Here are the essential concepts you must grasp in order to answer the question correctly.
Riemann Sums
Riemann sums are a method for approximating the value of a definite integral by dividing the area under a curve into smaller rectangles. The sum of the areas of these rectangles provides an estimate of the integral's value. Depending on whether the left or right endpoints of the subintervals are used, the sums can yield different approximations, which converge to the actual integral as the number of rectangles increases.
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Definite Integral
A definite integral represents the signed area under a curve between two specified limits, often denoted as β«βα΅ f(x) dx. It quantifies the accumulation of quantities, such as area, over an interval [a, b]. The Fundamental Theorem of Calculus connects differentiation and integration, stating that the definite integral can be evaluated using the antiderivative of the function.
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Subintervals and n
In the context of Riemann sums, 'n' refers to the number of subintervals into which the interval of integration is divided. Each subinterval has a width of Ξx, calculated as (b - a)/n. The choice of n affects the accuracy of the approximation; a larger n results in narrower rectangles and a more precise estimate of the integral, while a smaller n may lead to greater error.
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