The Power Rule (y = x^n)
Drop a ball and the distance it has fallen grows with the square of the time; a widening
ripple's area, an inflating balloon's volume, a savings pot left to grow all follow powers
too. To find how fast any of them is changing you need the slope of a power — and this page
turns that into a one-step rule.
You have earned this page. Four times now you've fed a function into the difference
quotient, expanded, cancelled the stubborn h, and taken a limit —
once for a constant, once for x, once for
x^2, once for x^3. Each answer took a
page of algebra. Now line the four answers up side by side, and watch them confess:
\frac{d}{dx}[1] = 0 \qquad \frac{d}{dx}[x] = 1 \qquad \frac{d}{dx}[x^2] = 2x \qquad \frac{d}{dx}[x^3] = 3x^2
Look at what happens to the exponent as you climb the ladder. Reading
x^0,
x^1,
x^2,
x^3,
each derivative brings the old power down to the front as a multiplier and
drops the power by one. Once for a square (2x^1),
once for a cube (3x^2) — and if you dared to guess the next rung,
you'd write x^4 \to 4x^3. You'd be right. The rung after that?
5x^4. Right again. The pattern you discovered one power at a time
holds for every power, and today it finally gets its name: the
power rule.
You can watch the degree fall. Here is y = x^3 with its first
three derivatives — a cubic (y), then a parabola
(y'), then a line (y''), then a flat
constant (y'''). Each curve sits one whole degree lower than the
one before it, exactly as "drop the power by one" predicts. Those prime marks are the
prime notation
you met earlier — shorthand for "the derivative, then its derivative, and so on".
And, just for fun, differentiation flattens more than curves. Here's what four derivatives
do to a smile:
\tfrac{d}{dx} 🙂 = 🫤
\tfrac{d}{dx} 🫤 = 😐
\tfrac{d}{dx} 😐 = 😮
\tfrac{d}{dx} 😮 = 😵
The pattern, stated once and for all
Here it is — the single most-used fact in all of differential calculus:
-
For any real number n,
\frac{d}{dx}\bigl[\,x^n\,\bigr] = n\,x^{\,n-1}.
-
In words: bring the power down to the front as a multiplier, then
subtract one from the power.
-
n need not be a whole number — the rule holds for negative
powers (x^{-2}), fractional powers
(x^{1/2}), even irrational powers
(x^{\pi}), wherever the function is defined.
Check it against the ladder you built by hand:
x^3 \to 3x^2 (✓), x^2 \to 2x^1 = 2x
(✓), x^1 \to 1\cdot x^0 = 1 (✓), and even
x^0 \to 0\cdot x^{-1} = 0 (✓) — the constant rule falls right
out as the bottom rung. Four hard-won theorems have just become four easy special cases of
one line.
Appreciate what you're being handed here. Every derivative so far cost you a difference
quotient, an expansion, a cancellation and a limit. From this point on, for any power of
x, the whole ritual collapses into a two-second stencil:
power down, power drops. The limits haven't vanished — they're baked in, done once
in general so you never have to do them again. That's what a rule is:
a limit argument, pre-paid.
Worked examples: no limits required
Example 1 — f(x) = x^5. The old way would demand
expanding (x+h)^5 — six terms, five minutes, three chances to
drop a coefficient. The new way: the power is 5, so bring the
5 down and knock the exponent to 4:
f'(x) = 5x^4.
Done. Example 2 — g(x) = x^{10}. Power down,
power drops:
g'(x) = 10x^9.
Example 3 — evaluate a slope. How steep is y = x^5
at x = 2? Differentiate first, substitute second:
y' = 5x^4, so the slope there is
5 \cdot 2^4 = 5 \cdot 16 = 80. The tangent at
(2, 32) rises eighty units for every one across — that's how
savagely a fifth power grows.
And the party trick: \tfrac{d}{dx}[x^{100}] = 100x^{99}, written
faster than you can say "difference quotient". A century of powers, one second of work.
Try every power at once
A rule that claims to work for every n deserves to be
stress-tested. Slide n and watch the curve
x^n (solid) next to its derivative
n\,x^{n-1} (dashed). Two things to hunt for as you slide:
the dashed curve always sits one degree lower than the solid one — a
quartic's derivative is a cubic, a cubic's is a parabola — and wherever the solid curve is
momentarily flat, the dashed curve crosses zero at exactly
that x. The derivative isn't just a formula that resembles the
function; it's a running commentary on the function's slope, point by point.
Try n = 2 versus n = 3 and look at
the dashed curves. For x^2 the derivative
2x is negative on the left — the parabola runs downhill there.
For x^3 the derivative 3x^2 never
dips below zero — a cubic climbs on both sides, pausing flat only for an instant at the
origin.
The derivative is the slope
One more sanity check before we push the rule somewhere new. Here's
y = x^3 (solid) with the straight tangent line that just grazes
it (dashed). The power rule promises the slope at x = a is
3a^2. Slide a along the curve and
test the promise: at a = 1 the tangent should climb with slope
3; at a = 2 a steep
12; at a = -1, slope
3 again — because 3a^2 can't be
negative, the cubic leans uphill on both sides. And at
a = 0 the tangent lies perfectly flat along the axis.
Why it works: the binomial theorem's opening move
A pattern spotted four times isn't a proof — maybe the fifth power breaks it? Here's the
sketch that settles every power at once, and it's just the general version of the cube
picture from the
x^3 page. Expand
(x + h)^n with the
binomial
expansion. You only need to look at its first two terms:
(x + h)^n = x^n + n\,x^{n-1}h + (\text{terms with } h^2, h^3, \ldots)
Read it geometrically, the way you read the cube: an n-dimensional
"cube" of side x grows by a whisker h.
