utrecht university gerard ’t hooft and isaac newton institute, december 15, 2004

25
Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Upload: magdalen-oliver

Post on 18-Jan-2018

228 views

Category:

Documents


0 download

DESCRIPTION

The use of Hilbert Space Techniques as technical devices for the treatment of the statistics of chaos... A “state” of the universe: A simple model universe: Diagonalize:

TRANSCRIPT

Page 1: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Utrecht University

Gerard ’t Hooft

and

Isaac Newton Institute, December 15, 2004

Page 2: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Conventional QuantumMechanics

Deterministic QuantumMechanics

All choices of basisare equivalent

There is a preferred

basis

The rules for physical calculations are identical

Locality applies tocommutators

outsidethe light cone

Locality can only be

understood in this basis

Gauge equivalence classes of states

Ontological equivalence classes

Page 3: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

The use of Hilbert Space Techniques as technical

devices for the treatment of the statistics of chaos ...

, ... , , ..., , ..., , anything ... x p i í ýA “state” of the universe:

A simple model universe: í 1ý í 2ý í 3ý í 1ý

Diagonalize:

0 0 11 0 00 1 0

U2 2 2

1 2 3, , P P P

;321

iH

i

i ee

eU

3/2

3/2

1

Page 4: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

02 / 3

2 / 3H p

p

æ ö÷ç ÷ç ÷ç ÷ç ÷® -ç ÷÷ç ÷ç ÷ç ÷+ ÷çè ø

(An atom in a magnetic field)

An operator that is diagonal in the primordial basis, is a BEABLE .

1[ ] 0

2 ; all all , '

3t t

(t) , '(t')

, O O O O

11

1

Other operators such as H, or:

are CHANGEABLES

In the original basis:

Page 5: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Deterministic evolution ofcontinuous degrees of freedom:

( ) ( )i id q t f qdt

( )ii

i

H p f q iip qi

but, … this H is not bounded from below !

Page 6: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

The harmonic oscillatorTheorem: its Hilbert Space is that ofa particle moving along a circle

H

?

Page 7: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Our assignment: Find the true beables of our world!

Beables can be identified for:

An atom in a magnetic field

Second quantized MASSLESS, NON-INTERACTING “neutrinos”

Free scalar bosons

Free Maxwell photons

Page 8: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Beables for the first quantized neutrino:

, i j ijk k ijH p i Is s s e s d= × = +rr

ˆ ˆ ˆ{ , , } ,tp p p x (t)O

) 0ˆ ( , ˆ where xi

i pppp

ˆ ˆ ˆ( ) (0) ; ( ) (0) ˆ ˆ ˆ ˆ( ) (0) , ( ) (0)x t x t p x t p x p tp t p p t p

s ss s

= + × = × + ×= × = ×

r r r rr rr r

0 ˆ ˆ]ˆ ,ˆ[ ii p

ppipxp

1ˆp

Page 9: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

But, single “neutrinos” have

!!! 0 ,

HpH

Dirac’s second quantization:H

0}empty

}fullBut a strict discussionrequires a cut-off for every orientation of :p̂

But, how do we introduce mass?How do we introduce interactions?How do the “flat membranes” behave in curved space-time ?

Page 10: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

A key ingredient for an ontological theory: Information loss

Introduce equivalence classes

í 1ý,í 4ý í 2ý í 3ý

Page 11: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Neutrinos aren’t sheets ...They are equivalence classes

p̂There is an ontological position x , as well asan orientation for themomentum.

The velocity in the directionis c , but there is “random”, or“Brownian” motion in the transversedirection.

Note: v c>

Page 12: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Two coupled degrees of freedom

Page 13: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Does dissipation help to produce a lower bound to the Hamiltonian ?

Consider first the harmonic oscillator:The deterministic case: write

. . , . [ , ] , [ , ]x yx y y x x p i y p i= = - = =

yx xpypH

212

22

2212

12

121

2412

412

412

41

)()(

)()()()(

HHQPQP

xpxpypypH yyxx

22222121 , , , xp

PpyQypPpx

Q yxxy

Page 14: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

0 ] , [ , 2121 HHHHH

. H , 2 2P , 2

, , 22

11

21

2

yxypxQ

pxpyH

x

yx

Important to note: The Hamiltonian nearly coincides with theClassical conserved quantity 22 yx

We now impose a constraint (caused by information loss?)

Two independent QUANTUM harmonic oscillators!

Page 15: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

This oscillator has two conserved quantities:†

2 2 2 ; ( )

; [ , ] 0 ; [ , ] 0 .x yD xp yp i D D

x y H D Hr r

º + - =º + = =

22 21 1 11,2 4 4( ) ( )H H D ir rr= ± + +Write

Alternatively, one may simply remove the last part, and write 2

2 0 H H r= ® =

Or, more generally:2 , where is a conserved quantity.H ra a=

Then, the operator D is no longer needed.

Page 16: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Compare the Hamiltonian for a (static)black hole.

III HHH We only “see” universe # I.

Information to and from universe II is lost.We may indeed impose the constraint:

12 is equivalent to " ". only.II IH H H

Page 17: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

But, even in a harmonic oscillator, this lock-in isdifficult to realize in a model.

Projecting onto states with can only happen if there is information loss.

H U

The “classical quantization” of energy:

;ine tH n

U k n

k

Let H be the Hamiltonian and U be an ontological energy function.

Page 18: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

This way, one can also get into grips with the anharmonic oscillator.

Since H must obey T

nH 2

where T is the period of the (classical) motion,we get that only special orbits are allowed.

Here, information loss sets in. The special orbitsare the stable limit cycles!

If T is not independent of , then the allowed values of H are not equidistant, as in a genuine anharmonic oscillator.

rnE

Page 19: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

The perturbed oscillator has discretizedstable orbits. This is what causes quantization.

Page 20: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

A deterministic “universe” may showPOINCARÉ CYCLES:

Equivalence classes form pure cycles:

Gen. Relativity: time is a gauge parameter !

Dim( ) = # different Poincaré cycles

0 fixed , EEH

Heisenberg Picture: fixed.

Page 21: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

For black holes, the equivalence classes are very large!

Page 22: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

The black hole as an information processing machine

65 2

One bit ofinformationon every

cm0 724 10 -.

These statesare alsoequivalence

classes.The ontologicalstates are inthe bulk !!

Page 23: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

The cellular automaton

Page 24: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

Suppose: ★ a theory of ubiquitous fluctuating variables ★ not resembling particles, or fields ... Suppose: ★ that what we call particles and fields are actually complicated statistical features of said theory ...

One would expect ★ statistical features very much as in QM

(although more probably resembling Brownian motion etc.

★ Attempts to explain the observations in ontological terms would also fail, unless

we’d hit upon exactly the right theory ...

Page 25: Utrecht University Gerard ’t Hooft and Isaac Newton Institute, December 15, 2004

dobbelgod