Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26....

39
Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass) What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc 2 Deriving relativistic quantum Lagrangian-Hamiltonian relations Feynman’s flying clock and phase minimization Geometry of relativistic mechanics (Includes Lecture 25 review) 1 Tuesday, April 3, 2012

Transcript of Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26....

Page 1: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics

(Ch. 2-5 of Unit 2 4.03.12)

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

(Includes Lecture 25 review)

1Tuesday, April 3, 2012

Page 2: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

2Tuesday, April 3, 2012

Page 3: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Introducing the “Sin-Tan Rosetta Stone”

https://www.uark.edu/ua/pirelli/php/hyper_constrct.php

NOTE: Angle φ is now called stellar aberration angle σ

Fig. C.2-3and

Fig. 5.4in Unit 2

3Tuesday, April 3, 2012

Page 4: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

More about the“Sin-Tan Rosetta”

Note identities

4Tuesday, April 3, 2012

Page 5: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsGeometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

5Tuesday, April 3, 2012

Page 6: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts

(From Fig. 2.3.4)

GGrroouupp vveelloocciittyy u aanndd pphhaassee vveelloocciittyy c2/uaarree hhyyppeerrbboolliicc ttaannggeenntt ssllooppeess

Newtonian speed u~cρRelativisticgroup wavespeed u=c tanh ρ

LLooww ssppeeeedd aapppprrooxxiimmaattiioonn

33−

== BB==22ϖ

433221100--11

4

--22

BB ccoosshh ρ

BB ssiinnhh ρBB ee--ρ ck

ω

== 22BB==442ϖ

Δω

c Δk

PPGG

BB ee++ρ

Ghyperbolas

P hyperbolasc line

cc

ω

ck

u

cu

c dω =dcckkcckkω=

Group velocity

k=BB ssiinnhh ρω=BB ccoosshh ρ

ω =cckkccuu

Phase velocity

== BBϖ

Rare but important case where

with LARGE Δk(not infinitesimal)

dωdk =

ΔωΔk

PPΔω

c Δk

ccuu

BB ssiinnhh ρ

BB ccoosshh ρ

Rapidity ρ approaches u/c

Lecture 25 ended here 6Tuesday, April 3, 2012

Page 7: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

PPΔω

c Δk

BB ssiinnhh ρ

BB ccoosshh ρ

Group vs. phase velocity and tangent contacts

7Tuesday, April 3, 2012

Page 8: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

PPΔω

c Δk

BB ssiinnhh ρ

BB ccoosshh ρ

8Tuesday, April 3, 2012

Page 9: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

9Tuesday, April 3, 2012

Page 10: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Start with low speed approximations : ω = Bcoshρ = B(1+2

1 ρ2 + ...) where: ρ uc

10Tuesday, April 3, 2012

Page 11: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Start with low speed approximations : ω = Bcoshρ = B(1+2

1 ρ2 + ...) where: ρ uc

11Tuesday, April 3, 2012

Page 12: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Start with low speed approximations : ω = Bcoshρ = B(1+2

1 ρ2 + ...) where: ρ uc

12Tuesday, April 3, 2012

Page 13: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Start with low speed approximations : ω = Bcoshρ = B(1+2

1 ρ2 + ...) where: ρ uc

13Tuesday, April 3, 2012

Page 14: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

14Tuesday, April 3, 2012

Page 15: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

15Tuesday, April 3, 2012

Page 16: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

cp'=hck'cctt

cctt''

EnergyE=hω

Momentumcp=hck

Mc2

ωm=49ω1

76543210-1-2-3-4-4-6m

36

251694

(a) Einstein-Planck Dispersion

(b) DeBroglie-Bohr Dispersion

E'=hω'E2 - c2p2 =(Mc2)2

photon: M=0E = c p

E = p2/2M

E = B m2

tachyon:

Bohr - Schrodinger Dispersion

Einstein - Planck Dispersion

16Tuesday, April 3, 2012

Page 17: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

17Tuesday, April 3, 2012

Page 18: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

18Tuesday, April 3, 2012

Page 19: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

19Tuesday, April 3, 2012

Page 20: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

20Tuesday, April 3, 2012

Page 21: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

21Tuesday, April 3, 2012

Page 22: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Mrest(γ)=0 Mmom(γ)=p/c=k/c=ω/c2 Meff(γ)=∞

Equations (4.11) in Unit 2

Three kinds of mass for photon γ in CW relativistic theory What’s the matter with light?

