Understanding Definite Integrals and Riemann Sums
This page introduces the concept of definite integrals and their relationship to Riemann sums. It provides a comprehensive overview of the mathematical foundations and practical applications of these crucial calculus concepts.
Definition: A definite integral of a bounded function f: [a,b] → R is defined as the limit of Riemann sums as the partition of the interval becomes infinitely fine.
The definite integral is formally expressed as:
∫[a to b] f(x) dx = lim[n→∞] Σ[i=1 to n] f(ξᵢ)(xᵢ - xᵢ₋₁)
Where P is a partition of the interval [a,b], and ξᵢ are sample points in each subinterval.
Highlight: The definite integral represents the area under the curve of f(x) bounded by the lines x=a, x=b, y=0, and the graph of f(x).
The page also introduces the concept of Suma Riemanna (Riemann sum), which is a finite approximation of the definite integral. The Riemann sum is given by:
S(P) = Σ[i=1 to n] f(ξᵢ)(xᵢ - xᵢ₋₁)
Vocabulary: The diameter of a partition, denoted as δ(P), is the maximum width of any subinterval in the partition.
The fundamental theorem of calculus is presented, stating that if f(x) is continuous, then it is integrable, and:
∫[a to b] f(x) dx = F(b) - F(a)
Where F(x) is any antiderivative of f(x).
Example: The definite integral ∫[a to b] c dx = c(b-a), where c is a constant.
The page concludes by listing several important properties of definite integrals, including additivity with respect to the interval and linearity.