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Consider the motion of a particle of mass in falling vertically under the earth's gravitational field, and suppose the downward motion is opposed by a frictional force \(p(v)\) dependent on the velocity \(v(t)\) of the particle. Then the velocity satisfies the equation $$ m v^{\prime}(t)=-m g+p(v), \quad t \geq 0, \quad v(0) \text { given } $$ Let \(m=1 \mathrm{~kg}, g=9.8 \mathrm{~m} / \mathrm{sec}^{2}\), and \(v(0)=0\). Solve the differential equation for \(0 \leq t \leq 20\) and for the following choices of \(p(v)\) : (a) \(p(v)=-0.1 v\), which is positive for a falling body. (b) \(\quad p(v)=0.1 v^{2}\). Find answers to at least three digits of accuracy. Graph the functions \(v(t) .\) Compare the solutions.

Short Answer

Expert verified
For (a), the solution is \( v(t) = -98 + 98e^{-0.1t} \). For (b), the solution is \( v(t) = \sqrt{980e^{\frac{t}{10}} - 980} \). Plot and compare both.

Step by step solution

01

Understanding the Differential Equation

Given the differential equation for the particle's velocity: \[ m v^{\prime}(t) = -m g + p(v) \] with initial conditions: \[ m = 1 \text{ kg}, \ g = 9.8 \text{ m/sec}^2, \ v(0) = 0 \] It can be simplified as: \[ v^{\prime}(t) = -9.8 + p(v) \]
02

Case (a) Solve for p(v) = -0.1v

Substitute \( p(v) = -0.1v \) into the simplified differential equation: \[ v^{\prime}(t) = -9.8 - 0.1v \] This is a first-order linear differential equation. To solve it, use the integrating factor method. The standard form is: \[ v^{\prime} + 0.1v = -9.8 \] The integrating factor \( \mu(t) \) is: \[ \mu(t) = e^{\int 0.1 dt} = e^{0.1t} \] Multiplying through by the integrating factor gives: \[ e^{0.1t} v^{\prime} + 0.1 e^{0.1t} v = -9.8 e^{0.1t} \] The left side is the derivative of \( e^{0.1t} v \), so: \[ \frac{d}{dt} (e^{0.1t} v) = -9.8 e^{0.1t} \] Integrate both sides: \[ e^{0.1t} v = -9.8 \int e^{0.1t} dt = -9.8 \frac{e^{0.1t}}{0.1} + C = -98 e^{0.1t} + C \] Solve for \( v \): \[ v(t) = -98 + Ce^{-0.1t} \] Using the initial condition \( v(0) = 0 \), solve for \( C \): \[ 0 = -98 + C \implies C = 98 \] Thus, the solution is: \[ v(t) = -98 + 98e^{-0.1t} \]
03

Case (b) Solve for p(v) = 0.1v^2

Substitute \( p(v) = 0.1v^2 \) into the simplified differential equation: \[ v^{\prime}(t) = -9.8 + 0.1v^2 \] This is a nonlinear differential equation and can be solved using separation of variables. Write it in separable form: \[ \frac{dv}{-9.8 + 0.1v^2} = dt \] Integrate both sides. Let \( v^2 = \frac{u}{0.1} = 10u \), so \( dv = \frac{du}{10v} \): \[ \int \frac{10}{-9.8 + u} du = \int dt \] Solving the integrals, we get: \[ 10 \int \frac{1}{-9.8 + u} du = t + C \] The left integral is: \[ 10 \ln| -9.8 + u | = t + C \] Reverting back to \( v \): \[ 10 \ln| -9.8 + 0.1v^2 | = t + C \] Exponentiating both sides: \[ -9.8 + 0.1v^2 = e^{\frac{t}{10} + C} = Ae^{\frac{t}{10}} \] Solving for \( v \): \[ 0.1v^2 = -9.8 + Ae^{\frac{t}{10}} \implies v(t) = \sqrt{10(Ae^{\frac{t}{10}} - 98)} \] Using the initial condition \( v(0) = 0 \) to find \( A \): \[ 0 = \sqrt{10(A - 98)} \implies A = 98 \] Thus, the solution is: \[ v(t) = \sqrt{10(98e^{\frac{t}{10}} - 98)} = \sqrt{980e^{\frac{t}{10}} - 980} \]
04

