step drops out. That is why any two points on a line give the same slope.
69
slope 0.3
slope 2.5
slope −2.5, just as steep
steepnessHow sharply a line climbs. The bigger the slope in size, the steeper, whichever way it leans.
70
positive slopeThe line climbs left to right. As the input grows, so does the output.
71
negative slopeThe line falls left to right. As the input grows, the output shrinks.
72
rise 0
0 ÷ anything = 0
zero slopeNo climb at all. Move as far across as you like and the height never changes.
73
slope 8
slope 40
no run: undefined
undefined slopeAn upright line has no run to divide by, and dividing by nothing is not an answer. That is why it is undefined rather than infinite.
74
45°slope 1
27°slope 0.5
63°slope 2
angle of inclinationThe angle the line makes with the horizontal. Slope and angle carry the same information in different units.
75
still never meeting
parallel linesSame slope, different position. They never meet, however far either is extended.
76
2 × −0.5 = −1
perpendicular linesCrossing at a right angle. Their slopes multiply to −1, which is the algebraic form of that fact.
77
2 → −1/2
1/3 → −3
negative reciprocalFlip the fraction and change the sign. Doing that to a slope turns a line through a right angle.
78
(2, 0)
(−3, 0)
x-interceptWhere the line crosses the horizontal axis, so the output is zero. Solving a linear equation is exactly finding this.
79
(0, 2)
(0, −3)same slope, moved down
y-interceptWhere the line crosses the vertical axis, so the input is zero. It is the starting value before anything happens.
80
y = 0.5x + 1
fits0.5(2) + 1 = 2
does notso it is off the line
equation of a lineThe condition every point on the line satisfies, and no other point does. The line and the equation are the same object.
81
straight
no longer linear
linear equationAn equation where the letters appear only to the first power. That restriction is exactly what makes the graph straight.
82
slides up and down
pivots about the intercept
slope-intercept formy = mx + c. The two numbers you can read straight off a graph: how steep, and where it starts.
83
(1, 0.5)
same point, new line
point-slope formBuilt from one point and a slope. Useful when you know where a line goes and how steep it is, but not where it crosses.
84
only one fits both
two-point formTwo points are enough to fix a line, because they fix both the slope and the position.
85
3x + 4y = 12
(4, 0)(0, 3)both fall out easily
standard formBoth letters on one side, as Ax + By = C. It treats x and y evenly, which suits solving pairs of equations.
86
3x + 4y = 12
3x + 4y − 12 = 0
general formEverything moved to one side, equal to zero. It is the form a computer prefers, because there is nothing to rearrange.
87
x/4 + y/3 = 1
intercept formWritten from the two lengths the line cuts off the axes. It says at a glance where the line meets each one.
88
Pshortest
Plonger
distance from a point to a lineThe shortest route, which is always the perpendicular one. Any other path to the line is longer.
89
Pfoot
Pfootthe foot moves too
foot of the perpendicularWhere that shortest route lands. It is the point on the line closest to P.
90
slopes multiply to −1
angle between two linesHow far one must turn to lie along the other. It depends only on their slopes, not on where they cross.
91
AB
AB
perpendicular bisectorThe line cutting a segment in half at a right angle. Every point on it is the same distance from both ends.
92
AB
AB
ABa whole line
locus of equidistant pointsThe set of all points equally far from two others. It turns out to be exactly that perpendicular bisector.
93
fromto
fromtosame segment, opposite journey
direction of travelA segment with an arrow on it. Adding direction turns a length into the beginning of a vector.
94
the line is the set
a line as a set of pointsNot a stroke of ink, but every point whose coordinates satisfy the equation. The drawn line is just the ones that fit on the page.
3

Regions, shapes and systems

52 concepts · 52 drawable

By the endTurn a picture of a region into arithmetic, and back.

