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QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

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Page 1: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480

“On the Shoulders of Giants”

An Introduction to Classical Mechanics

Page 2: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480

If I have seen further it is by standing on the shoulders of giants. Isaac Newton, Letter to Robert Hooke,

February 5, 1675English mathematician & physicist (1642 - 1727)

Page 3: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480

Quantum Mechanics (QM) is based on classical mechanics. It combines classical mechanics with statistics and statistical mechanics.

For native English-speakers, it is somewhat unfortunate that it uses the word “quantum”. A better English word which describes the thrust of this approach would be “pixel”.

Page 4: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Lights! Camera! Action!

2nd Century BC Hero of Alexandria found that light, traveling from one point to

another by a reflection from a plane mirror, always takes the shortest possible path.

1657 Pierre de Fermat reformulates the principle by postulating that

the light travels in a path that takes the least time! In hindsight, if c is constant then Hero and Fermat are in

complete agreement. Based on his reasoning, he is able to deduce both the law of

reflection and Snell’s law (nsin = n’ sin’)

Page 5: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 An Aside

Fermat is most famous for his last theorem:

Xn +Yn = Zn where n=2 and …

On his deathbed, he wrote:

And n= arrgh! I’m having a heartattack!

His last theorem was only solved by computer in the last 10 years…

Page 6: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Now we wait for the Math

1686 The calculus of variations is begun by Isaac

Newton

1696 Johann and Jakob Bernoulli extend

Newton’s ideas

Page 7: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Now we can get back

1747 Pierre-Louise-Moreau de Maupertuis asserts a

“Principle of Least Action” More Theological than Scientific “Action is minimized through the Wisdom of God” His idea of action is also kind of vague

Action (today’s definition)— Has dimensions of length x momentum or energy x

time Hmm… p * x or E*t … seems familiar…

Page 8: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 To the Physics

1760Joseph Lagrange reformulates the principle

of least action

The Lagrangian, L, is defined as L=T-V where T= kinetic energy of a system and V=potential energy of a system

Page 9: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Hamilton’s Principle

1834-1835 William Rowan Hamilton’s publishes two

papers on which it is possible to base all of mechanics and most of classical physics.

Hamilton’s Principle is that a particle follows a path that minimizes L over a specific time interval (and consistent with any constraints).

A constraint, for example, may be that the particle is moving along a surface.

Page 10: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Lagrange’s Equations

02dt

d

2dt

d

dt

d

00

gRearrangin

Recall

2

2

xm

xdx

d(-U)

so

xm

xxmxm

xmdx

d(-U)and xm

dx

dU-

dx

dU(x)-xmF

Page 11: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Lagrange’s Equations

0)(02

2

xUx

andxm

x

Now

And I can add zero to anything and not change the result

0dt

d

2

0)(2dt

d)(

2

2

22

x

L

dx

dL

Thus

VTLandTxm

but

xUxm

xx-U

xm

dx

d

Page 12: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Expanding to 3 Dimensions

Since x, y, and z are orthogonal and linearly independent, I can write a Lagrange’s EOM for each. In order to conserve space, I call x, y, and z to be dimensions 1, 2, and 3.

So

Amusingly enough, 1, 2, 3, could represent r, , (spherical coordinates) or r, , z (cylindrical) or any other 3-dimensional coordinate system.

3,2,10dt

d

iq

L

dq

dL

ii

Page 13: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480Example: Simple Harmonic

Oscillator Recall for

SHO: V(x)= ½ kx2 and let T=1/2 mv2

Hooke’s Law: F=-kx

xmkxorxmkx

so

xmxmandxmxmxx

L

kxkxdx

d

dx

dL

kxxmL

q

L

dq

dL

0

dt

d

2

1

2

12

1

2

1

0dt

d

2

2

22

Page 14: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Tip

The trick in the Lagrangian Formalism of mechanics is not the math but the proper choice of coordinate system.

The strength of this approach is that

1. Energy is a scalar and so is the Lagrangian

2. The Lagrangian is invariant with respect to coordinate transformations

Page 15: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480Two Conditions Required for

Lagrange’s Equations

1. The forces acting on the system (apart from the forces of constraint) must be derivable from a potential i.e. F=-dU/dx or some similar type of function

2. The equations of constraint must be relations that connect the coordinates of the particles and may be functions of time.

Page 16: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Your Turn

Projectile: Go to the board and work a simple projectile

problem in cartesian coordinates. Don’t worry about initial conditions yet.

Now do the same in polar coordinates.

Hint:

sin2

1

2

1 22

mgrU

rmrmT

Page 17: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Introducing the Hamiltonian

First, any Lagrangian which describes a uniform force field is independent of time i.e. dL/dt=0.

qq

L

q

L

dt

dq

dt

dL

q

L

dt

d

q

LSince

qq

Lq

q

L

dt

dL

t

L

t

q

q

L

t

q

q

L

dt

dL

qqLL

),(

Page 18: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Introducing the Hamiltonian

Hmmm… H for Hornblower or Hamilton?