Graph the Functions and Compare Solutions

Plot the functions \( v(t) = -98 + 98e^{-0.1t} \) and \( v(t) = \sqrt{980e^{\frac{t}{10}} - 980} \) for \( 0 \leq t \leq 20 \). Comparing both solutions, observe the decay behavior in the first case (a) and the nonlinear growth in the second case (b).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Gravitational Motion
Gravitational motion describes the movement of objects under the influence of gravity. For a particle falling towards Earth, gravity is the primary force acting on it. The gravitational force on a particle of mass is given by Newton's law of universal gravitation, simplified as: \[ F = mg \] where:
  • \(F\) is the force due to gravity,
  • \(m\) is the mass of the particle, and
  • \(g\) is the acceleration due to gravity (approximately \(9.8 \, \text{m/s}^{2}\) near the Earth's surface).
In this exercise, the motion is also influenced by friction, which is a resistive force dependent on the particle's velocity. The falling particle's downward velocity thus satisfies a differential equation that accounts for both gravitational pull and frictional resistance.
First-Order Linear Differential Equations
A first-order linear differential equation has the general form: \[ \frac{dv}{dt} + P(t)v = Q(t) \] where \(P(t)\) and \(Q(t)\) are given functions of \(t\). In this particular problem, when \(p(v) = -0.1v\), the differential equation becomes: \[ \frac{dv}{dt} = -9.8 - 0.1v \] Rewriting in the standard form: \[ \frac{dv}{dt} + 0.1v = -9.8 \] This format is suitable for solving using methods such as the integrating factor method, which helps in finding the general solution to these kinds of equations efficiently.
Nonlinear Differential Equations
Nonlinear differential equations contain terms that are non-linear with respect to the unknown function or its derivatives. In the given exercise, when \(p(v) = 0.1v^2\), the equation becomes: \[ \frac{dv}{dt} = -9.8 + 0.1v^2 \] This is a nonlinear differential equation. Solving nonlinear differential equations often requires different methods compared to linear ones, like separation of variables, which helps isolate the terms involving the unknown function. Nonlinear equations can exhibit more complex behavior and solutions compared to their linear counterparts.
Integrating Factor Method
The integrating factor method is a technique used to solve first-order linear differential equations. The idea is to multiply the differential equation by an integrating factor, which simplifies the equation into an easily integrable form. For the equation: \[ \frac{dv}{dt} + 0.1 v = -9.8 \] The integrating factor \( \mu(t) \) is calculated as: \[ \mu(t) = e^{\int 0.1 dt} = e^{0.1t} \] Multiplying both sides of the equation by \( \mu(t) \) transforms it into: \[ \frac{d}{dt} (e^{0.1t} v) = -9.8 e^{0.1t} \] Now the equation can be integrated easily, allowing us to solve for \(v(t)\).
Separation of Variables
Separation of variables is a method for solving differential equations by separating the variables (unknown function and its derivative) on different sides of the equation. For the nonlinear equation: \[ \frac{dv}{dt} = -9.8 + 0.1v^2 \] We rewrite it in a separable form: \[ \frac{dv}{-9.8 + 0.1v^2} = dt \] Then, both sides of the equation can be integrated individually. This technique helps in tackling the complexity of nonlinear differential equations and finding their solutions by breaking down the problem into simpler integrable parts. Keeping track of integrating limits and initial conditions is crucial for finding the appropriate constant and thus the exact solution.

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Most popular questions from this chapter

Consider the initial value problem $$ Y^{\prime}(x)=\alpha x^{\alpha-1}, \quad Y(0)=0 $$ where \(\alpha>0\). The true solution is \(Y(x)=x^{\alpha}\). When \(\alpha \neq\) integer, the true solution is not infinitely differentiable. In particular, to have \(Y\) twice continuously differentiable, we need \(\alpha>2\). Use the Euler method to solve the initial value problem for \(\alpha=2.5,1.5,1.1\) with stepsize \(h=0.2,0.1,0.05\). Compute the solution errors at the nodes, and determine numerically the convergence orders of the Euler method for these problems.

Convert the following system of second-order equations to a larger system of firstorder equations. It arises from studying the gravitational attraction of one mass by another. $$ x^{\prime \prime}(t)=\frac{-c x(t)}{r(t)^{3}}, \quad y^{\prime \prime}(t)=\frac{-c y(t)}{r(t)^{3}}, \quad z^{\prime \prime}(t)=\frac{-c z(t)}{r(t)^{3}} $$ with \(c\) positive constant and \(r(t)=\left[x(t)^{2}+y(t)^{2}+z(t)^{2}\right]^{1 / 2}, t=\) time.

Consider the differential equation $$ Y^{\prime}(x)=f_{1}(x) f_{2}(Y(x)) $$ for some given functions \(f_{1}(x)\) and \(f_{2}(z) .\) This is called a separable differential equation, and it can be solved by direct integration. Write the equation as $$ \frac{Y^{\prime}(x)}{f_{2}(Y(x))}=f_{1}(x) $$ and find the antiderivative of each side: $$ \int \frac{Y^{\prime}(x) d x}{f_{2}(Y(x))}=\int f_{1}(x) d x $$ On the left side, change the integration variable by letting \(z=Y(x)\). Then the equation becomes $$ \int \frac{d z}{f_{2}(z)}=\int f_{1}(x) d x $$ After integrating, replace \(z\) by \(Y(x)\); then solve for \(Y(x)\), if possible. If these integrals can be evaluated, then the differential equation can be solved. Do so for the following problems, finding the general solution and the solution satisfying the given initial condition: \(\begin{array}{ll}\text { (a) } Y^{\prime}(x)=x / Y(x), & Y(0)=2\end{array}\) (b) \(Y^{\prime}(x)=x e^{-Y(x)}, \quad Y(1)=0\) (c) \(\quad Y^{\prime}(x)=Y(x)[a-Y(x)], \quad Y(0)=a / 2, \quad a>0\)

Solve the equation $$ Y^{\prime}(x)=\lambda Y(x)+\frac{1}{1+x^{2}}-\lambda \tan ^{-1}(x), \quad Y(0)=0 $$ \(Y(x)=\tan ^{-1}(x)\) is the true solution. Use Euler's method, the backward Euler method, and the trapezoidal method. Let \(\lambda=-1,-10,-50\), and \(h=0.5,0.1\), \(0.001\). Discuss the results.

Consider the linear equation $$ Y^{\prime}(x)=\lambda Y(x)+(1-\lambda) \cos (x)-(1+\lambda) \sin (x), \quad Y(0)=1 $$ from (8.3) of Section 8.1. The true solution is \(Y(x)=\sin (x)+\cos (x)\). Solve this problem using Euler's method with several values of \(\lambda\) and \(h\), for \(0 \leq x \leq 10\). Comment on the results. (a) \(\quad \lambda=-1 ; \quad h=0.5,0.25,0.125\) (b) \(\lambda=1 ; \quad h=0.5,0.25,0.125\) (c) \(\quad \lambda=-5 ; \quad h=0.5,0.25,0.125,0.0625\) (d) \(\quad \lambda=5 ; \quad h=0.0625\)

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