95
polygonA closed shape made only of straight sides. Add a side and you have a new one; there is no upper limit.
96
vertexA corner, where two sides meet. A polygon has exactly as many corners as sides.
97
sideOne straight edge. Going round them all in order is what closes the shape.
98
still a triangle
three triangles
triangleThree points not in a line, joined up. The simplest polygon, and the one every other polygon can be cut into.
99
the hypotenuse is a length
right triangleOne corner square. This is the shape Pythagoras applies to, which is why every distance on this sheet is one.
100
==
isosceles triangleTwo sides equal, and with them two equal angles. Symmetry about a line through the odd corner.
101
equilateral triangleAll three sides equal, so all three angles are sixty degrees. The most symmetric triangle there is.
102
now a rectangle
quadrilateralFour straight sides. Every rectangle, square, rhombus and trapezium below is one of these with something extra promised.
103
rectangleFour right angles. Opposite sides come out equal as a consequence, not as a second condition.
104
sixteen unit squares
squareA rectangle whose sides are all equal. It is the unit of area: everything else is measured in these.
105
same base, same height
parallelogramBoth pairs of opposite sides parallel. Push a rectangle sideways and you have one, with the same area.
106
rhombusA parallelogram with all four sides equal. Its diagonals cross at right angles.
107
average them
trapeziumExactly one pair of parallel sides. Its area is the average of those two, times the distance between them.
108
6 + 4 + 6 + 4 = 20
perimeterThe distance all the way round. Add the sides; there is no formula beyond that.
109
half of 6 × 4
same area
still the same
area of a triangleHalf the base times the height. Slide the top corner along a parallel line and the area never changes, because neither does.
110
(−3,−2)(3,−1)(0,3)
no height needed
shoelace formulaArea straight from the corner coordinates, with no height to find. Multiply crosswise round the shape and subtract.
111
half |4·3 − 1·1|
the determinant itself
determinant formThe same computation written as a determinant. It is why area and determinants turn out to be the same idea.
112
three triangles
area of a polygonCut it into triangles from one corner and add them. Any polygon can be cut this way, so nothing else is needed.
113
regionA part of the plane rather than a line through it. Regions are what inequalities describe.
114
half-planeEverything on one side of a line. Two of them, and the line between, make up the whole plane.
115
inequalityA condition met by a whole region rather than by a single answer. Its picture is shading, not a point.
116
x + y = 2
0 ≤ 2 ✓
x + y ≤ 2
linear inequalityThe boundary is a straight line, so the region is a half-plane. Test any single point to find out which side is wanted.
117
edge excluded
edge included
strict inequalityThe boundary itself is excluded, drawn dashed. The difference matters at the edge and nowhere else.
118
boundary lineThe edge of a region. Solid when it belongs to the region, dashed when it does not.
119
the overlap
shaded regionWhere two or more conditions hold at once. Each one alone allows more; together they allow less.
120
smaller each time
feasible regionEverything allowed by every constraint. Add a constraint and it can only shrink.
121
stays inside
the join leaves it
convex regionJoin any two of its points and the segment stays inside. Feasible regions from linear constraints are always like this.
122
bounded regionIt fits inside some box. A bounded region always has a highest and a lowest point of anything measured on it.
123
still going
unbounded regionIt runs on without limit. A quantity measured over one may have no largest value at all.
124
intersection of two linesWhere both lines pass at once. Unless they are parallel, there is exactly one such place.
125
(2, 1)
point of intersectionThe one point satisfying both equations. Reading off its coordinates is solving the pair.
126
many points fit
many fit this too
only one fits both
simultaneous equationsTwo conditions to hold at the same time. Each is a line; the answer is where they meet.
127
now nothing fits all three
system of equationsAny number of equations considered together. More equations usually means fewer answers, and often none.
128
nearer parallel, still one point
unique solutionDifferent slopes, so the lines must cross, and can only cross once.
129
meets somewhere
meets far away
never
no solutionSame slope, different intercept. Parallel lines never meet, so no pair of numbers satisfies both.
130
no meeting
every point solves both
infinitely many solutionsThe two equations describe the same line, so every point on it solves both. Usually one is a multiple of the other.
131
also consistent
consistent systemIt has at least one solution. Either the lines cross, or they coincide.
132
no common point
inconsistent systemNo solution at all. The conditions contradict each other, and the algebra ends in something false like 0 = 5.
133
3x + 5y = 5
6x + 10y = 10, the same line
dependent equationsOne equation carries no new information, because it is a rescaling of another. Two equations, one condition.
134
(2, 1)
graphical solutionDraw both and look. It gives an answer you can see and trust to about a grid square, which is often enough.
135
(2, 1)
substitution methodUse one equation to express a letter, then put it into the other. Geometrically, you have fixed one coordinate first.
136
a horizontal line: x is gone
(2, 1)
elimination methodAdd or subtract the equations so one letter cancels. The combination is a third line through the same crossing.
137
bestat a corner
linear programmingFind the best allowed value of something. Because the region is convex and the objective is straight, the answer is always at a corner.
138
the last that still touches
objective functionThe quantity being maximised or minimised. Its lines of equal value are parallel, so sliding them across the region finds the best point.
139
bestfive to check, not infinitely many
corner pointA vertex of the feasible region. Checking only these is enough, which turns an infinite search into a short list.
140
three crossings
concurrent
concurrencyThree or more lines through one point. It is not automatic, which is why it is worth a name when it happens.
141
concurrent
mediansEach line from a corner to the midpoint of the opposite side. All three always pass through one point.
142
centroidthe average of the corners
centroidWhere the medians meet, and the average of the three corners. A cardboard triangle balances on it.
143
circumcentreThe centre of the circle through all three corners. It is equally far from each, so it sits on every perpendicular bisector.
144
touching all three sides
incentreThe centre of the largest circle that fits inside. It is equally far from each side, rather than from each corner.
145
an obtuse triangle pushes it out
orthocentreWhere the three altitudes meet. Unlike the others it can fall outside the triangle entirely.
146
always
Euler lineThe circumcentre, centroid and orthocentre always lie on one line, in that order, whatever the triangle. A surprise that has no obvious reason to be true.
4

The function idea

50 concepts · 47 drawable

By the endSay what a rule promises, and test whether a picture keeps it.

