Definite Integral as Area Under a Curve

⚡ Key Takeaways

The definite integral ∫abf(x) dx\int_a^b f(x)\,dx measures the signed area between the curve y=f(x)y=f(x) and the xx-axis from x=ax=a to x=bx=b. Key result: it is the limit of summing the areas of infinitely many thin rectangles under the curve. Applies to computing areas, accumulated quantities (distance, work, volume) wherever a rate is integrated. Origin: rigorously formalized by Bernhard Riemann (1854), building on Newton, Leibniz, Cauchy.

💡 The Core Insight

Slice the region under a curve into many thin vertical rectangles. Each has height f(xi)f(x_i) and width Δx\Delta x, so area f(xi) Δxf(x_i)\,\Delta x. Add them all up to estimate the total area. Then let the rectangles become infinitely thin (Δx→0\Delta x \to 0, number →∞\to \infty). The limit of these sums — if it exists — is the definite integral. The genius is that "infinitely many infinitely thin pieces" converges to a finite, exact answer.

Formal Statement

DefinitionRiemann Sum

Partition [a,b][a,b] into nn subintervals using points

1
a=x0<x1<x2<⋯<xn=b\quad a = x_0 < x_1 < x_2 < \cdots < x_n = b

Derivation hint: any increasing sequence of points starting at aa and ending at bb defines a valid partition. Let Δxi=xi−xi−1\Delta x_i = x_i - x_{i-1} be the width of subinterval ii, and choose a sample point xi∗∈[xi−1,xi]x_i^* \in [x_{i-1}, x_i]. The Riemann sum is

2
Sn=∑i=1nf(xi∗) Δxi\quad S_n = \sum_{i=1}^{n} f(x_i^*)\,\Delta x_i

Derivation hint: each term f(xi∗)Δxif(x_i^*)\Delta x_i is the area of one rectangle with height f(xi∗)f(x_i^*) and width Δxi\Delta x_i. For a regular partition (equal widths), Δx=b−an\Delta x = \dfrac{b-a}{n} and xi=a+i Δxx_i = a + i\,\Delta x, giving

3
Sn=∑i=1nf ⁣(a+i Δx) Δx,Δx=b−an\quad S_n = \sum_{i=1}^{n} f\!\left(a + i\,\Delta x\right)\,\Delta x, \qquad \Delta x = \frac{b-a}{n}

Derivation hint: substitute equal width Δx=(b−a)/n\Delta x=(b-a)/n into [2] and use xi=a+iΔxx_i = a + i\Delta x.

DefinitionThe Definite Integral

The definite integral of ff from aa to bb is the limit of Riemann sums as the largest subinterval width (the norm ∥P∥=max⁡iΔxi\|P\|=\max_i \Delta x_i) shrinks to zero:

4
∫abf(x) dx=lim⁡∥P∥→0∑i=1nf(xi∗) Δxi\quad \int_a^b f(x)\,dx = \lim_{\|P\|\to 0} \sum_{i=1}^{n} f(x_i^*)\,\Delta x_i

Derivation hint: the integral exists precisely when this limit gives the same value regardless of how partitions are refined or sample points chosen. Here aa is the lower limit, bb the upper limit, f(x)f(x) the integrand, xx the variable of integration, and dxdx the symbol indicating the infinitesimal width. The function ff is then called integrable on [a,b][a,b].

TheoremIntegrability of Continuous Functions

If ff is continuous on the closed interval [a,b][a,b], then ff is integrable on [a,b][a,b]; the limit in [4] exists and is a unique finite number. (More generally, a bounded function with only finitely many discontinuities is integrable.)

TheoremBasic Properties of the Definite Integral

For integrable functions f,gf,g and constants c,kc,k:

5
∫ab[ c f(x)+k g(x) ] dx=c∫abf(x) dx+k∫abg(x) dx\quad \int_a^b \big[\,c\,f(x) + k\,g(x)\,\big]\,dx = c\int_a^b f(x)\,dx + k\int_a^b g(x)\,dx

Derivation hint: linearity of the limit and of finite sums in [2] passes through to the integral.

