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               Chapter 2                 Newton’s Second Law
               The First Law of Thermodynamics  The fundamental equation of classical mechanics is Newton’s second law of motion:

                                                                          F   ma                            (2.1)*
                                         where m is the mass of a body, F is the vector sum of all forces acting on it at some
                                         instant of time, and a is the acceleration the body undergoes at that instant. F and a
                                         are vectors, as indicated by the boldface type. Vectors have both magnitude and di-
                                         rection. Scalars (for example, m) have only a magnitude. To define acceleration, we
                                         set up a coordinate system with three mutually perpendicular axes x, y, and z. Let r be
                                         the vector from the coordinate origin to the particle (Fig. 2.1). The particle’s velocity v
                                         is the instantaneous rate of change of its position vector r with respect to time:
                                                                         v   dr>dt                          (2.2)*
                                         The magnitude (length) of the vector v is the particle’s speed v. The particle’s accel-
               Figure 2.1                eration a is the instantaneous rate of change of its velocity:
                                                                                 2
               The displacement vector r from                       a   dv>dt   d r>dt 2                    (2.3)*
               the origin to a particle.
                                             A vector in three-dimensional space has three components, one along each of the
                                         coordinate axes. Equality of vectors means equality of their corresponding compo-
                                         nents, so a vector equation is equivalent to three scalar equations. Thus Newton’s sec-
                                         ond law F   ma is equivalent to the three equations
                                                             F   ma ,   F   ma ,   F   ma    z               (2.4)
                                                                                 y
                                                              x
                                                                           y
                                                                                       z
                                                                    x
                                         where F and a are the x components of the force and the acceleration. The x compo-
                                                x     x
                                         nent of the position vector  r is simply  x, the value of the particle’s  x coordinate.
                                                                 2
                                                                     2
                                         Therefore (2.3) gives a   d x/dt , and (2.4) becomes
                                                             x
                                                                  2
                                                                                2
                                                                                               2
                                                                 d x           d y            d z
                                                          F   m   2  ,   F   m   2  ,   F   m   2            (2.5)
                                                                          y
                                                                                        z
                                                           x
                                                                 dt            dt             dt
                                             The weight W of a body is the gravitational force exerted on it by the earth. If g is
                                         the acceleration due to gravity, Newton’s second law gives
                                                                          W   mg                             (2.6)
                                         Units
                                         In 1960 the General Conference on Weights and Measures recommended a single sys-
                                         tem of units for use in science. This system is called the International System of
                                         Units (Système International d’Unités), abbreviated SI. In mechanics, the SI uses me-
                                         ters (m) for length, kilograms (kg) for mass, and seconds (s) for time. A force that pro-
                                                                                2
                                         duces an acceleration of one meter per second when applied to a one-kilogram mass
                                         is defined as one newton (N):
                                                                      1 N   1 kg m/s 2                       (2.7)
                                             If one were to adhere to SI units, pressures would always be given in
                                                      2
                                         newtons/meter (pascals). However, it seems clear that many scientists will continue
                                         to use such units as atmospheres and torrs for many years to come. The current scien-
                                         tific literature increasingly uses SI units, but since many non-SI units continue to be
                                         used, it is helpful to be familiar with both SI units and commonly used non-SI units.
                                                                                                     3
                                         SI units for some quantities introduced previously are cubic meters (m ) for volume,
                                              3
                                         kg/m for density, pascals for pressure, kelvins for temperature, moles for amount of
                                         substance, and kg/mol for molar mass.
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