147
still a relation
the middle input has no partner
relationAny pairing at all between two sets. No promises: an input may have many partners, or none.
148
one input has two
one arrow each
functionA relation that promises exactly one output for every allowed input. That single promise is the whole definition.
149
36double it
34add onesame input, new rule
ruleThe instruction that turns an input into an output. It can be words, a formula, a table, or a machine.
150
36double it
510double it
−2−4double it
inputWhat goes in. Choosing it is the one free act; everything after is decided by the rule.
151
36
510settled, not chosen
outputWhat comes out. You do not choose it; the input and the rule between them settle it.
152
−5−4−3−2−1012345every number allowed
−5−4−3−2−1012345from −2 upward
−5−4−3−2−1012345one value refused
domainEvery input the rule will accept. Stating it is part of stating the function, not an afterthought.
153
−5−4−3−2−1012345x² − 2
−5−4−3−2−1012345never below −2
−5−4−3−2−1012345the range
rangeEvery output the rule actually produces. Not what it might produce: what it does.
154
the range
the codomain, larger
codomainThe set outputs are allowed to come from. It may be bigger than the range, and often is, because it is declared rather than computed.
155
39
416
imageWhere a particular input is sent. The image of 3 under squaring is 9.
156
39and −3 as well
−1nothingno square is negative
preimageWhich input produced a given output. Running the arrow backwards, which may find one answer, several, or none.
157
FRJPParisTokyo
mappingAnother word for a function, used when the sets are not numbers. It emphasises the sending rather than the calculating.
158
a fork
arrow diagramTwo columns and arrows between them. The clearest way to see whether a rule keeps its promise.
159
{(−2,−1), (0,1), (1,2), (3,0)}
−2013−1120
set of ordered pairsA function written out as a list of what goes to what. Nothing is hidden: the list is the whole rule.
160
one arrow
which?
well-definedThe rule settles on one answer, and the same answer every time. Without this, nothing built on top of it can be trusted.
161
sharing is fine
splitting is not
one input one outputThe promise, stated as plainly as it can be. Two inputs may share an output; one input may not split.
162
24
249no longer a function
the forkOne input with two arrows. It is the only way a relation fails to be a function, and it is always fatal.
163
never more than one hit
vertical line testSweep an upright line across a graph. It works because a vertical line collects every output at one input.
164
two hits
one hit
none
horizontal line testSweep a flat line instead. Two hits means two inputs share an output, so the rule cannot be reversed.
165
the output is shared
one-to-oneNo output is used twice. It is the condition that lets a rule be run backwards.
166
one spare, still injective
injectiveThe formal name for one-to-one. Every output is used at most once; some may go unused.
167
3−39
many-to-oneSeveral inputs landing on the same output. Perfectly legal, and what squaring does to 3 and −3.
168
one output unreached
ontoNothing in the target is left out. Every possible output is actually reached by something.
169
surjectiveThe formal name for onto. Nothing in the codomain is wasted.
170
still a function backwards
bijectiveBoth at once: nothing shared and nothing left out. A perfect pairing, and exactly what an inverse needs.
171
f(x)the output f gives to x
f × xf is a rule, not a quantity
function notationA compact way to name the output a rule gives an input. The brackets mean "apply", never "multiply".
172
f(x) = 2x + 1
f(4) = 2(4) + 1= 9
f(x)Read "f of x". The letter names the rule, the bracket holds whatever it is being applied to.
173
492x + 1
012x + 1
evaluatingInput given, output wanted. Substitute and compute; there is only ever one answer.
174
492x + 1 = 9
3−39x² = 9legal: the plural is on the input side
solving for the inputOutput given, input wanted. The arrow runs backwards, and there may be more than one answer, or none.
175
independent variableThe one you set. It goes across, and nothing in the rule constrains it beyond the domain.
176
you did not pick 2.8
dependent variableThe one that follows. It goes up, and you never choose it directly: the rule and your input decide it.
177
f( 4 )
f( a )
f( x + h )the same procedure
argumentWhatever sits inside the brackets. It need not be a number: an expression works the same way.
178
f(2) = 5
f(4) = 9
value of a functionThe number that comes out at a stated input. One input, one value, always.
179
f(⬚) = 2⬚ + 1
f(4) = 2(4) + 1= 9
f(x+h) = 2(x+h) + 1the bracket holds it together
substituting into a ruleWhatever arrives goes into every blank. Reading the rule with a blank in it makes the next step obvious.
180
2x + 1
table of valuesA few rows of the rule, written out. It cannot show every input, but it can show the pattern.
181
graph of a functionEvery input-output pair plotted at once. The table is a sample of it; the graph is all of it.
182
double, then add one
f(x) = 2x + 1
four representationsWords, table, formula and graph. Fluency is moving between them in any direction, not reciting each in turn.
183
−5−4−3−2−1012345nothing negative
−5−4−3−2−1012345nothing that divides by zero
natural domainEverything the formula will take, before anyone restricts it further. Found by scanning for what would break.
184
−5−4−3−2−1012345
−5−4−3−2−1012345x cannot be 2
implied domainThe domain a formula states without anyone writing it down. Silence is not permission: it is the formula speaking.
185
−6−5−4−3−2−101234567891011121314x² takes anything
−6−5−4−3−2−101234567891011121314no negative lengths
−6−5−4−3−2−101234567891011121314set by the situation
contextual domainNarrowed by what the quantity means rather than by the algebra. A count cannot be negative even when the formula would allow it.
186
two inputs per height
one input per height now
restricted domainInputs deliberately withheld. It is how a rule that cannot be reversed is made reversible.
187
−5−4−3−2−1012345
−5−4−3−2−1012345the same fact, drawn
excluded valueA single input the rule refuses. Drawn as a hollow endpoint, or as a hole in a curve.
188
1/0.5 = 2
1/0.25 = 4
no value at all
division by zeroThe commonest reason an input is refused. It is not that the answer is large: there is no answer.
189
nothing to the left
even root of a negativeThe other common refusal. No real number squares to something negative, so the root has nothing to return.
190
−5−4−3−2−1012345
−5−4−3−2−1012345
−5−4−3−2−1012345
interval notationA stretch of the line written in brackets. Square includes the end, round excludes it.
191
−5−4−3−2−1012345(−2, 3)
−5−4−3−2−1012345even near the edge
open intervalNeither end included. Every point in it has room on both sides, which is what makes it useful for limits.
192
−5−4−3−2−1012345[−2, 3]
−5−4−3−2−1012345
closed intervalBoth ends included. A continuous rule on one of these always attains a highest and a lowest value.
193
−5−4−3−2−1012345
−5−4−3−2−1012345
half-open intervalOne end in, one out. Common when a quantity starts somewhere definite and runs on without reaching a limit.
194
−5−4−3−2−1012345
−5−4−3−2−1012345now two pieces
−5−4−3−2−1012345three
union of intervalsTwo or more stretches taken together. Removing a point from the line always produces one.
195
−5−4−3−2−1012345[1, ∞)
−10−9−8−7−6−5−4−3−2−1012345678910111213141516171819202122232425262728293031323334353637383940still going
unbounded intervalOne end and no other. Infinity always takes a round bracket, because it is a direction rather than a place you arrive at.
196
{ x : x > 2 }every x more than 2
−5−4−3−2−1012345the same set
set-builder notationA set written as the condition its members satisfy, rather than as a list. It works when the list would be infinite.
5

Families of curves

67 concepts · 65 drawable

By the endRecognise a shape from its rule, and a rule from its shape.

