Area functions for linear functions Consider the following functions Ζ and real numbers a (see figure).
(a) Find and graph the area function A (π) = β«βΛ£ Ζ(t) dt .
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Ζ(t) = 4t + 2 , a = 0
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Area functions for linear functions Consider the following functions Ζ and real numbers a (see figure).
(a) Find and graph the area function A (π) = β«βΛ£ Ζ(t) dt .
<IMAGE>
Ζ(t) = 4t + 2 , a = 0
Bounds on an integral Suppose Ζ is continuous on [a, b] with Ζ''(π) > 0 on the interval. It can be shown that (bβa) Ζ [(a + b) /2] β€ β«βα΅ Ζ(π) dπ β€ (bβa) [ (Ζ(a) + Ζ(b)) /2]
(a) Assuming Ζ is nonnegative on [a, b], draw a figure to illustrate the geometric meaning of these inequalities. Discuss your conclusions. b.
Working with area functions Consider the function Ζ and its graph.
(a) Estimate the zeros of the area function A(π) = β«βΛ£ Ζ(t) dt , for 0 β€ π β€ 10 .
Area functions The graph of Ζ is shown in the figure. Let A(x) = β«ββΛ£ Ζ(t) dt and F(x) = β«βΛ£ Ζ(t) dt be two area functions for Ζ. Evaluate the following area functions.
(a) A (β2)
{Use of Tech} Midpoint Riemann sums with a calculator Consider the following definite integrals.
(a) Write the midpoint Riemann sum in sigma notation for an arbitrary value of n.
β«ββ΄ 2βπ dπ
Planetary orbits The planets orbit the Sun in elliptical orbits with the Sun at one focus (see Section 12.4 for more on ellipses). The equation of an ellipse whose dimensions are 2a in the π-direction and 2b in the y-direction is (πΒ²/aΒ²) + (yΒ² /bΒ²) = 1.
(a) Let dΒ² denote the square of the distance from a planet to the center of the ellipse at (0, 0). Integrate over the interval [ βa, a] to show that the average value of dΒ² is (aΒ² + 2bΒ²) /3 .