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The Principle of Least Action: Derivation and Applications, Study notes of Advanced Calculus

An in-depth exploration of the Principle of Least Action, a fundamental concept in physics. It covers the derivation of the Euler-Lagrange equations, applications to various physical systems, and solutions for problems such as the brachistochrone and the catenary. The document also includes Mathematica code for visualizing the solutions.

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The Principle of Least Action
Jason Gross, Dece mber 7, 2010
Introduction
Recall that we defined the Lagrangian to be the kinetic energy less potential ener gy, LKU, at a point. The action is then
defined to be the integral of the Lagrangian along the path,
Sf
Ã
t0
t1
Ltf
Ã
t0
t1
KUt
It is (remarkably!) true that, in any physical system, the path an object actually takes minimizes the action. It can be shown that
the extrema of action occur at
L
q
t
L
q
f0
This is called the Euler equation, or the Euler-Lagrange Equation.
Derivation
Courtesy of Scott Hughes’s Lecture notes for 8.033. (Most of this is copied almost verbatim from that.)
Suppose we have a function f
+
x,x
;t
/
of a variable x and its derivative x
f
x
s
t. We want to find an extremum of
J
Ã
t0
t1
f+x+t/,x
+t/;t/t
Our goal is to compute x
+
t
/
such that J is at an extremum. We consider the limits of integration to be fixed. That is, x
+
t
1
/
will be
the same for any x we care about, as will x
+
t
2
/
.
Imagine we have some x
+
t
/
for which J is at an extremum, and imagine that we have a function which par ametrizes how far our
current path is from our choice of x:
x
+
t;
/
x
+
t
/
A
+
t
/
The function A is totally arbitrary, except that we require it to vanish at the endpoints: A
+
t
0
/
A
+
t1
/
0. The parameter allows
us to control how the variation A
+
t
/
enters into our path x
+
t;
/
.
The “correct” path x
+
t
/
is unknown; our goal is to figure out how to construct it, or to figure out how f behaves when we are on it.
Our basic idea is to ask how does the integral J behave when we are in the vicinity of the extremum. We know that ordinary
functions are flat --- have zero first derivative --- when we are at an extremum. So let us put
J
+
/
Ã
t0
t
1
f
+
x
+
t;
/
,x
+
t;
/
;t
/
t
pf3
pf4
pf5
pf8
pf9
pfa
pfd

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The Principle of Least Action

Jason Gross, December 7, 2010

Introduction

Recall that we defined the Lagrangian to be the kinetic energy less potential energy, LKU , at a point. The action is then defined to be the integral of the Lagrangian along the path, S  (^)  t 0

t 1 Lt  (^)  t 0

t 1 KUt

It is (remarkably!) true that, in any physical system, the path an object actually takes minimizes the action. It can be shown that the extrema of action occur at  Lq ^

t

 L

q^ ^ ^0 This is called the Euler equation, or the Euler-Lagrange Equation.

 Derivation

Courtesy of Scott Hughes’s Lecture notes for 8.033. (Most of this is copied almost verbatim from that.) Suppose we have a function f  x , x^ ^ ; t  of a variable x and its derivative x^ ^   x  t. We want to find an extremum of

J  (^)  t 0

t 1 f  x  t , x^ ^  t ; t   t

Our goal is to compute x  t  such that J is at an extremum. We consider the limits of integration to be fixed. That is, x  t 1  will be the same for any x we care about, as will x  t 2 . Imagine we have some x  t  for which J is at an extremum, and imagine that we have a function which parametrizes how far our current path is from our choice of x : x  t ;   x  t    A  t  The function A is totally arbitrary, except that we require it to vanish at the endpoints: A  t 0   A  t 1   0. The parameter  allows us to control how the variation A  t  enters into our path x  t ; . The “correct” path x  t  is unknown; our goal is to figure out how to construct it, or to figure out how f behaves when we are on it. Our basic idea is to ask how does the integral J behave when we are in the vicinity of the extremum. We know that ordinary functions are flat --- have zero first derivative --- when we are at an extremum. So let us put J   (^)  t 0

t 1 f  x  t ; , x^ ^  t ; ; t   t

We know that   0 corresponds to the extremum by definition of . However, this doesn’t teach us anything useful, sine we don’t know the path x  t ^ that corresponds to the extremum.

But we also know We know that   J  0  0 since it’s an extremum. Using this fact,

J  

 (^)  t 0

t 1  fx

x  

fx^ 

x^  

tx  ^

   x  t ^  ^ A  t ^ ^ A  t   x^   

t

 x  t    A  t   ^ At So

J  

 (^)  t 0

t 1  fx

A  t  

fx^ 

 A

t

t

Integration by parts on the section term gives

 t 0

t 1  fx^ 

 A

t ^ t^ ^ A  t ^

fx^ ^ t 0

t 1  (^)  t 0

t 1 A  t 

t

fx^ ^ ^ t

Since A  t 0   A  t 1   0, the first term dies, and we get

J 

t 0

t 1 A  t 

fx

t

fx^ ^

t

This must be zero. Since A  t  is arbitrary except at the endpoints, we must have that the integrand is zero at all points:

fx

t

fx^ ^

This is what was to be derived.