197
still flat
constant functionThe same output whatever goes in. Flat, and the only rule whose graph a horizontal line test fails everywhere.
198
a rule and its inverse
identity functionGives back exactly what it was handed. It is the diagonal, and the mirror every inverse is reflected in.
199
linear functionOne steepness, everywhere. Equal steps in give equal steps out, which is what makes it the simplest kind of change.
200
same slope, new intercept
affine functionA line that need not pass through the origin. Strictly, only lines through the origin are linear; the rest are affine.
201
quadratic functionA squared term is enough to bend it. One turning point, and a mirror through it.
202
parabolaThe curve a quadratic draws. Every point on it is equally far from a fixed point and a fixed line, which is the other way to define it.
203
(0, 0)
(2, −2)
vertex of a parabolaThe single turning point, and the only place the curve is flat. Everything about a quadratic is easiest to read from here.
204
it follows the vertex
axis of symmetryThe vertical line the curve folds onto itself along. It always runs through the vertex.
205
x² − 2x − 2
(1, −3)(x − 1)² − 3
completing the squareRewriting a quadratic so the vertex can be read straight off. The curve does not change; only the way it is written does.
206
slides sideways
slides up
flips and flattens
vertex forma(x − h)² + k. The two numbers h and k are exactly where the vertex is, so no work is needed to find it.
207
0.6(x + 2)(x − 3)
factored formWritten as a product, so the roots are visible. Each bracket vanishing gives one crossing.
208
never reaches zero
rootAn input that makes the output zero. On a graph it is a crossing of the horizontal axis.
209
infinitely many
zero of a functionThe same thing as a root, under the name used when the rule is not a polynomial.
210
b² − 4ac > 0
b² − 4ac = 0
b² − 4ac < 0
discriminantOne number that says how many roots there are before you find any. Positive gives two, zero gives one, negative gives none.
211
touches, does not cross
repeated rootThe curve touches the axis and turns back instead of crossing. Two roots that have landed on the same place.
212
up to two, not always two
cubic functionA third power allows two turns. Both ends head opposite ways, so it always crosses the axis at least once.
213
still quartic
quartic functionA fourth power allows three turns, and both ends go the same way. That is why it can have a W shape.
214
polynomialSums of whole-number powers. Smooth everywhere, defined everywhere, and with no breaks or corners anywhere.
215
degreeThe highest power present. It caps the number of turns at one less, and decides what the ends do.
216
both ends up
both ends down
ends disagree
leading coefficientThe number on the highest power. Its sign alone decides which way the far ends of the curve point.
217
the turns become invisible
end behaviourWhat happens far from the origin, where the highest power drowns out everything else.
218
turning pointWhere the curve stops rising and starts falling, or the reverse. Momentarily flat.
219
localhigher
local maximumHigher than everything immediately around it, though possibly not the highest anywhere.
220
locallower
local minimumLower than everything immediately around it. The dip a ball would settle in, if the curve were a track.
221
climbs without limit
global maximumThe highest the rule ever gets, anywhere in its domain. A rule may have none at all.
222
falls without limit
global minimumThe lowest it ever gets. On a closed interval a continuous rule always has one; on an open one it may not.
223
the denominator is zero at 1
rational functionOne polynomial divided by another. Wherever the bottom vanishes the rule has nothing to give, so the curve breaks.
224
closer, never touching
asymptoteA line the curve gets arbitrarily close to and never reaches. It is a statement about forever, not about the visible part.
225
no bound either side
vertical asymptoteAn upright line the curve runs alongside without limit. It marks an input the rule refuses.
226
settles at 2
horizontal asymptoteA level the curve settles toward far out. It answers what happens in the long run.
227
the gap closes
oblique asymptoteA slanted line approached at both ends. It appears when the top of a fraction outgrows the bottom by exactly one power.
228
(x² − 1) ÷ (x − 1)= x + 1, except at x = 1
hole in a graphA single point missing from an otherwise unbroken curve. It happens when a factor cancels, which is illegal at exactly one input.
229
reciprocal functionOne over the input. Two branches, each hugging both axes, and nothing at all at zero.
230
hyperbola (rectangular)The curve whose two coordinates always multiply to the same number. Double one and the other halves.
231
squaring, mirrored
square root functionUndoes squaring, but only for inputs that are not negative. It starts at the origin and flattens as it climbs.
232
the restriction moved with it
radical functionAny rule with a root in it. Shifting what is under the root moves where the curve is allowed to start.
233
one accepts negatives, one does not
cube root functionUndoes cubing, and unlike the square root it accepts negatives, because cubing keeps the sign.
234
corner
the negative half folded up
absolute value functionDistance from zero, so the sign is thrown away. Two straight pieces meeting at a corner.
235
a join is possible, not required
piecewise functionDifferent rules on different stretches. One function, described in parts, which is how most real quantities behave.
236
jumps every two
step functionConstant, then it jumps, then constant again. Postage and parking charges work exactly like this.
237
−1.3 goes to −2
floor functionThe whole number at or below the input. It rounds down, including for negatives, where that surprises people.
238
one step apart, except at whole numbers
ceiling functionThe whole number at or above the input. It rounds up, always.
239
the size is gone, the sign remains
signum functionReports only the sign: minus one, nothing, or one. It throws away everything except direction.
240
level at 4, then it pulls away
exponential functionEqual steps in multiply the output by a fixed factor. That is why it eventually outruns any power, however large.
241
steeper
now decaying
baseThe factor each step multiplies by. Bigger than one and it grows; between zero and one and it decays.
242
looks gentle
the same rule
exponential growthThe amount added depends on how much there already is. Slow at first, and then not.
243
exponential decayA fixed fraction lost each step, so it approaches nothing without ever arriving.
244
another 3 units
always 3
doubling timeHow long growth takes to double. For an exponential it is the same however much there already is, which is the surprising part.
245
always 3
half-lifeHow long decay takes to halve. Like doubling time, it does not depend on where you start.
246
e ≈ 2.718
height 2.718, slope 2.718
the number eThe one base whose steepness equals its own height everywhere. About 2.718, and it is not a coincidence that calculus keeps finding it.
247
mirrored in y = x
logarithmAsks what power gives this number. It is the exponential run backwards, so it undoes it.
248
still rising, very slowly
logarithmic functionDefined only for positive inputs, and it climbs ever more slowly. It never stops climbing, which is easy to miss.
249
at e, 1
ln x above, 1/x below
natural logarithmThe logarithm to base e. It is the one whose slope at x is exactly one over x, which is why calculus prefers it.
250
each digit is one step
common logarithmThe logarithm to base ten. It counts digits, which is why it is the one used for scales like pH and decibels.
251
log(ab) = log a + log b
log(a/b) = log a − log b
log(aⁿ) = n log a
log lawsThey turn multiplying into adding. That is what made logarithms worth inventing, three centuries before calculators.
252
repeating
sineThe height of a point going round a circle, plotted against the angle. It repeats forever because the circle does.
253
a quarter turn apart
cosineThe across-ness of the same circling point. The identical wave, started a quarter turn earlier.
254
tangent functionSine divided by cosine. Wherever cosine is zero it has nothing to give, so it breaks and starts again.
255
taller, same timing
amplitudeHow far the wave reaches from its centre line. It changes the height and nothing else.
256
twice as often
periodThe horizontal length of one full repeat. Changing it stretches the wave sideways without changing its height.
257
same wave, later
phase shiftThe wave slid sideways. Nothing about its shape changes; only where it starts.
258
frequency (of a wave)How many repeats fit into a given stretch. It is the period turned upside down.
259
arc = radius
π radians
radian measureAngle measured by the arc it cuts, in units of the radius. It is the measure that makes calculus of waves come out clean.
260
the same as π radians
degree measureA full turn cut into 360 parts. Older, more familiar, and arbitrary: 360 was chosen because it divides neatly.
261
(cos, sin)
(cos, sin)cosine has gone negative
unit circleThe circle of radius one. Every point on it hands you a cosine and a sine at once, which is where both come from.
262
identical each time
periodicityRepeating the same shape at fixed intervals, forever. Knowing one cycle is knowing all of them.
263
sinusoidAny wave of this shape, whatever its height, length and starting point. Sound, light and alternating current are all made of these.
6

