Mechanics Canonical Transformation 3, Lecture Notes - Physics, Study notes of Mechanics

Mechanics Physics Canonical Transformations Infinitesimal CT Poisson Bracket Hamilton’s equations Momentum Conservation Angular Momentum Integrating ICT Rotation CT Free Fall Harmonic Oscillator Liouville’s Theorem

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Mechanics
Physics 151
Lecture 22
Canonical Transformations
(Chapter 9)
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Mechanics

Physics 151

Lecture 22

Canonical Transformations

(Chapter 9)

What We Did Last Time „^

Direct Conditions^ „

Necessary and sufficientfor Canonical Transf. „^

Infinitesimal CT

„^

Poisson Bracket^ „

Canonical invariant „ Fundamental PB „ ICT expressed by „ Infinitesimal time transf. generated by Hamiltonian^ Æ

Hamilton’s equations

,

,

j

i j^

i^ Q P

q p

p

Q q^

P

⎛^

⎞^

∂⎛

∂^

=

⎜^

⎟^

⎜^

⎜^

⎟ ∂^

∂⎝

⎝^

⎠^

,

,

j

i j^

i^ Q P

q p

q

Q p^

P

⎛^

⎞^

∂⎛

∂^

= −

⎜^

⎟^

⎜^

⎜^

⎟ ∂^

∂⎝

⎝^

,

,

j

i j^

i^ Q P

q p

p

P q^

Q

⎛^

⎞^

∂⎛

∂^

= −

⎜^

⎟^

⎜^

⎜^

⎟ ∂^

∂⎝

⎝^

⎠^

,

,

j

i j^

i^ Q P

q p

q

P p^

Q

⎛^

⎞^

∂⎛

∂^

=

⎜^

⎟^

⎜^

⎜^

⎟ ∂^

∂⎝

⎝^

[^

] ,

i^

i^

i^

i

u^

v^

u^

v

u v

q^

p^

p^

q

∂^

∂^

∂^

≡^

∂^

∂^

∂^

[^

,^

]^

[^

,^

]^

i^

j^

i^

j

q^

q^

p^

p

=^

=^

[^

,^

]^

[^

,^

]

i^

j^

i^

j^

ij

q^

p^

p^

q

δ

=^

−^

[ ,

]^

u

u^

u G

t t

δ^

=^

Dynamic View of CT „^

A system evolves with time^ „

At any moment,

q

and

p satisfy Hamilton’s equations

„^

The time-evolution must be a Canonical Transformation!^ „

Static View = Coordinate system is changing „ Dynamic View = Physical system is moving

0

0

(^

),^

(^

q t

p t

q t

p t

q

p

This movement

is a CT

Infinitesimal Time CT „^

Infinitesimal CT^ „

We know that the generator = Hamiltonian „ Integrating it with time should give us the “finite” CT thatturns the initial conditions

q

( t^0

),^

p (

t ) into the configuration^0

q (

t ),

p

( t ) of the system at arbitrary time „^

That’s a new definition of “solving” the problem

q t

p t

(^

),^

(^

q t

dt

p t

dt

+^

[ ,

]^

u

du

dt u H

dtt

=^

∂^

[ ,

]

q^

q H ^ =

[^

,^

]

p^

p H =

Hamiltonian is the generator of the system’s

motion with time

Hamiltonian is the generator of the system’s

motion with time

Conservation „^

Consider an ICT generated by

G

„^

Suppose

G

is conserved and

has no explicit

t -dependence

„^

How is

H

(without

t -dependence) changed by the ICT?

„^

A transformation that does not affect

H

Æ

Symmetry of the system

Æ

Generator of the transformation is conserved

[ ,

]^

u

u^

u G

t t

δ^

=^

[^

,^

]^

G H

[^

,^

]^

H

H

H G

t t

δ^

=^

+^

If an ICT does not affectHamiltonian, its generator

is conserved

Momentum Conservation „^

Simplest example:^ „

What is the ICT generated by momentum

p

? i

„^

That’s a shift in

q

by i

ε^ Æ

spatial translation

„^

If Hamiltonian is unchanged by such shift, then Æ

Momentum

p

is conserved i

„^

This is not restricted to linear momentum

[^

,^

]

j^

j^

i^

ij

q^

q^

p

δ^

=^

=^

[^

,^

]^

j^

j^

i

p^

p^

p

δ^

=^

[^

,^

]^

i H p

Hamiltonian isunchanged by a shift of acoordinate

q

The generatorof the ICT isthe conjugatemomentum

p

p^

is conserved

[^

,^

]^

H

p

Angular Momentum „^

The generator

is obviously

„^

i.e. the

z -component of the total momentum

„^

Generator for rotation about an axis given by a unit vector

n

should be

„^

We now know generators of 3 important ICTs^ „

Hamiltonian generates displacement in time „ Linear momentum generates displacement in space „ Angular momentum generates rotation in space

i^

iy^

i^

ix

G

x p

y p

=^

−^

(^

z^

i^

i^ z

L^

=^

×

r^

p

G

L n

Integrating ICT „^

I said we can “integrate” ICT to get finite CT^ „

How do we integrate

„^

First, let’s rewrite it as^ „

We want the solution

u

(^ α

) as a function

of

with the initial condition

u

u 0

„^

Taylor expand

u

(^ α

) from

α^

[ , = 0

]

u^

u G

δ^

[ ,

]

du

d^

u G α =^

[ ,

]

du

u G

d^ α

2

2

3

3

0

2

3

0

0

0

(^

)^

du

d u

d u

u^

u^

d^

d^

d

α

α

α

α^

α

α

α

=^

+^

+^

+^

This is

[ u

, G

]^0

What can I do with these?

