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Ch. 8 - Integration Techniques
Briggs - Calculus: Early Transcendentals 3rd Edition
Briggs3rd EditionCalculus: Early TranscendentalsISBN: 9780136847243Not the one you use?Change textbook
Chapter 8, Problem 8.5.94c

94. [Use of Tech] Skydiving A skydiver has a downward velocity given by v(t) = V_T [(1 - e^(-2gt/V_T))/(1 + e^(-2gt/V_T))],
where t = 0 is the instant the skydiver starts falling, g = 9.8 m/s² is the acceleration due to gravity, and V_T is the terminal velocity of the skydiver.
c. Verify by integration that the position function is given by
s(t) = V_T t + (V_T²/g) ln[(1 + e^(-2gt/V_T))/2],
where s'(t) = v(t) and s(0) = 0.

Verified step by step guidance
1
Start with the given velocity function: \(v(t) = V_T \left( \frac{1 - e^{-\frac{2gt}{V_T}}}{1 + e^{-\frac{2gt}{V_T}}} \right)\). Since velocity is the derivative of position, we have \(s'(t) = v(t)\), so to find \(s(t)\), integrate \(v(t)\) with respect to \(t\).
Rewrite the velocity function to simplify the integral. Notice that \(\frac{1 - e^{-x}}{1 + e^{-x}} = \tanh\left( \frac{x}{2} \right)\), where \(x = \frac{2gt}{V_T}\). So, \(v(t) = V_T \tanh\left( \frac{gt}{V_T} \right)\). This substitution makes the integral more straightforward.
Set up the integral for position: \(s(t) = \int v(t) \, dt = \int V_T \tanh\left( \frac{gt}{V_T} \right) dt\). Since \(V_T\) is constant, factor it out: \(s(t) = V_T \int \tanh\left( \frac{gt}{V_T} \right) dt\).
Use substitution to integrate: Let \(u = \frac{gt}{V_T}\), so \(du = \frac{g}{V_T} dt\) or \(dt = \frac{V_T}{g} du\). Rewrite the integral: \(s(t) = V_T \int \tanh(u) \cdot \frac{V_T}{g} du = \frac{V_T^2}{g} \int \tanh(u) du\).
Recall the integral of hyperbolic tangent: \(\int \tanh(u) du = \ln(\cosh(u)) + C\). Therefore, \(s(t) = \frac{V_T^2}{g} \ln(\cosh(u)) + C = \frac{V_T^2}{g} \ln\left( \cosh\left( \frac{gt}{V_T} \right) \right) + C\). Use the initial condition \(s(0) = 0\) to solve for \(C\) and express \(\cosh\) in terms of exponentials to match the given formula.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Relationship Between Velocity and Position via Integration

Velocity is the derivative of position with respect to time. To find the position function s(t) from a given velocity v(t), you integrate v(t) with respect to time. The constant of integration is determined using initial conditions, such as s(0) = 0 in this problem.
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Integration of Exponential Functions

The velocity function involves exponential terms of the form e^(-2gt/V_T). Integrating such functions requires understanding how to handle exponentials and logarithms, often using substitution methods to simplify the integral into a form involving natural logarithms.
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Initial Conditions and Determining Constants of Integration

When integrating to find position, an arbitrary constant appears. Applying the initial condition s(0) = 0 allows you to solve for this constant, ensuring the position function accurately reflects the physical scenario starting at zero displacement.
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Related Practice
Textbook Question

45–48. {Use of Tech} Trapezoid Rule and Simpson’s Rule Consider the following integrals and the given values of n.

46. ∫(0 to 2) x⁴ dx; n = 30

c. Compute the absolute errors in the Trapezoid Rule and Simpson’s Rule with 2n subintervals.

Textbook Question

109. Escape velocity and black holes The work required to launch an object from the surface of Earth to outer space is given by W = ∫ from R to ∞ of F(x) dx, where R = 6370 km is the approximate radius of Earth, F(x) = (GMm)/x² is the gravitational force between Earth and the object, G is the gravitational constant, M is the mass of Earth, m is the mass of the object, and GM = 4 × 10¹⁴ m³/s².

c. The French scientist Laplace anticipated the existence of black holes in the 18th century with the following argument: If a body has an escape velocity that equals or exceeds the speed of light, c = 300,000 km/s, then light cannot escape the body and it cannot be seen. Show that such a body has a radius R ≤ 2GM/c². For Earth to be a black hole, what would its radius need to be?

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Textbook Question

Prove the following orthogonality relations (which are used to generate Fourier series). Assume m and n are integers with m ≠ n.

c.

π

∫ sin(mx) cos(nx) dx = 0, when |m + n| is even

0

Textbook Question

3. What term(s) should appear in the partial fraction decomposition of a proper rational function with each of the following?

c. A factor of (x² + 2x + 6) in the denominator

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Textbook Question

60. Two Methods

c. Verify that your answers to parts (a) and (b) are consistent.

Textbook Question

91. [Use of Tech] Regions bounded by exponentials Let a > 0 and let R be the region bounded by the graph of y = e^(-a·x) and the x-axis

on the interval [b, ∞).

c. Find the minimum value b* such that when b > b*, there exists some a > 0 where A(a,b) = 2.