6
∫abf(x) dx=∫acf(x) dx+∫cbf(x) dx,a≤c≤b\quad \int_a^b f(x)\,dx = \int_a^c f(x)\,dx + \int_c^b f(x)\,dx, \qquad a \le c \le b

Derivation hint: split each partition at the point cc; the two pieces' Riemann sums add to the whole.

7
∫aaf(x) dx=0,∫baf(x) dx=−∫abf(x) dx\quad \int_a^a f(x)\,dx = 0, \qquad \int_b^a f(x)\,dx = -\int_a^b f(x)\,dx

Derivation hint: zero-width interval gives zero area; reversing limits flips the sign of every Δx\Delta x.

Why It Holds / Derivation

ProofArea of a Region Equals the Limit of Rectangle Sums

We show that summing thin rectangles converges to the true area for a continuous, non-negative ff on [a,b][a,b].

Step 1 — Bound the area. On each subinterval [xi−1,xi][x_{i-1},x_i], since ff is continuous it attains a minimum mim_i and a maximum MiM_i. The true area AiA_i of the strip satisfies

8
mi Δx≤Ai≤Mi Δx\quad m_i\,\Delta x \le A_i \le M_i\,\Delta x

Derivation hint: the strip contains a rectangle of height mim_i and is contained in one of height MiM_i.

Step 2 — Form lower and upper sums. Summing over all strips:

9
Ln=∑i=1nmi Δx≤A≤∑i=1nMi Δx=Un\quad L_n = \sum_{i=1}^{n} m_i\,\Delta x \le A \le \sum_{i=1}^{n} M_i\,\Delta x = U_n

Derivation hint: add inequality [8] over i=1,…,ni=1,\dots,n; the middle sum telescopes to total area AA.

Step 3 — Squeeze the gap. The difference is

10
Un−Ln=∑i=1n(Mi−mi) Δx\quad U_n - L_n = \sum_{i=1}^{n} (M_i - m_i)\,\Delta x

Derivation hint: subtract LnL_n from UnU_n term by term. Because ff is continuous on a closed interval it is uniformly continuous, so for fine enough partitions each Mi−miM_i - m_i becomes arbitrarily small (less than any chosen ε\varepsilon). Then Un−Ln≤ε∑Δx=ε(b−a)→0U_n - L_n \le \varepsilon \sum \Delta x = \varepsilon(b-a) \to 0.

Step 4 — Conclude. Since Ln≤A≤UnL_n \le A \le U_n and Un−Ln→0U_n - L_n \to 0, both sums converge to the same limit, and any Riemann sum [2] (whose value lies between LnL_n and UnU_n) is squeezed to that limit. That common value is, by definition [4], ∫abf(x) dx=A\int_a^b f(x)\,dx = A. ■\blacksquare

∎
BR
Bernhard Riemann
1826–1866

The German mathematician Bernhard Riemann gave the integral its modern rigorous footing in his 1854 Habilitationsschrift "On the representation of a function by a trigonometric series." Earlier, Newton and Leibniz had used integration intuitively (1660s–80s), and Cauchy had defined the integral for continuous functions (1823); Riemann's contribution was a precise definition — the limit of sums in [4] — that worked even for discontinuous functions, with an exact criterion for when the limit exists. The construction is now universally called the Riemann integral. Riemann's broader genius spanned geometry (Riemannian manifolds, later the language of general relativity) and analysis (the Riemann zeta function), all before his death from tuberculosis at age 39.

Building Intuition

🧠 Intuition

Think of painting a region with vertical brushstrokes. Each stroke is a tall thin rectangle: its height is how far the curve sits above the axis at that spot, its width is how thick the brush is. A thick brush gives a rough, blocky estimate of the painted area; a thin brush traces the curve more faithfully. The integral is what you get in the imaginary limit of an infinitely thin brush — perfect fidelity. A second picture: imagine water flowing into a tank at a rate f(t)f(t) litres per second. Over a tiny time dtdt, the volume added is f(t) dtf(t)\,dt. The total water after time aa to bb is the sum of all those tiny contributions — exactly ∫abf(t) dt\int_a^b f(t)\,dt. This is why integrals appear everywhere a rate accumulates into a total: the "area under the rate curve" is the accumulated amount.