(1)Einstein rest mass (2) Galilean momentum mass (3) Newtonian inertial mass Mrest= Mmom=p/u= Mmom=F/a=

ω proper

c2

kdωdk

d 2ωdk 2

A 2-CW 600THz cavity has zero total momentum p, but each photon adds a tiny mass Mγ to it.

Mγ=ω/c2=ω (1.2·10-51)kg·s= 4.5·10-36kg (for: ω = 2π·600THz )

A 1-CW state has no rest mass, but 1-photon momentum is a non-zero value pγ=Mγ c. (Galilean revemge II.)

pγ=k=ω/c=ω (4.5·10-43)kg·m=1.7·10-27kg·m·s-1 (for: ω = 2π·600THz )

22Tuesday, April 3, 2012

Page 23: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Mrest(γ)=0 Mmom(γ)=p/c=k/c=ω/c2 Meff(γ)=∞

Equations (4.11) in Unit 2

Three kinds of mass for photon γ in CW relativistic theory What’s the matter with light?

(1)Einstein rest mass (2) Galilean momentum mass (3) Newtonian inertial mass Mrest= Mmom=p/u= Meff=F/a=

ω proper

c2

kdωdk

d 2ωdk 2

A 2-CW 600THz cavity has zero total momentum p, but each photon adds a tiny mass Mγ to it.

Mγ=ω/c2=ω (1.2·10-51)kg·s= 4.5·10-36kg (for: ω = 2π·600THz )

A 1-CW state has no rest mass, but 1-photon momentum is a non-zero value pγ=Mγ c. (Galilean revemge II.)

pγ=k=ω/c=ω (4.5·10-43)kg·m=1.7·10-27kg·m·s-1 (for: ω = 2π·600THz )

23Tuesday, April 3, 2012

Page 24: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Mrest(γ)=0 Mmom(γ)=p/c=k/c=ω/c2 Meff(γ)=∞

Equations (4.11) in Unit 2

Three kinds of mass for photon γ in CW relativistic theory What’s the matter with light?

(1)Einstein rest mass (2) Galilean momentum mass (3) Newtonian inertial mass Mrest= Mmom=p/u= Meff=F/a=

ω proper

c2

kdωdk

d 2ωdk 2

A 2-CW 600THz cavity has zero total momentum p, but each photon adds a tiny mass Mγ to it.

Mγ=ω/c2=ω (1.2·10-51)kg·s= 4.5·10-36kg (for: ω = 2π·600THz )

A 1-CW state has no rest mass, but 1-photon momentum is a non-zero value pγ=Mγ c. (Galilean revemge II.)

pγ=k=ω/c=ω (4.5·10-43)kg·m=1.7·10-27kg·m·s-1 (for: ω = 2π·600THz )

24Tuesday, April 3, 2012

Page 25: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Mrest(γ)=0 Mmom(γ)=p/c=k/c=ω/c2 Meff(γ)=∞

Equations (4.11) in Unit 2

Three kinds of mass for photon γ in CW relativistic theory What’s the matter with light?

(1)Einstein rest mass (2) Galilean momentum mass (3) Newtonian inertial mass Mrest= Mmom=p/u= Meff=F/a=

ω proper

c2

kdωdk

d 2ωdk 2

A 2-CW 600THz cavity has zero total momentum p, but each photon adds a tiny mass Mγ to it.

Mγ=ω/c2=ω (1.2·10-51)kg·s= 4.5·10-36kg (for: ω = 2π·600THz )

A 1-CW state has no rest mass, but 1-photon momentum is a non-zero value pγ=Mγ c. (Galilean revemge II.)

pγ=k=ω/c=ω (4.5·10-43)kg·m=1.7·10-27kg·m·s-1 (for: ω = 2π·600THz )

25Tuesday, April 3, 2012

Page 26: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

26Tuesday, April 3, 2012

Page 27: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Bohr-Schrodinger (BS) approximation throws out Mc2

E =Mc2

1− u2 / c2= Mc2 coshρ = Mc2 1+ sinh2 ρ = Mc2( )2 + cp( )2

E = Mc2( )2 + cp( )2⎡

⎣⎢

⎦⎥1/2

≈ Mc2 + 12M

p2 BS−approx⎯ →⎯⎯⎯⎯12M

p2

The BS claim: may shift energy origin (E=Mc2, cp=0) to (E=0, cp=0). (Frequency is relative!)