Rotation CT „^

Let’s integrate the ICT for rotation around

z

„^

Let me forget the particle index

i

„^

Parameter

α^

is

θ^

in this case

„^

Let’s see how

x changes with

θ

„^

Evaluate the Poisson Brackets „^

Where does this lead us?

y^

x

G

xp

yp

=^

2

3

0

0

0

0

[ ,

]^

[[ ,

],^

]^

[[[ ,

],^

],^

]

x^

x^

x G

x G

G

x G

G

G

θ

θ

θ

θ

=^

+^

+^

+^

[ ,

]

x G

y = −

[[ ,

],^

]

x G

G

x =^

−^

[[[ ,

],^

],^

]

x G

G

G

y

[[[[ ,

],^

],^

],^

]

x G

G

G

G

x =^

Repeats after this

Rotation CT

„^

Similarly

2

3

0

0

0

0

2

3

4

0

0

0

0

0

2

4

3

5

0

0

0

0

[ ,

]^

[[ ,

],^

]^

[[[ ,

],^

],^

]

cos

sin

x^

x^

x G

x G

G

x G

G

G

x^

y^

x^

y^

x

x^

y

x^

y

θ

θ

θ

θ

θ^

θ^

θ

θ

θ^

θ

θ^

θ

θ

θ

θ

=^

+^

+^

+^

=^

−^

−^

+^

+^

⎛^

⎞^

⎛^

=^

−^

+^

−^

−^

−^

+^

⎜^

⎟^

⎜^

⎝^

⎠^

⎝^

=^

2

3

0

0

0

0

0

0

[ ,

]^

[[ ,

],^

]^

[[[ ,

],^

],^

]

cos

sin

y^

y^

y G

y G

G

y G

G

G

y^

x

=^

+^

+^

+^

=^

Infinitesimal Rotation „^

ICT for rotation is generated by^ „

We’ve studied infinitesimal rotation in Lecture 8 „ Infinitesimal rotation of

d

θ^

about

n

moves a vector

r as

„^

Compare the two expressions

„^

Equation

holds for any

r

that rotates

together with the system^ „

Several useful rules can be derived from this

G

L n

d^

d^ θ

=^

×

r^

n^

r

[ ,

]

d^

d^

d

=^

⋅^

=^

×

r^

r L n

n^

r^

[ ,

]

⋅^

=^

×

r L n

n^

r

[ ,

]

⋅^

=^

×

r L n

n^

r

Scalar Products „^

Consider a scalar product

of two vectors

„^

Try to rotate it „^

Obvious: scalar product doesn’t change by rotation „^

Also obvious: length of any vector is conserved

a b

[^

,^

]^

[ ,

]^

[ ,

]

(^

)^

(^

(^

)^

(^

⋅^

⋅^

=^

⋅^

⋅^

+^

⋅^

=^

⋅^

×^

+^

⋅^

×

=^

⋅^

×^

+^

⋅^

×

a b L n

a^

b L n

b^

a L n

a^

n^

b^

b^

n^

a

a^

n^

b^

a^

b^

[ , n

]

⋅^

=^

×

r L n

n^

r

Angular Momentum „^

Imagine two conserved quantities

A

and

B

„^

How does [

A ,

B ] change with time?

„^

Poisson bracket of two conserved quantities is conserved

„^

Now consider^ „

If 2 components of

L

are conserved, the 3

rd^

component must

Æ

Total vector

L

is conserved

[^

,^

]^

[^

,^

]^

A H

B H

=^

[[^

,^

],^

]^

[[^

,^

],^

]^

[[^

,^

],^

]^

A B

H

B H

A^

H A

B

=^

−^

−^

Jacobi’s identity

[^

,^

]

i^

j^

ijk^

k

L^

L^

L

Angular Momentum „^

Remember the Fundamental Poisson Brackets?^ „

Now we know „ Poisson brackets between

L

,^ x Ly

,^ L

are non-zero z

„^

On the other hand,

, so |

L | may be a canonical

momentum „^

QM: You may measure |

L | and, e.g.,

L

simultaneously, but z

not

L

and x

L

, etc. y

[^

,^

]^

[^

,^

]^

i^

j^

i^

j

q^

q^

p^

p

=^

=^

[^

,^

]^

[^

,^

]

i^

j^

i^

j^

ij

q^

p^

p^

q

δ

=^

−^

PB of two canonical momenta is 0[^

,^

]

i^

j^

ijk^

k

L^

L^

L

[^

,^

]^

i L^

L^

Only 1 of the 3 components of the angular momentum

can be a canonical momentum