Moving a curve

31 concepts · 29 drawable

By the endPredict where a graph goes before drawing it.

264
same family
parent functionThe plainest member of a family, before anything is done to it. Every other member is this one moved, stretched or flipped.
265
transformationA rule applied to a whole curve at once. The shape is carried somewhere else rather than redrawn.
266
every point moved 2 right, 1 down
translationSliding without turning or resizing. Every point moves the same distance in the same direction.
267
minus, so it went right
plus, so it went left
horizontal shiftMoving sideways. It is done inside the bracket, and it moves the opposite way to the sign you write.
268
plus, so it went up
no surprise here
vertical shiftMoving up or down. It is done outside the bracket, and it moves the way the sign says.
269
sideways
sideways again, squeezed
inside the bracketChanges made to the input, before the rule runs. They act sideways, and they act backwards.
270
up
taller
outside the bracketChanges made to the answer, after the rule has run. They act vertically, and they behave as written.
271
x = 0
now at x = 2x − 2 must equal 0, so x = 2
shift against the signx − 2 sends the curve right, not left. The bracket asks what to feed the rule, so to get the old answer you must arrive two later.
272
reflectionFlipping the curve across a line, as a mirror would. Distances to the mirror are preserved; sides are swapped.
273
heights reversed
reflection in the x-axisNegate the answer, and the curve turns upside down. Anything sitting on the axis does not move.
274
reflection in the y-axisNegate the input, and left swaps with right. For an even curve nothing appears to happen at all.
275
the inverse
reflection in y = xSwap the two coordinates and the diagonal becomes the mirror. This is exactly what taking an inverse does.
276
the axis did not move
stretchPulling the curve away from a line, so distances from it are multiplied. The line itself stays put.
277
compressionThe same operation with a factor under one: everything is pulled toward the line rather than away from it.
278
height doubled
vertical stretchMultiply the answer and every height scales. It happens outside the bracket, so the factor means what it says.
279
factor 2 in, half the width out
and the other way
horizontal stretchMultiply the input and the curve squeezes sideways by the reciprocal. Feed it 2x and it finishes in half the distance.
280
flipped as well
scale factorThe number every distance is multiplied by. Above one it grows, below one it shrinks, and negative flips as well as scales.
281
centre
centreaway from the centre
dilationA stretch about a fixed centre. Every point moves along the line joining it to that centre.
282
the crossings did not move
the same two points
invariant pointA point a transformation leaves exactly where it was. It is the anchor the rest of the picture turns around.
283
2x², then down 3
the vertex landed elsewhere
order of transformationsDoing them in a different order gives a different curve. Stretch then shift is not shift then stretch.
284
0.5(x − 1)² − 2
composition of transformationsSeveral applied one after another, read from the inside out. The written form is a set of instructions in reverse.
285
nothing changed: f(−x) = f(x)
even functionFeeding it the negative gives back the same answer. Its graph is unchanged by a flip in the vertical axis.
286
nothing changed: f(−x) = −f(x)
odd functionFeeding it the negative flips the answer too. Turning the graph half a turn about the origin leaves it alone.
287
symmetry about the y-axisThe left half is the right half, mirrored. Only even rules do this.
288
(2, 0.8)
(−2, −0.8)through the origin
symmetry about the originHalf a turn about the origin puts the curve back on itself. Every point has a partner directly opposite.
289
the same square, order 4
rotational symmetryTurning by a fixed fraction of a full circle leaves the shape looking identical. How many such turns is its order.
290
flipped in both axes
image curveWhat is left after the transformation has been applied. The original is the object; this is its image.
291
(x, y) → (x + 3, y − 1)
every point, the same way
mapping notationWriting where a general point goes, rather than describing the move in words. It leaves no room for ambiguity.
292
(1, 0)(0, 1)
(2, 1)(−1, 2)those are the two columns
transformation matrixA small grid of numbers that performs the move by multiplication. Its two columns are simply where the two unit arrows land.
293
(x, y) → (−y, x)
rotation about the originTurning everything by the same angle around a fixed point. Distances from that point never change.
294
the base stayed, the top slid
shearSliding each row sideways by an amount that grows with its height. A rectangle becomes a leaning one, of exactly the same area.
7

Conics, loci and other coordinates

46 concepts · 45 drawable

By the endDescribe a curve by the condition its points satisfy.

