Before you can read a single line of the parent proofs, you must own every symbol they use. Below, each piece is built from nothing, drawn as a picture, and justified. Read top to bottom — each rung of the ladder rests on the one below it.
Everything we do sits on this road. When we "add up numbers," we are collecting a handful of these marks and asking for their total. Look at the figure: the coloured dots are the numbers 1,2,3,4 — the very things we will soon be summing.
Why the topic needs it: every symbol below is ultimately a position on this line. If you can point to a number, you can add it.
Why we need it: to describe "add up the first few numbers" without writing them all out, we need a way to say "the number in position k." That is the entire job of k.
Other common index letters are i,j,m — same idea, different letter. Choose any letter — meaning is the same.
This is the star of the whole topic, so we build it slowly.
Look at the figure: the big Σ is a machine. You feed in a rule (here, "k"), the spotlight walks from the bottom number to the top number, and at each stop it drops a term into a bucket. At the end the bucket's total is the answer.
Why the topic needs it:Σ is shorthand. Writing 1+2+⋯+1000 is painful; ∑k=11000k says the same thing in one breath — and is the object we will find a shortcut for.
Why we need it: the four headline sums are ∑1 (power 0), ∑k (power 1), ∑k2 (power 2), ∑k3 (power 3). Powers are the ingredient list of the whole chapter.
This is the one rule of manipulation every proof leans on.
Why the topic needs it: every proof mixes k2,k,1 together on one side. Linearity lets us separate them so we can substitute the shorter formulas we already know.
Why we need it: the master trick (telescoping) is stated as "pick a rule f whose difference is the term you want." We literally cannot say that sentence without the symbol f(k).
Look at the figure: the arrows show each + meeting its matching −; watch them vanish until only the two endpoints are left standing.
Why the topic needs it: this single collapse is the engine behind all four formula proofs. You choose f cleverly (e.g. f(k)=k3) so that its difference contains the power you want (k2), sum both sides, and the left collapses to just two terms.
Why we need it: the differences we telescope, like (k+1)3−k3, must be expanded before the k2 term becomes visible. This connects to Binomial Theorem, the general machine for expanding (k+1)p.