cp'=hck'cctt

cctt''

EnergyE=hω

Momentumcp=hck

Mc2

ωm=49ω1

76543210-1-2-3-4-4-6m

36

251694

(a) Einstein-Planck Dispersion

(b) DeBroglie-Bohr Dispersion

E'=hω'E2 - c2p2 =(Mc2)2

photon: M=0E = c p

E = p2/2M

E = B m2

tachyon:

Bohr - Schrodinger Dispersion

Einstein - Planck Dispersion

=dkdω

Group velocity u=Vgroup is a differential quantity unaffected by origin shift.

Phase velocity =Vphase is greatly reduced by deleting Mc2 from E=ω.

It slows from Vphase=c2/u to a sedate sub-luminal speed of Vgroup/2.

ω BS (k) = k 2

2M gives: v phase=

ω BS

k= k

2M

and: vgroup=dω BS

dk= kM

27Tuesday, April 3, 2012

Page 28: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Bohr-Schrodinger (BS) approximation throws out Mc2

E =Mc2

1− u2 / c2= Mc2 coshρ = Mc2 1+ sinh2 ρ = Mc2( )2 + cp( )2

E = Mc2( )2 + cp( )2⎡

⎣⎢

⎦⎥1/2

≈ Mc2 + 12M

p2 BS−approx⎯ →⎯⎯⎯⎯12M

p2

The BS claim: may shift energy origin (E=Mc2, cp=0) to (E=0, cp=0). (Frequency is relative!)

cp'=hck'cctt

cctt''

EnergyE=hω

Momentumcp=hck

Mc2

ωm=49ω1

76543210-1-2-3-4-4-6m

36

251694

(a) Einstein-Planck Dispersion

(b) DeBroglie-Bohr Dispersion

E'=hω'E2 - c2p2 =(Mc2)2

photon: M=0E = c p

E = p2/2M

E = B m2

tachyon:

Bohr - Schrodinger Dispersion

Einstein - Planck Dispersion

=dkdω

Group velocity u=Vgroup is a differential quantity unaffected by origin shift.

Phase velocity =Vphase is greatly reduced by deleting Mc2 from E=ω.

It slows from Vphase=c2/u to a sedate sub-luminal speed of Vgroup/2.

ω BS (k) = k 2

2M gives: v phase=

ω BS

k= k

2M

and: vgroup=dω BS

dk= kM

28Tuesday, April 3, 2012

Page 29: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

=dkdω

Group velocity u=Vgroup is a differential quantity unaffected by origin shift.

But, Phase velocity =Vphase is greatly reduced by deleting Mc2 from E=ω.

It slows from Vphase=c2/u to a sedate sub-luminal speed of Vgroup/2.

Bohr-Schrodinger (BS) approximation throws out Mc2

E =Mc2

1− u2 / c2= Mc2 coshρ = Mc2 1+ sinh2 ρ = Mc2( )2 + cp( )2

E = Mc2( )2 + cp( )2⎡

⎣⎢

⎦⎥1/2

≈ Mc2 + 12M

p2 BS−approx⎯ →⎯⎯⎯⎯12M

p2

The BS claim: may shift energy origin (E=Mc2, cp=0) to (E=0, cp=0). (Frequency is relative!)

cp'=hck'cctt

cctt''

EnergyE=hω

Momentumcp=hck

Mc2

ωm=49ω1

76543210-1-2-3-4-4-6m

36

251694

(a) Einstein-Planck Dispersion

(b) DeBroglie-Bohr Dispersion

E'=hω'E2 - c2p2 =(Mc2)2

photon: M=0E = c p

E = p2/2M

E = B m2

tachyon:

Bohr - Schrodinger Dispersion

Einstein - Planck Dispersion

ω BS (k) = k 2

2M gives: v phase=

ω BS

k= k

2M

and: vgroup=dω BS

dk= kM

29Tuesday, April 3, 2012

Page 30: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

=dkdω

Group velocity u=Vgroup is a differential quantity unaffected by origin shift.

But, Phase velocity =Vphase is greatly reduced by deleting Mc2 from E=ω.