HttanconsaLq

Lq

So

Lq

Lq

dt

d

dt

dL

q

Lq

dt

d

q

Lq

dt

dq

q

L

q

L

dt

dq

dt

dL

0

Page 19: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Introducing the Hamiltonian

)!(

)(2

22

1

)()(

22

energymechanicalEVT

but

HVTVTT

So

Tqmq

Tqqm

q

TqmTIf

q

T

q

qVqT

q

L

HLq

Lq

Page 20: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 H is only E when

It is important to note that H is equal to E only if the following conditions are met: The kinetic energy must be a homogeneous

quadratic function of velocity

The potential energy must be velocity independent

While it is important to note that there is an association of H with E, it is equally important to note that these two are not necessarily the same value or even the same type of quantity!

Page 21: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480Making Simple Problems

Difficult with the Hamiltonian

Most students find that the Lagrangian formalism is much easier than the Hamiltonian formalism

So why bother?

Page 22: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480Making Simple Problems

Difficult with the Hamiltonian

First, we need to define one more quantity: generalized momenta, pj

LqpHorLqpH

becomesLq

LqHSo

jwhereq

Lp

jjj

jj

3

1

3,2,1

Page 23: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 SHO with the Hamiltonian

22

222

22

2

22

2

1

2

2

1

2

2

1

2

1

kxm

pH

kxm

p

m

pL

m

ppH

becomesLqpHSo

xm

px

m

pxm

q

Lp

kxxmL

Big deal, right? But look what we did

L=f(q,dq/dt,t) H=f(q,p,t) So our mechanics all

depend on momentum but not velocity

Recall light has constant velocity, c, but a momentum which is p=hc/ !

Page 24: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 The Big Deal

So if we are going to define mechanics for light, it does not make any sense to use the Lagrangian formulation, only the Hamiltonian!

Page 25: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 That Feynman Guy!

Richard Feynman thought that Lagrangian mechanics was too powerful a tool to ignore.

Feynman developed the path integral formalism of quantum mechanics which is equivalent to the picture of Schroedinger and Dirac.

So which is better? Both and Neither There seems to be no undergraduate treatment of

path integral formalism.

Page 26: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480Hamilton’s Equations of

Motion Just like Lagrangian formalism, the Hamiltonian

formalism has equations of motion. There are two equations for every degree of freedom

They are

q

Hp

p

Hq

Page 27: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Finishing the SHO

kxF

pdt

dpFSince

kxporkxq

Hp

m

p

p

Hx

kxm

pH

22

2

1

2

Hooke’s Law again!

Page 28: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Symmetry

Note that Hamilton’s EOM are symmetric in appearance i.e. that q and p can almost be interchanged!

Because of this symmetry, q and p are said to be conjugate

q

Hp

p

Hq

Page 29: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Definition of Cyclic

Consider a Hamiltonian of a free particle i.e. H=f(p)… then – dp/dt=0 i.e. momentum is a “constant of the motion”

Now in the projectile problem, U=-mgy and for x-component, H=f(px) only!

Thus, px= constant and the horizontal variable, x is

said to “cyclic”!

A more practical definition of cyclic is “ignorable” and modern texts sometimes use this term.

Page 30: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Definition of canonical

Canonical is used to describe a simple, general set of something … such as equations or variables.

It was first introduced by Jacobi and rapidly gained common usuage but the reason for its introduction remained obscured even to contemporaries

Lord Kelvin was quoted as saying “Why it has been so called would be hard to say”

Page 31: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Poisson Brackets

},{},{

0},{

0},{

0},{

p? and q of functions were vandu ifWhat

},{

as defined is

p and q variablescanonical therespect to with vandu ofBracket Poisson

, jijiji

ji

yx

ji

qppq

pp

p

x

y

y

p

y

x

xyxExample

qq

p

u

q

v

p

v

q

uvu

Page 32: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Kronecker Delta

i,k=1 if i=k

i,k=0 if i≠k

Page 33: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Back to Fish

Consider two continuous functions g(q,p) and h(q,p) If {g,h}=0 then h and g are said to commute In other

words, the order of operations does not matter

If {g,h}=1 then quantities are canonically conjugate

• A look ahead: we will find that canonically conjugate quantities obey the Uncertainty principle

Page 34: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Properties of Fish

},{ c)

},{ b)

p)H(q,Hn HamiltoniaH where

},{ a)

BracketPoisson theof properties are following The

Hpp

Hqq

t

gHg

dt

dg

jj

jj

Page 35: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Levi-Civita Notation

1

1

0

order) of(out n permutatio oddan isk j, i, if 1-

2,3 1, of permuationeven an isk j, i, if 1

otherany equalsindex any if 0

C

notation

compact ain expressed becan components individual The

B AC

B and A ofproduct vector heConsider t

132321213

231312123

133112122

,i

ijk

kjkjijk

where

BA

Page 36: QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics

QM 480 Levi-Civita Notation

23132321231

132

123

23321

321

321

1

1

Consider

3̂2̂1̂

C

B and A ofproduct vector heConsider t

BABAC

BABAC

BBB

AAA