:::svg[Riemann rectangles approximating the area under y=f(x)y=f(x) on [a,b][a,b]] ```svg x y a b Δx y = f(x) Σ f(xᵢ)Δx ```

Worked Examples

ExampleArea under a parabola from the definition

Given: Compute ∫02x2 dx\displaystyle\int_0^2 x^2\,dx directly from the Riemann sum (regular partition, right endpoints).

Step 1 — Set up the partition. Δx=2−0n=2n\Delta x = \dfrac{2-0}{n} = \dfrac{2}{n}, and xi=0+iΔx=2inx_i = 0 + i\Delta x = \dfrac{2i}{n}.

Step 2 — Write the sum.

Sn=∑i=1n(2in)2⋅2n=8n3∑i=1ni2S_n = \sum_{i=1}^{n} \left(\frac{2i}{n}\right)^2 \cdot \frac{2}{n} = \frac{8}{n^3}\sum_{i=1}^{n} i^2

Step 3 — Use the sum-of-squares formula ∑i=1ni2=n(n+1)(2n+1)6\sum_{i=1}^n i^2 = \dfrac{n(n+1)(2n+1)}{6}:

Sn=8n3⋅n(n+1)(2n+1)6=8(n+1)(2n+1)6n2=43⋅(n+1)(2n+1)n2S_n = \frac{8}{n^3}\cdot \frac{n(n+1)(2n+1)}{6} = \frac{8(n+1)(2n+1)}{6n^2} = \frac{4}{3}\cdot\frac{(n+1)(2n+1)}{n^2}

Step 4 — Take the limit. As n→∞n\to\infty, (n+1)(2n+1)n2→2\dfrac{(n+1)(2n+1)}{n^2}\to 2:

∫02x2 dx=43⋅2=83\int_0^2 x^2\,dx = \frac{4}{3}\cdot 2 = \frac{8}{3}

Boxed answer: ∫02x2 dx=83≈2.667\displaystyle\int_0^2 x^2\,dx = \boxed{\dfrac{8}{3} \approx 2.667} (square units). Check via antiderivative: [x3/3]02=8/3[x^3/3]_0^2 = 8/3. ✓

ExampleSigned area and a real accumulation

Given: A particle moves with velocity v(t)=t−3v(t) = t - 3 metres per second for t∈[0,5]t\in[0,5] seconds. Find (a) the net displacement and (b) the total distance travelled.

Step 1 — Net displacement is the signed integral.

∫05(t−3) dt=[t22−3t]05=(252−15)−0=−2.5\int_0^5 (t-3)\,dt = \left[\frac{t^2}{2} - 3t\right]_0^5 = \left(\frac{25}{2} - 15\right) - 0 = -2.5

The negative sign means the particle ends up 2.5 m2.5\text{ m} behind its start.

Step 2 — Identify where vv changes sign. v=0v=0 at t=3t=3. On [0,3][0,3], v<0v<0 (moving backward); on [3,5][3,5], v>0v>0 (forward).

Step 3 — Total distance uses absolute values of each piece.

∫03(t−3) dt=[t22−3t]03=(4.5−9)=−4.5  ⇒  distance 4.5 m\int_0^3 (t-3)\,dt = \left[\tfrac{t^2}{2}-3t\right]_0^3 = (4.5-9) = -4.5 \;\Rightarrow\; \text{distance } 4.5\text{ m}
∫35(t−3) dt=[t22−3t]35=(12.5−15)−(4.5−9)=−2.5+4.5=2.0  ⇒  2.0 m\int_3^5 (t-3)\,dt = \left[\tfrac{t^2}{2}-3t\right]_3^5 = (12.5-15)-(4.5-9) = -2.5 + 4.5 = 2.0 \;\Rightarrow\; 2.0\text{ m}

Step 4 — Add the unsigned pieces. Total distance =4.5+2.0=6.5 m= 4.5 + 2.0 = 6.5\text{ m}.

Boxed answers: Net displacement =−2.5 m= \boxed{-2.5\text{ m}}, total distance =6.5 m= \boxed{6.5\text{ m}}.

Common Misconceptions

⚠️ Common mistake

"The integral always gives a positive area." False. The definite integral gives signed area: where f(x)<0f(x)<0, the rectangles have negative height and contribute negatively. To get the geometric (always-positive) area between the curve and the axis, you must integrate ∣f(x)∣|f(x)| — splitting the interval at every point where ff crosses the axis. Confusing ∫abf dx\int_a^b f\,dx with "geometric area" is the single most common error.