295
each is 2.5 from the origin
the condition drew the circle
locusThe set of every point obeying some condition, and nothing else. Curves stop being shapes you draw and become answers to a question.
296
the same distance
circleEvery point the same distance from one point. The condition is short enough to check on any point you like.
297
(0, 0)
(1.5, −1)
centreThe point every distance is measured from. Move it and the whole circle goes with it, unchanged in size.
298
radiusThe fixed distance in the condition. It is the only thing that decides how big the circle is.
299
(x − a)² + (y − b)² = r²
(1, −0.5)a = 1, b = −0.5, r = 2.2
equation of a circlePythagoras applied to the condition: the squared distance from the centre equals the squared radius.
300
x² + y² − 2x + y − 4 = 0
(x − 1)² + (y + 0.5)² = 5.25
general form of a circleThe same circle multiplied out, with the centre hidden. Completing the square in both letters puts it back.
301
no chord is longer
diameterA chord that passes through the centre, and the longest one there is. It is twice the radius.
302
chordA straight segment joining two points on the circle. It cuts the circle into two pieces.
303
the rest of the way round
arcA stretch of the circle itself, rather than of the plane inside it. Two points cut off a short one and a long one.
304
a quarter turn, a quarter of the area
sectorThe slice between two radii, arc included. A pie piece, and its area is the fraction of the turn it takes up.
305
the chord moved in
segment of a circleThe region a chord cuts off, without the centre. What is left of a sector once the triangle is removed.
306
tangent to a circleA line touching at exactly one point. It always meets the radius there at a right angle, which is the fact everything else is built on.
307
now a tangent
secant to a circleA line cutting the circle twice. Slide it outwards and the two crossings meet; at that moment it is a tangent.
308
point of contactThe single point a tangent shares with the curve. It is where the two crossings of a secant have collapsed together.
309
the focus never moved
conic sectionThe curves a flat cut through a cone can produce. Tilt the cut further and one becomes the next.
310
0.76 + 5.24 = 6
3 + 3 = 6, the same total
ellipseThe distances to two fixed points always add to the same total. A loop of string round two pins draws one.
311
both foci lie on it
major axisThe longest way across, through both foci. Half of it is the number that fixes the total distance.
312
minor axisThe shortest way across, at right angles to the major axis. It decides how round or how flat the ellipse looks.
313
focus
focusA point the curve is defined in terms of rather than drawn around. Light from it reflects off the curve in a single direction.
314
one point, so a circle
fociTwo of them, for an ellipse and for a hyperbola. Slide them together and the ellipse becomes a circle.
315
the loop has just opened
two branches now
eccentricityOne number saying how far from circular the curve is. Zero is a circle, below one an ellipse, exactly one a parabola, above one a hyperbola.
316
focus
both 3.25, so e = 1
directrixA fixed line the curve is measured against. Distance to the focus divided by distance to this line is the eccentricity, at every point.
317
e = 0.9
e = 1, it never closes
parabola as a conicThe single case where the two distances are equal. It is the boundary between the closed curves and the open ones.
318
width 4, and 4a = 4
latus rectumThe chord through the focus, parallel to the directrix. It is a quick measure of how wide the curve opens.
319
hyperbolaThe distances to two fixed points always differ by the same amount. That gives two separate branches, one round each focus.
320
transverse axisThe line through both vertices and both foci. It is the direction the branches open away from.
321
nothing is drawn here
the branches spread faster
conjugate axisThe perpendicular direction, which the curve never crosses. Its length still sets how steeply the branches spread.
322
the gap has closed
asymptotes of a hyperbolaTwo crossing lines the branches settle onto. Far enough out, a hyperbola is indistinguishable from them.
323
a hyperbola with nothing left of it
degenerate conicWhat the cut gives when it passes through the tip of the cone: a single point, one line, or a crossing pair.
324
t = π/2
t = π
t = 2π
parametric equationx and y each given separately in terms of a third quantity. The curve becomes a journey rather than a condition.
325
t = 0.6
t = 1.2
t = 1.6about to land
parameterThe third quantity doing the driving, often standing for time. It appears in the working and not in the picture.
326
equal times, equal arcs
same circle, faster later
parametrisationA choice of how to travel along a curve. The same path can be walked at different speeds, and neither is more correct.
327
x = 2.5 cos t, y = 2.5 sin t
x² + y² = 6.25
eliminating the parameterGetting rid of t to leave a relation between x and y alone. What survives is the shape, with the timing thrown away.
328
r = 3
θ = 45°
polar coordinatesLocating a point by how far and in what direction, instead of by two sideways steps. Anything built around a centre is simpler this way.
329
pole
poleThe point everything is measured from, the polar version of the origin. Every direction starts here.
330
θ = 120°
polar axisThe ray angles are measured from, usually pointing right. It plays the part the positive x-axis plays elsewhere.
331
same direction, further out
radial coordinateThe distance out from the pole, written r. Changing it alone moves the point straight in or straight out.
332
the distance never changed
angular coordinateThe direction, written θ. Changing it alone swings the point round a circle of fixed size.
333
r = 3, θ = 30°
x = 2.6, y = 1.5
polar to Cartesian conversionx is r cos θ and y is r sin θ. It is one right-angled triangle, with the distance as its hypotenuse.
334
polar curveA rule giving the distance for each direction. Sweep the direction all the way round and the rule draws the shape.
335
the pole is on it now
circle in polar formA circle round the pole needs only r = a. One passing through the pole needs the angle, and comes out as r = 2a cos θ.
336
3 petals
8 petals
5 petals
rose curvePetals, from r = cos kθ. An odd k gives k petals, an even k gives twice as many, which surprises everyone the first time.
337
r = 0 at θ = 180°
cardioidA heart shape, from r = a(1 + cos θ). The distance drops to nothing at one direction, which makes the dimple.
338
a plain dimple
a cardioid, the boundary case
an inner loop
limaçonr = b + a cos θ. When b is smaller than a the distance goes negative for a while, and the curve tucks an inner loop inside itself.
339
the gaps stay equal
Archimedean spiralr = aθ, so the distance grows evenly with the angle. Every turn is the same width apart, unlike a shell.
340
nothing between them
lemniscateA figure eight, from r² = a² cos 2θ. It exists only where the right-hand side is positive, so two lobes appear and the rest is empty.
8

Data on the plane

41 concepts · 41 drawable

By the endFit a curve to measurements, and say how well it fits.