Least action: F m a

Suppose we have the Newtonian kinetic energy, K  12 m v^2 , and a potential that depends only on position, UU  r^ . Then the Euler-Lagrange equations tell us the following:

ClearU, m, r L  1 2

m r 't^2  Urt; rt L  Dtr't L, t, Constants  m  0  Urt  m rt  0

Rearrangement gives

 U

r

m r^ ¨ Fm a

 Angular Momentum

Let us change to polar coordinates. xt_ : rt Cost yt_ : rt Sint K  ExpandFullSimplify 12 m x 't^2  y't^2   TraditionalForm 1 2

m r  t ^2 

m r  t ^2  t ^2

Using dot notation, this is K . r_ 't  OverDotr . r_t  r  TraditionalForm 1 2

^2 m r^2  m r

Note that  does not appear in this expression. If potential energy is not a function of  (is only a function of r ), then   L   m r^2  is constant. This is standard angular momentum, m r^2   r m r   rm v.

Classic Problem: Brachistochrone (“shortest time”)

 Problem

A bead starts at x  0, y  0, and slides down a wire without friction, reaching a lower point  x (^) f , y (^) f . What shape should the wire be in order to have the bead reach  x (^) f , y (^) f  in as little time as possible.

 Solution

 Idea

Use the Euler equation to minimize the time it takes to get from  xi , yi  to  x (^) f , y (^) f .

 Implementation

Letting  s be the infinitesimal distance element and v be the travel speed,

T  (^)  t i

tfs v ^ ts   x ^2   y ^2   y 1   x '^2 x '  ^ xy v  2 g y (Assumption: bead starts at rest)

T   0

y (^) f 1   x '^2 2 g y

y

Now we apply the Euler equation to f  1  2  g yx '^2 and change ty , x^ ^  x '.

fx

y

fx^ ^

fx

fx^ ^

2 g y

x ' 1   x '^2   y

fx^ ^

2 g y

x ' 1   x '^2

 Constant

Squaring both sides and making a special choice for the constant gives

 x '^2 2 g y  1   x '^2 

4 g A

xy

2 

y  2 A  1  y   2 A  ^

y^2 2 A yy^2

x  (^)  0

y (^) fxy ^ y^ ^  0

y (^) f y 2 A yy^2

y

To solve this, change variables:

yA  1  cos,  yA sin   FullSimplify2 A y  y^2 . y  A 1  Cos A^2 Sin^2 y 2 A yy^2

y

A  1  cos A^2 sin^2 

A sin    A  1  cos

x  (^)  0

A  1  cos    A   sin

Full solution: The brachistochrone is described by

xA   sin yA  1  cos

There’s no analytic solution, but we can compute them.

U  

0

lg ys

s   x ^2   y ^2   y 1   x '^2 x ' 

xy U  (^)  y 0

y (^) fg y 1   x '^2  y

Note that if we choose to factor  s the other way (for y '), we get a mess.

Now we apply the Euler-Lagrange equation to f   g y 1   x '^2 and change ty , x^ ^  x '.

fx

y

fx '

fx

fx '

g y x ' 1   x '^2

Since  ^ fx  0,  ^ xf ' is constant, say a  (^) ^1 g^  ^ fx '  y x ' 1  x '^2

. Then

x ' 

xy  ^

a y^2  a^2

Using the fact that

y y^2  a^2

 cosh^1

y a ^ b ,

integration of x ' gives

x  y    a cosh^1

y a

b

where b is a constant of integration.

Plotting this for a  1, b  0 gives:

In[14]:= Cleary; ManipulateParametricPlot a ArcCosh t a

  b, t, a ArcCosh t a

  b, t, t, ymin, ymax , PlotStyle  Black, a, 1 , 5, 5 , b, 0 , 5, 5 , ymin, 0, ymin ,  5, 5 , ymax, 2, ymax , 5, 5 

Out[14]=

a b ymin ymax

1.0 0.5 0.5 1.

Problem: Bead on a Ring

From 8.033 Quiz #

Clearr, , ; DeferL  Lpolar  ExpandFullSimplifyL . x  Functiont, R Cos t Sint, y  Functiont, R Sin t Sint, z  Functiont, R  R Cost  . 't   . t    TraditionalForm 0  Defer L  Dt"", t  L  EL  ExpandFullSimplify t Lpolar  t 't Lpolar . t    TraditionalForm  ''t  ''t . SolveEL  0, ''t 1   TraditionalForm

L  g m R cos  g m R

m R^2 ^2 cos 2  

^2 m R^2 

m R^2 ^2

0 

 L

t

 L

 ^

  g m R sin  m R^2 ^2 sin cos  m R^2  t 

 t  

R ^2 sin t  cos t   g sin t  R Finding the minimum value of  for the bead to be in equilibrium gives ''t . SolveEL  0, ''t 1   0  TraditionalForm RefineReduce  ''t . SolveEL  0, ''t 1   0, Cost, Sint 0 && R Cost 0 && g 0 && R 0  . t    TraditionalForm R ^2 sin t  cos t   g sin t  R ^0 cos 

g R ^2 In order for this to have a solution, we must have

 

g R If   2, then cos  0, so   .

Problem 11.8: K & K 8.

 Problem

A pendulum is rigidly fixed to an axle held by two supports so that it can only swing in a plane perpendicular to the axle. The pendulum consists of a mass m attached to a massless rod of length l. The supports are mounted on a platform which rotates with constant angular velocity . Find the pendulum’s frequency assuming the amplitude is small.

 Solution by torque

(From the problem set solutions)

The torque about the pivot point is  p   Ip

k^ ^ :  g  m sin   F cent cos  ^ ¨ Ip^ (1) The centrifugal effective force is F cent  m  sin ^2 For small angles, sin  , cos  1. Then equation (1) becomes

g  m   m ^2  ^2  m ^2 

¨

¨  g 

 ^2   0

If ^2  g  , the motion is no longer harmonic.