It slows from Vphase=c2/u to a sedate sub-luminal speed of Vgroup/2.

Bohr-Schrodinger (BS) approximation throws out Mc2

E =Mc2

1− u2 / c2= Mc2 coshρ = Mc2 1+ sinh2 ρ = Mc2( )2 + cp( )2

E = Mc2( )2 + cp( )2⎡

⎣⎢

⎦⎥1/2

≈ Mc2 + 12M

p2 BS−approx⎯ →⎯⎯⎯⎯12M

p2

The BS claim: may shift energy origin (E=Mc2, cp=0) to (E=0, cp=0). (Frequency is relative!)

cp'=hck'cctt

cctt''

EnergyE=hω

Momentumcp=hck

Mc2

ωm=49ω1

76543210-1-2-3-4-4-6m

36

251694

(a) Einstein-Planck Dispersion

(b) DeBroglie-Bohr Dispersion

E'=hω'E2 - c2p2 =(Mc2)2

photon: M=0E = c p

E = p2/2M

E = B m2

tachyon:

Bohr - Schrodinger Dispersion

Einstein - Planck Dispersion

ω BS (k) = k 2

2M gives: Vphase=

ω BS

k= k

2M

and: Vgroup=dω BS

dk= kM

30Tuesday, April 3, 2012

Page 31: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

31Tuesday, April 3, 2012

Page 32: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

(a) Hamiltonian

Momentum p

PP′

P′′

-L-L′-L′′

L(q,q)

Velocity u=q

QQ′Q′′

-H

-H′

-H′′

HH′

H′′LL′L′′

H

H′

H′′

slope:

slope:

∂H∂p

= q= u

∂L∂q

= p

(b) LagrangianH(q,p)

radius = Mc2

O

O

Light cone u=1=chas infiniteH

and zero L

Fig. 5.1. Geometry of contact transformation between relativistic (a) Hamiltonian (b) Lagrangian

Deriving relativistic quantum Lagrangian-Hamiltonian relations

dΦ = kdx − ω dt= −µ dτ = -(Mc2/) dτ. dτ = dt √(1-u2/c2)=dt sech ρ

Differential action: is Planck scale times differential phase: dS = dΦ

For constant u the Lagrangian is: L =−µτ = -Mc2√(1-u2/c2)= -Mc2sech ρ = -Mc2

Start with phase and set k=0 to get product of proper frequency and proper timeΦ µ = Mc2/ τ

dS = Ldt = p·dx − H·dt = k·dx − ω ·dt = dΦ

cosσ

32Tuesday, April 3, 2012

Page 33: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

(a) Hamiltonian

Momentum p

PP′

P′′

-L-L′-L′′

L(q,q)

Velocity u=q

QQ′Q′′

-H

-H′

-H′′

HH′

H′′LL′L′′

H

H′

H′′

slope:

slope:

∂H∂p

= q= u

∂L∂q

= p

(b) LagrangianH(q,p)

radius = Mc2

O

O

Light cone u=1=chas infiniteH

and zero L

Fig. 5.1. Geometry of contact transformation between relativistic (a) Hamiltonian (b) Lagrangian

Deriving relativistic quantum Lagrangian-Hamiltonian relations

dΦ = kdx − ω dt= −µ dτ = -(Mc2/) dτ. dτ = dt √(1-u2/c2)=dt sech ρ

Differential action: is Planck scale times differential phase: dS = dΦ

For constant u the Lagrangian is: L =−µτ = -Mc2√(1-u2/c2)= -Mc2sech ρ = -Mc2

Start with phase and set k=0 to get product of proper frequency and proper timeΦ µ = Mc2/ τ

cosσ

dS = Ldt = p·dx − H·dt = k·dx − ω ·dt = dΦ

33Tuesday, April 3, 2012

Page 34: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

(a) Hamiltonian

Momentum p

PP′

P′′

-L-L′-L′′

L(q,q)

Velocity u=q

QQ′Q′′

-H

-H′

-H′′

HH′

H′′LL′L′′

H

H′

H′′

slope:

slope:

∂H∂p

= q= u

∂L∂q

= p

(b) LagrangianH(q,p)

radius = Mc2

O

O

Light cone u=1=chas infiniteH

and zero L

Fig. 5.1. Geometry of contact transformation between relativistic (a) Hamiltonian (b) Lagrangian