341
scatter plot
342
two numbers per case
bivariate data
343
the one you set
explanatory variable
344
the one you watch
response variable
345
trend
346
both rise together
positive correlation
347
one rises, one falls
negative correlation
348
no lean at all
no correlation
349
r near 1 means tight
correlation coefficient
350
leaning together is not causing
causation against correlation
351
line of best fit
352
these gaps, squared, made small
least squares
353
y = 0.6x
regression line
354
observed minus predicted
residual
355
no pattern left is good
residual plot
356
insidebetween the data
interpolation
357
outsidebeyond the data
extrapolation
358
outlier
outlier
359
one point drags the line
influential point
360
linear model
361
exponential model
362
power model
363
growth that levels off
logistic model
364
which shape suits?
curve fitting
365
how much is left over
goodness of fit
366
measured in order
time series
367
histogram
368
how many, not how much
frequency (of a value)
369
a running total
cumulative frequency
370
box plot
371
a quarter each side
quartile
372
half above, half below
median
373
the balance point
mean
374
the usual distance from the middle
standard deviation
375
normal curve
376
the chance is the area
area as probability
377
z = 1.5how many deviations out
z-score
378
height is density, not chance
probability density
379
the running total of chance
cumulative distribution
380
a few chosen from many
sampling
381
few points, unstable line
sample size
9

Change, and the bridge to limits

49 concepts · 47 drawable

By the endSay which two things were subtracted, and what was divided by what.

382
891011121314151617181920212223242526272829303132333430 − 12 = 18
difference
383
Δx and Δy
delta
384
−10123456789a step of 3
increment
385
−10123456789from 2 to 7
change
386
−101234567897 − 2, not 2 − 7
new minus old
387
Δy = +2.8
Δy = −2.8
signed change
388
4 over 5
rate
389
one across, 0.8 up
per unit
390
Δy ÷ Δx
rate of change
391
the steady rate that matches
average rate of change
392
secant line
393
rise over run again
slope of a secant
394
chord of a curve
395
−5−4−3−2−1012345from −1 to 3
interval
396
−5−4−3−2−1012345Δx = 4
width of an interval
397
[f(a+h) − f(a)] ÷ h
difference quotient
398
[ f(a + h) − f(a) ] ÷ hone endpoint, and a step of h
h notation
399
slope 1.75
slope 1.40
slope 1.05
slope 0.84
shrinking the interval
400
slope 1.75
slope 1.12
slope 0.80
slope 0.70
instantaneous rate
401
tangent line
402
the local steepness
slope of a tangent
403
touches here
point of tangency
404
crowding around 2
approaching a value
405
near the point, not at it
neighbourhood
406
as close as demanded
arbitrarily close
407
no value at x = 1
the limit is 2
limit
408
from below only
left-hand limit
409
from above only
right-hand limit
410
both sides agree
two-sided limit
411
both sides give 2
one side 0.5, the other 3
existence of a limit
412
the valuethey can disagree
limit against value
413
0 ÷ 0decides nothing on its own
indeterminate form
414
(x²−4)/(x−2)
(x−1)/(x²−1)
1/x at 0
zero over zero
415
(x² − 4) ÷ (x − 2)= (x−2)(x+2) ÷ (x−2)= x + 2, for every x but 2
factor and cancel
416
no break at all
continuity
417
value = limit
continuous at a point
418
unbroken throughout
continuous on an interval
419
discontinuity
420
one point missing
removable discontinuity
421
the sides disagree
jump discontinuity
422
no bound either side
infinite discontinuity
423
settles at 2
limit at infinity
424
asymptotic behaviour
425
trapped between two
squeeze theorem
426
it must cross
intermediate value theorem
427
a highest and a lowest
extreme value theorem
428
a tolerance on the output
epsilon
429
the input room it buys
delta (the tolerance)
430
for every ε there is a δ
epsilon-delta definition
10

Derivatives

63 concepts · 56 drawable

By the endMeasure how fast, at a point, and use it to find the best of something.

431
slope 1.75
slope 1.12
slope 0.84
f'(1) = 0.70
derivative
432
curve above, slopes below
differentiation
433
a tangent exists here
differentiable
434
f'(2) = 1.4
derivative at a point
435
a slope for every input
derivative as a function
436
f'(x)the slope rule of f
prime notation
437
dy / dxΔy/Δx with the interval shrunk
Leibniz notation
438
dy / dxnot a fraction, but it remembers being one
dy/dx
439
d/dx [ f(x) ]an instruction to differentiate
operator notation
440
no tangentunbroken, still not smooth
differentiability implies continuity
441
two candidate slopes
non-differentiable point
442
corner
corner
443
cusp
cusp
444
slope with no number
vertical tangent
445
xⁿ becomes n·xⁿ⁻¹
power rule
446
flat has no slope
constant rule
447
triple the rule, triple the slope
constant multiple rule
448
add the curves, add the slopes
sum rule
449
the same, subtracted
difference rule
450
uvu'vuv'u'v + uv'
product rule
451
(u/v)' = (u'v − uv') ÷ v²no picture; it is algebra
quotient rule
452
xuydu/dxdy/durates multiply along the chain
chain rule
453
( 4x + 1 )³innerouterwhat is done first, and last
outer and inner function
454
a tangent without solving for y
implicit differentiation
455
take logs, then differentiateturns products into sums
logarithmic differentiation
456
its own slope
derivative of an exponential
457
ln x gives 1/x
derivative of a logarithm
458
sine gives cosine
derivatives of sine and cosine
459
slopes are reciprocal
derivative of an inverse function
460
the slope of the slope
second derivative
461
differentiate again, and again
higher derivatives
462
switches herewhich way it bends
concavity
463
holds water
concave up
464
spills it
concave down
465
bending changes sides
point of inflection
466
f' = 0 or undefined
critical point
467
flat for an instant
stationary point
468
f' > 0
f' = 0
f' < 0
first derivative test
469
f'' > 0 means a minimum
second derivative test
470
f' > 0
increasing function
471
f' < 0
decreasing function
472
never turns back
monotonic
473
maxmin
local extremum
474
the highest
global extremum
475
still climbing
nearly there
f' = 0
optimisation
476
best allowedthe peak is out of bounds
constraint
477
dV/dt = dV/dr · dr/dtone rate drives another
related rates
478
position against time
displacement
479
the slope of position
velocity
480
velocity without its sign
speed
481
the slope of velocity
acceleration
482
the cost of one more
marginal cost
483
percentage change in oneper percentage change in the othera rate of relative changes
elasticity
484
near enough, near the point
tangent line approximation
485
indistinguishable
linearisation
486
dy along the tangent
differential
487
closing on √5
Newton's method
488
equal ends force a flat point
Rolle's theorem
489
some tangent matches the chord
mean value theorem
490
lim f/g = lim f′/g′when both go to zero together
L'Hopital's rule
491
hugging further out
Taylor polynomial
492
built at 0
Maclaurin series
493
useful only inside
radius of convergence
11

Integrals

61 concepts · 53 drawable

By the endAdd up a changing quantity, and know why that undoes a derivative.

