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What is a Riemann Sum?
A Riemann sum approximates the area (definite integral) between a function f(x) and the x-axis as the sum of many small rectangles (or trapezoids). The interval [a, b] is divided into n pieces of width Δx = (b−a)/n, and depending on how the height of each piece is chosen, you get the left Riemann sum, right Riemann sum, midpoint Riemann sum, or trapezoidal rule. As n grows (finer subdivisions), the approximation converges to the true definite integral.