Page 203 - Intro to Tensor Calculus
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               is satisfied. Integrating the second term of this integral by parts we find

                                       Z  t 1  ∂L       ∂L     t 1  Z  t 1  d     ∂L
                                                          i
                                                                                 i
                                               i
                                  δI =        η dt +     η (t)  −               η (t) dt =0.          (2.2.32)
                                           ∂x i       ∂ ˙x i          dt  ∂ ˙x i
                                        t 0                   t 0  t 0
                                     i
               The end condition on η (t) makes the middle term in equation (2.2.32) vanish and we are left with the
               integral
                                                 Z
                                                   t 1    ∂L    d   ∂L
                                                      i
                                            δI =    η (t)     −           dt =0,                      (2.2.33)
                                                          ∂x i  dt  ∂ ˙x i
                                                  t 0
                                                    i
                                          i
               which must equal zero for all η (t). Since η (t) is arbitrary, the only way the integral in equation (2.2.33) can
                             i
               be zero for all η (t) is for the term inside the brackets to vanish. This produces the result that the integral
               of the Lagrangian is an extremum when the Euler-Lagrange equations

                                               d   ∂L     ∂L
                                                        −     =0,   i =1,... ,N                       (2.2.34)
                                              dt  ∂ ˙x i  ∂x i
               are satisfied. This is a necessary condition for the integral I( ) to have a minimum value.
                   In general, any line integral of the form
                                                         Z  t 1
                                                                    i
                                                                 i
                                                     I =    φ(t, x , ˙x ) dt                          (2.2.35)
                                                          t 0
                                                                    i
                                                              i
               has an extremum value if the curve c defined by x = x (t),i =1,... ,N satisfies the Euler-Lagrange
               equations

                                               d   ∂φ     ∂φ
                                                       −     =0,   i =1,... ,N.                       (2.2.36)
                                              dt  ∂ ˙x i  ∂x i
               The above derivation is a special case of (2.2.36) when φ = L. Note that the equations of motion equations
               (2.2.34) are just another form of the equations (2.2.24). Note also that


                                       δT    δ   1     i j         i j       i       i
                                          =       mg ij v v  = mg ij v f = mf i v = mf i ˙x
                                        δt   δt  2
                                                                                                       ∂V
               and if we assume that the force Q i is derivable from a potential function V ,then mf i = Q i = −  ,so
                                                                                                       ∂x i
                    δT        i      i    ∂V   i    δV     δ
               that    = mf i ˙x = Q i ˙x = −  ˙ x = −  or  (T + V )= 0 or T + V = h = constant called the energy
                    δt                    ∂x i      δt    δt
               constant of the system.
                   Action Integral
                   The equations of motion (2.2.34) or (2.2.24) are interpreted as describing geodesics in a space whose
               line-element is
                                                    2
                                                                      j
                                                  ds =2m(h − V )g jk dx dx k
               where V is the potential function for the force system and T + V = h is the energy constant of the motion.
               The integral of ds along a curve C between two points P 1 and P 2 is called an action integral and is

                                                    Z                 j  k    1/2
                                                √     P 2           dx dx
                                           A =   2m       (h − V )g jk         dτ
                                                                    dτ dτ
                                                     P 1
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