The new volume is the old x^n, plus n
thin slabs — one glued to each of the n faces, each of size
x^{n-1} h — plus crumbs in the corners, all of them carrying
h^2 or worse. Now run the difference quotient:
\frac{(x+h)^n - x^n}{h} = \frac{n\,x^{n-1}h + (\text{terms with } h^2, \ldots)}{h} = n\,x^{n-1} + (\text{terms still carrying } h).
The x^ns cancel, one h cancels, and
everything left over still holds at least one factor of h — so
as h \to 0, the crumbs melt away and only the slabs survive:
\frac{d}{dx}\bigl[x^n\bigr] = \lim_{h \to 0}\Bigl(n\,x^{n-1} + \cdots\Bigr) = n\,x^{n-1}.
That's where both halves of the stencil come from. The n out
front counts the n faces of the growing cube; the
x^{n-1} is the area of each face. The rule isn't a coincidence
you memorise — it's geometry you can picture.
The twist: it isn't just for whole numbers
Here's the part nobody would dare guess from the ladder. The rule keeps working when
n is negative or a fraction —
you just have to rewrite the function as a power first. This
rewrite-then-differentiate move is where most exam marks in this topic live, so watch both
classics in slow motion.
Rewrite 1 — reciprocals are negative powers. Since
\tfrac{1}{x^2} = x^{-2}, the power rule applies with
n = -2: bring the -2 down, then drop
the exponent by one — from -2 down to -3:
\frac{d}{dx}\!\left[\frac{1}{x^2}\right] = \frac{d}{dx}\bigl[x^{-2}\bigr] = -2\,x^{-3} = -\frac{2}{x^3}.
The minus sign is not an accident — it's information. 1/x^2 is a
falling function (for x > 0, bigger input means smaller
output), so its slope must come out negative. The simplest case works the same way:
\tfrac{1}{x} = x^{-1} \Rightarrow -1 \cdot x^{-2} = -\tfrac{1}{x^2}.
Rewrite 2 — roots are fractional powers. Since
\sqrt{x} = x^{1/2}, apply the rule with
n = \tfrac12. Down comes the half; the exponent drops from
\tfrac12 to \tfrac12 - 1 = -\tfrac12:
\frac{d}{dx}\bigl[\sqrt{x}\bigr] = \frac{d}{dx}\bigl[x^{1/2}\bigr] = \tfrac{1}{2}\,x^{-1/2} = \frac{1}{2\sqrt{x}}.
Same recipe every time: rewrite as a power, power to the front, drop it by one —
and then, usually, rewrite back into root-or-fraction form for the final answer. Here's the
square root with its derivative. Watch how \tfrac{1}{2\sqrt{x}}
behaves at the two ends: near x = 0 it blows up — the root curve
launches almost vertically — while far to the right it sinks toward zero, because
\sqrt{x} keeps rising but ever more lazily.
A small dictionary of disguised powers worth carrying into any exam:
\tfrac{1}{x} = x^{-1},
\tfrac{1}{x^3} = x^{-3},
\sqrt{x} = x^{1/2},
\sqrt[3]{x} = x^{1/3},
\tfrac{1}{\sqrt{x}} = x^{-1/2}, and
x\sqrt{x} = x^{3/2}. Translate first; differentiate second.
Three traps claim more marks on this topic than all others combined:
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The rule is for x^n — a variable raised to a fixed
power. It does not apply to n^x, where the
variable sits in the exponent: \tfrac{d}{dx}[2^x] is
absolutely not x \cdot 2^{x-1}. Ask yourself where the
x lives: in the base, power rule; in the exponent, that's
an exponential
function — a different beast with its own rule, coming later.
-
Don't drop the sign on negative powers. Differentiating
x^{-2} gives -2x^{-3} — the
exponent goes down, from -2 to
-3, more negative, and the coefficient keeps its minus. Writing
-2x^{-1} (subtracting the wrong way) or
2x^{-3} (losing the sign) are the two classic wrecks.
-
Fractional powers: subtract one, honestly. From
n = \tfrac12 the new exponent is
\tfrac12 - 1 = -\tfrac12 — not
\tfrac12 again, and not -1. If your
derivative of \sqrt{x} doesn't end up with a root in the
denominator, the subtraction went wrong.
The rule says \tfrac{d}{dx}[x^{\pi}] = \pi\,x^{\pi - 1} — but
hold on, what does x^{\pi} even mean? You can't
multiply x by itself \pi times.
Humanity needed centuries to stretch the word "power" this far. Around 1350, Nicole Oresme
toyed with fractional exponents; in the 1650s John Wallis made negative and fractional
powers respectable; and in 1676 Isaac Newton — writing to Leibniz, of all people — treated
exponents like \tfrac12 and -1 as
entirely ordinary citizens, extending the binomial theorem to them. Each extension was
chosen so the old rules of exponents (x^a x^b = x^{a+b})
survived unbroken.
Irrational powers came last: x^{\pi} is defined by squeezing —
it's the value trapped between x^{3.14},
x^{3.141}, x^{3.1415}, \ldots as the
exponents close in on \pi (a limit again — they're everywhere).
And the miracle: after all that stretching, the power rule never flinches. For every real
n, rational or not, the derivative is still
n\,x^{n-1}. A pattern you spotted in four whole-number examples
turns out to govern a continuum.