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30     CHAPTER 1 First-Order Differential Equations


                        SECTION 1.4        PROBLEMS


                     In each of Problems 1 through 14, find the general solu-  14. y +  2  y =  3  y  2

                     tion. These problems include all three types discussed in  x  x
                     this section.                                 15. Consider the differential equation

                            1    1                                                      ax + by + c
                              2


                      1. y =  y −  y + 1                                         y = F
                            x  2  x                                                     dx + py +r
                            1  2
                                  −4/3
                      2. y +  =  y                                     in which a,b,c,d, p,and r are constants. Show that
                            x  x  3
                                                                       this equation is homogeneous if and only if c =r = 0.

                      3. y + xy = xy 2
                                                                       Thus, suppose at least one of c and r is not zero.
                            x  y                                       Then this differential equation is called nearly homo-

                      4. y =  +
                            y  x                                       geneous. Show that if ap − bd  = 0 it is possible to
                             y                                         choose constants h and k such that the transforma-

                      5. y =                                           tion x = X + h, y = Y + k results in a homogeneous
                            x + y
                                                                       equation.
                            1     1   4
                               2
                      6. y =  y −  y −
                            2x    x   x
                                                                   In each of Problems 16 through 19, use the idea from
                      7. (x − 2y)y = 2x − y                        Problem 15 to solve the differential equation.

                      8. xy = x cos(y/x) + y

                                                                            y − 3

                            1   1                                  16. y =  x + y − 1

                      9. y +  y =  y  −3/4
                            x   x  4
                                                                          3x − y − 9
                              2

                         2
                     10. x y = x + y 2                             17. y =

                                                                           x + y + 1
                             1    2
                               2
                     11. y =− y +  y                                       x + 2y + 7
                             x    x                                18. y =

                                                                          −2x + y − 9
                              2
                         3

                     12. x y = x y − y 3
                                                                          2x − 5y − 9

                                2
                              −x
                     13. y =−e y + y + e x                         19. y =  −4x + y + 9

                     1.5         Additional Applications
                                 This section is devoted to some additional applications of first-order differential equations. We
                                 will need Newton’s second law of motion, which states that the sum of the external forces acting
                                 on an object is equal to the derivative (with respect to time) of the product of the mass and
                                 the velocity. When the mass is constant, dm/dt = 0, and Newton’s law reduces to the familiar
                                 F = ma in which a = dv/dt is the acceleration.
                                 Terminal Velocity An object is falling under the influence of gravity in a medium such as water,
                                 air, or oil. We want to analyze the motion.
                                    Let v(t) be the velocity of the object at time t. Gravity pulls the object downward, while
                                 the medium retards the downward motion. Experiment has shown that this retarding force is
                                 proportional in magnitude to the square of the velocity. Let m be the mass of the object, g the
                                 usual constant acceleration due to gravity, and α the constant of proportionality in the retarding
                                 force of the medium. Choose downward as the positive direction (this is arbitrary). Let F be the
                                 magnitude of the total external force acting on the object. By Newton’s law,
                                                                             dv
                                                                        2
                                                              F = mg − αv = m   .
                                                                             dt
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