"dxdx is just decoration." No — dxdx records which variable you integrate and represents the infinitesimal width. It is essential for substitution, units, and reading the integral as a sum of f(x)⋅dxf(x)\cdot dx products. The integral ∫abf(x) dx\int_a^b f(x)\,dx carries units of [height]×[width].

Counterexample

Consider f(x)=sin⁡xf(x) = \sin x over [0,2π][0, 2\pi]. One might guess the "area under one full wave" is large and positive. But

∫02πsin⁡x dx=[−cos⁡x]02π=(−1)−(−1)=0.\int_0^{2\pi} \sin x\,dx = [-\cos x]_0^{2\pi} = (-1) - (-1) = 0.

The positive hump on [0,π][0,\pi] exactly cancels the negative trough on [π,2π][\pi,2\pi]. The signed area is zero, while the geometric area is ∫02π∣sin⁡x∣ dx=4\int_0^{2\pi}|\sin x|\,dx = 4. This vividly shows the integral is not "the area you see."

Connections

connection

The definite integral connects to a wide web of ideas. It is glued to differentiation by the Fundamental Theorem of Calculus, which says integration and differentiation are inverse operations — turning the hard limit of [4] into an easy antiderivative subtraction. The technique of finding those antiderivatives is the subject of Indefinite Integral and Antiderivatives. The Riemann sum [2] is a special case of the broader theory in Riemann Sums and Numerical Integration, where rules like the trapezoidal and Simpson's rule estimate integrals that have no closed form. Geometrically, the integral generalizes to Area Between Two Curves (integrate the difference of functions) and to Volumes of Revolution (integrate cross-sectional area). The limit concept underlying [4] is the same one studied in Limits and Continuity.

Real-World Applications

🔬 Where this appears

Historical Development

⏳ History
- c. 250 BCE — Archimedes: Computes the area of a parabolic segment by the method of exhaustion, summing inscribed triangles — a Riemann sum in spirit two millennia early.
- 1635 — Cavalieri: "Method of indivisibles" treats areas as sums of infinitely many line segments, a bold (if shaky) precursor.
- 1660s–1680s — Newton & Leibniz: Independently develop calculus; Leibniz introduces the elongated-S sign ∫\int (1675) for summa (sum) and the dxdx notation.
- 1820s — Cauchy: Gives the first rigorous definition of the integral for continuous functions as a limit of sums, anchoring it to limits rather than infinitesimals.
- 1854 — Riemann: Defines the integral via arbitrary partitions and sample points [4], with a precise integrability criterion; works for many discontinuous functions.
- 1875 — Darboux: Introduces upper and lower sums (our [9]), giving a clean equivalent formulation now standard in textbooks.
- 1902 — Lebesgue: Creates a more powerful integral by partitioning the range instead of the domain, integrating wildly discontinuous functions the Riemann integral cannot handle.
- 20th century: Numerical integration (trapezoidal, Simpson, Gaussian quadrature) and computer methods make definite integrals routinely computable in science and engineering.

Subtleties & Limits

open-problem

The Riemann integral, for all its power, has boundaries. The function that is 11 on rationals and 00 on irrationals (the Dirichlet function) is bounded yet not Riemann-integrable: its upper sums are always 11 and lower sums always 00, so the squeeze in [10] never closes. The Lebesgue integral repairs this — yet even Lebesgue integration cannot give finite, well-defined answers to many integrals arising in modern physics, such as the path integrals of quantum field theory, where the relevant "integral over all paths" still lacks a fully rigorous mathematical definition in the general case. Likewise, improper integrals over infinite intervals or with infinite integrands require careful limit definitions and may diverge (e.g. ∫1∞1x dx=∞\int_1^\infty \frac{1}{x}\,dx = \infty), forcing distinctions between conditional and absolute convergence that remain technically delicate. Defining "area" itself for sufficiently pathological sets connects to deep open questions in measure theory.

See Also

Fundamental Theorem of Calculus · Indefinite Integral and Antiderivatives · Riemann Sums and Numerical Integration · Area Between Two Curves · Improper Integrals · Limits and Continuity · Applications of Integration