Deriving relativistic quantum Lagrangian-Hamiltonian relations

dΦ = kdx − ω dt= −µ dτ = -(Mc2/) dτ. dτ = dt √(1-u2/c2)=dt sech ρ

Differential action: is Planck scale times differential phase: dS = dΦ

For constant u the Lagrangian is: L =−µτ = -Mc2√(1-u2/c2)= -Mc2sech ρ = -Mc2

Start with phase and set k=0 to get product of proper frequency and proper timeΦ µ = Mc2/ τ

cosσ

dS = Ldt = p·dx − H·dt = k·dx − ω ·dt = dΦ

34Tuesday, April 3, 2012

Page 35: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

(a) Hamiltonian

Momentum p

PP′

P′′

-L-L′-L′′

L(q,q)

Velocity u=q

QQ′Q′′

-H

-H′

-H′′

HH′

H′′LL′L′′

H

H′

H′′

slope:

slope:

∂H∂p

= q= u

∂L∂q

= p

(b) LagrangianH(q,p)

radius = Mc2

O

O

Light cone u=1=chas infiniteH

and zero L

Fig. 5.1. Geometry of contact transformation between relativistic (a) Hamiltonian (b) Lagrangian

Deriving relativistic quantum Lagrangian-Hamiltonian relations

dΦ = kdx − ω dt= −µ dτ = -(Mc2/) dτ. dτ = dt √(1-u2/c2)=dt sech ρ

Differential action: is Planck scale times differential phase: dS = dΦ

For constant u the Lagrangian is: L =−µτ = -Mc2√(1-u2/c2)= -Mc2sech ρ = -Mc2

Start with phase and set k=0 to get product of proper frequency and proper timeΦ µ = Mc2/ τ

dS = Ldt = p·dx − H·dt = k·dx − ω ·dt = dΦ

cosσ

L= p· x − H = p·u − H...with Poincare invariant:

35Tuesday, April 3, 2012

Page 36: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

36Tuesday, April 3, 2012

Page 37: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Fig. 5.2 “True” paths carry extreme phase and fastest clocks. Light-cone has only stopped clocks.

Fig. 5.3 Quantum waves interfere constructively on “True” path but mostly cancel elsewhere.

Feynman’s flying clock and phase minimization

37Tuesday, April 3, 2012

Page 38: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

Group vs. phase velocity and tangent contacts Reviewing “Sin-Tan Rosetta” geometry

How optical CW group and phase properties give relativistic mechanics Three kinds of mass (Einstein rest mass, Galilean momentum mass, Newtonian inertial mass)

What’s the matter with light? Bohr-Schrodinger (BS) approximation throws out Mc2

Deriving relativistic quantum Lagrangian-Hamiltonian relationsFeynman’s flying clock and phase minimization

Geometry of relativistic mechanics

Relativistic Classical and Quantum Mechanics

38Tuesday, April 3, 2012

Page 39: Lecture 26. Introduction to Relativistic Classical and ......2012/04/03  · Lecture 26. Introduction to Relativistic Classical and Quantum Mechanics (Ch. 2-5 of Unit 2 4.03.12) Group

ρ

ρHHaammiillttoonniiaann ==HH ==BB ccoosshh ρ

--LLaaggrraannggiiaann

--LL ==BB sseecchh ρRReesstt

EEnneerrggyy

BB ==MMcc22

HH

BB

--LL

VVeelloocciittyy aabbeerrrraattiioonn

aannggllee φ

33−

433221100--11

4

--22

BB ccoosshh ρ

BB ee--ρcp

H=E

BB

BB ee++ρ

BB sseecchh ρ

22

11

BBlluuee sshhiiffttRReedd sshhiifftt

(a) Geometry of relativistic transformationand wave based mechanics

(b) Tangent geometry (u/c=3/5)

(c) Basic construction given u/c=45/53

u/c =3/5u/c =1

cp =3/4

H =5/4

-L =4/5

cp =45/28

H =53/28

-L=28/45

e-ρ=1/2e-ρ=2/7

(d) u/c=3/5

11

1 1

bb--cciirrccllee

g-circle

p-circle

Fig. 5.5 Relativistic wave mechanics geometry. (a) Overview.

(b-d) Details of contacting tangents.

39Tuesday, April 3, 2012