Approximate the area under the curve over the interval using the Midpoint Riemann sum with subintervals.
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8. Definite Integrals
Riemann Sums
Problem 5.2.32c
Textbook Question
{Use of Tech} Approximating definite integrals Complete the following steps for the given integral and the given value of n.
(c) Calculate the left and right Riemann sums for the given value of n.
β«βΒ² (πΒ²β2) dπ ; n = 4

1
Step 1: Understand the problem. You are tasked with approximating the definite integral β«βΒ² (πΒ²β2) dπ using left and right Riemann sums with n = 4 subintervals. Riemann sums approximate the area under a curve by summing the areas of rectangles.
Step 2: Divide the interval [0, 2] into n = 4 equal subintervals. The width of each subinterval, Ξπ, is calculated as Ξπ = (b - a) / n, where a = 0 and b = 2. Substitute the values to find Ξπ.
Step 3: For the left Riemann sum, use the left endpoints of each subinterval to evaluate the function f(π) = πΒ² - 2. The left endpoints are πβ = 0, πβ = Ξπ, πβ = 2Ξπ, and πβ = 3Ξπ. Compute f(π) at each left endpoint and multiply each value by Ξπ. Sum the results.
Step 4: For the right Riemann sum, use the right endpoints of each subinterval to evaluate the function f(π) = πΒ² - 2. The right endpoints are πβ = Ξπ, πβ = 2Ξπ, πβ = 3Ξπ, and πβ = 4Ξπ. Compute f(π) at each right endpoint and multiply each value by Ξπ. Sum the results.
Step 5: Compare the left and right Riemann sums to understand how the choice of endpoints affects the approximation of the integral. This comparison can provide insight into the accuracy of the method.

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Key Concepts
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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Introduction to Riemann Sums
Definite Integral
A definite integral represents the signed area under a curve defined by a function over a specific interval. It is denoted as β«βα΅ f(x) dx, where 'a' and 'b' are the limits of integration. The definite integral can be interpreted both geometrically, as the area between the curve and the x-axis, and analytically, as the limit of Riemann sums as the number of subdivisions approaches infinity.
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Definition of the Definite Integral
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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Introduction to Riemann Sums
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