  1. 494antiderivative
  2. 495indefinite integral
  3. 496constant of integration
  4. 497integrand
  5. 498integral sign
  6. 499variable of integration
  7. 500definite integral
  8. 501limits of integration
  9. 502area under a curve
  10. 503signed area
  11. 504net area
  12. 505Riemann sum
  13. 506left-hand sum
  14. 507right-hand sum
  15. 508midpoint sum
  16. 509upper sum
  17. 510lower sum
  18. 511partition
  19. 512subinterval
  20. 513norm of a partition
  21. 514limit of Riemann sums
  22. 515integrability
  23. 516trapezoidal rule
  24. 517Simpson's rule
  25. 518numerical integration
  26. 519fundamental theorem of calculus
  27. 520first fundamental theorem
  28. 521second fundamental theorem
  29. 522accumulation function
  30. 523net change theorem
  31. 524substitution
  32. 525u-substitution
  33. 526integration by parts
  34. 527partial fractions
  35. 528trigonometric substitution
  36. 529reduction formula
  37. 530improper integral
  38. 531convergent integral
  39. 532divergent integral
  40. 533area between two curves
  41. 534volume of revolution
  42. 535disc method
  43. 536washer method
  44. 537shell method
  45. 538cross-section method
  46. 539arc length
  47. 540surface of revolution
  48. 541average value of a function
  49. 542centroid of a region
  50. 543moment
  51. 544work
  52. 545fluid pressure
  53. 546consumer surplus
  54. 547separable differential equation
  55. 548slope field
  56. 549direction field
  57. 550initial condition
  58. 551particular solution
  59. 552Euler's method
  60. 553exponential growth model
  61. 554logistic growth model
12

Off the page: vectors and more dimensions

74 concepts · 72 drawable

By the endKeep the method when the plane runs out of room.

  1. 555three-dimensional space
  2. 556z-axis
  3. 557octant
  4. 558coordinate space
  5. 559right-handed system
  6. 560vector
  7. 561scalar
  8. 562magnitude
  9. 563direction
  10. 564component
  11. 565position vector
  12. 566unit vector
  13. 567zero vector
  14. 568vector addition
  15. 569scalar multiplication
  16. 570dot product
  17. 571scalar product
  18. 572cross product
  19. 573vector product
  20. 574projection
  21. 575angle between vectors
  22. 576orthogonality
  23. 577linear combination
  24. 578span
  25. 579basis
  26. 580linear independence
  27. 581matrix
  28. 582matrix transformation
  29. 583eigenvector
  30. 584eigenvalue
  31. 585line in space
  32. 586vector equation of a line
  33. 587parametric equations in space
  34. 588plane in space
  35. 589normal vector
  36. 590equation of a plane
  37. 591distance in three dimensions
  38. 592sphere
  39. 593cylinder
  40. 594cone
  41. 595quadric surface
  42. 596surface
  43. 597level curve
  44. 598contour
  45. 599contour map
  46. 600function of two variables
  47. 601partial derivative
  48. 602gradient vector
  49. 603directional derivative
  50. 604tangent plane
  51. 605critical point in 3D
  52. 606saddle point
  53. 607Lagrange multiplier
  54. 608double integral
  55. 609iterated integral
  56. 610region of integration
  57. 611order of integration
  58. 612Jacobian
  59. 613change of variables
  60. 614polar substitution
  61. 615cylindrical coordinates
  62. 616spherical coordinates
  63. 617triple integral
  64. 618vector field
  65. 619divergence
  66. 620curl
  67. 621line integral
  68. 622surface integral
  69. 623flux
  70. 624conservative field
  71. 625potential function
  72. 626Green's theorem
  73. 627Stokes' theorem
  74. 628divergence theorem
13

Where the picture stops working

53 concepts · 28 drawable

By the endSay when to stop trusting your eyes, and reach for a proof instead.

  1. 629counterexample
  2. 630pathological function
  3. 631Dirichlet function
  4. 632nowhere continuous
  5. 633Weierstrass function
  6. 634nowhere differentiable
  7. 635everywhere continuous
  8. 636fractal
  9. 637self-similarity
  10. 638Koch snowflake
  11. 639Cantor set
  12. 640Hausdorff dimension
  13. 641measure
  14. 642measure zero
  15. 643almost everywhere
  16. 644Riemann integrable
  17. 645Lebesgue integral
  18. 646non-integrable function
  19. 647elementary function
  20. 648non-elementary antiderivative
  21. 649Liouville's theorem
  22. 650error function
  23. 651sine integral
  24. 652elliptic integral
  25. 653closed form
  26. 654algebraic number
  27. 655transcendental number
  28. 656countable set
  29. 657uncountable set
  30. 658dense set
  31. 659nowhere dense
  32. 660completeness of the reals
  33. 661supremum
  34. 662infimum
  35. 663bounded sequence
  36. 664convergent sequence
  37. 665divergent sequence
  38. 666pointwise convergence
  39. 667uniform convergence
  40. 668rigour
  41. 669formal proof
  42. 670intuition against proof
  43. 671the limits of visualisation
  44. 672higher-dimensional intuition
  45. 673axiom
  46. 674definition
  47. 675theorem
  48. 676lemma
  49. 677corollary
  50. 678necessary and sufficient
  51. 679existence proof
  52. 680constructive proof
  53. 681proof by contradiction