## This Week's Finds in Mathematical Physics (Week 33)

#### John Baez

With tremendous relief, I have finished writing a book, and will return to putting out This Week's Finds on a roughly weekly basis. Let me briefly describe my book, which took so much more work than I had expected... and then let me start catching up on listing some of the stuff that's cluttering my desk!

1) Gauge Fields, Knots and Gravity, by John Baez and Javier de Muniain, World Scientific Press, to appear in summer 1994.

This book is based on a seminar I taught in 1992-93. We start out assuming the reader is familiar with basic stuff - Maxwell's equations, special relativity, linear algebra and calculus of several variables - and try to prepare the reader to understand recent work on quantum gravity and its relation to knot theory. It proved difficult to do this well in a mere 460 pages. Lots of tantalizing loose ends are left dangling. However, there are copious references so that the reader can pursue various subjects further.

```Part 1.    Electromagnetism

Chapter 1. Maxwell's Equations
Chapter 2. Manifolds
Chapter 3. Vector Fields
Chapter 4. Differential Forms
Chapter 5. Rewriting Maxwell's Equations
Chapter 6. DeRham Theory in Electromagnetism

Part 2.    Gauge Fields

Chapter 1. Symmetry
Chapter 2. Bundles and Connections
Chapter 3. Curvature and the Yang-Mills Equations
Chapter 4. Chern-Simons Theory
Chapter 5. Link Invariants from Gauge Theory

Part 3.    Gravity

Chapter 1. Semi-Riemannian Geometry
Chapter 2. Einstein's Equations
Chapter 3. Lagrangians for General Relativity
Chapter 4. The ADM Formalism
Chapter 5. The New Variables
```

2) Quantum Theory: Concepts and Methods, by Asher Peres, Kluwer Academic Publishers, 1994.

As Peres notes, there are many books that teach students how to solve quantum mechanics problems, but not many that tackle the conceptual puzzles that fascinate those interested in the foundations of the subject. His book aims to fill this gap. Of course, it's impossible not to annoy people when writing about something so controversial; for example, fans of Everett will be distressed that Peres' book contains only a brief section on "Everett's interpretation and other bizarre interpretations". However, the book is clear-headed and discusses a lot of interesting topics, so everyone should take a look at it.

Schroedinger's cat, Bell's inequality and Wigner's friend are old chestnuts that everyone puzzling over quantum theory has seen, but there are plenty of popular new chestnuts in this book too, like "quantum cryptography", "quantum teleportation", and the "quantum Zeno effect", all of which would send shivers up and down Einstein's spine. There are also a lot of gems that I hadn't seen, like the Wigner-Araki-Yanase theorem. Let me discuss this theorem a bit.

Roughly, the WAY theorem states that it is impossible to measure an operator that fails to commute with an additive conserved quantity. Let me give an example to clarify this and then give the proof. Say we have a particle with position q and momentum p, and a measuring apparatus with position Q and momentum P. Let's suppose that the total momentum p + P is conserved - which will typically be the case if we count as part of the "apparatus" everything that exerts a force on the particle. Then as a consequence of the WAY theorem we can see that (in a certain sense) it is impossible to measure the particle's position q; all we can measure is its position relative to the apparatus, q - Q.

Of course, whenever a "physics theorem" states that something is impossible one must peer into it and determine the exact assumptions and the exact result! Lots of people have gotten in trouble by citing theorems that seem to show something is impossible without reading the fine print. So let's see what the WAY theorem really says!

It assumes that the Hilbert space for the system is the tensor product of the Hilbert space for the thing being observed - for short, let's call it the "particle" - and the Hilbert space for the measuring apparatus. Assume also that A and B are two observables belonging to the observed system, while C is an observable belonging to the measuring apparatus; suppose that B + C is conserved, and let's try to show that we can only measure A if it commutes with B. (Our assumptions automatically imply that A commutes with C, by the way.)

So, what do we mean when we speak of "measuring A"? Well, there are various things one might mean. The simplest is that if we start the combined system in some tensor product state u(i) ⊗ v, where v is the "waiting and ready" state of the apparatus and u(i) is a state of the observed system that's an eigenvector of A:

Au(i) = a(i)u(i),

then the unitary operator U corresponding to time evolution does the following:

U(u(i) ⊗ v) = u(i) ⊗ v(i)

where the state v(i) of the apparatus is one in which it can be said to have measured the observable A to have value a(i). E.g., the apparatus might have a dial on it, and in the state v(i) the dial reads "a(i)". Of course, we are really only justified in saying a measurement has occured if the states v(i) are distinct for different values of i.

Note: here the WAY theorem seems to be restricting itself to nondestructive measurements, since the observed system is remaining in the state u(i). If you go through the proof you can see to what extent this is crucial, and how one might modify the theorem if this is not the case.

Okay, we have to show that we can only "measure A" in this sense if A commutes with B. We are assuming that B + C is conserved, i.e.,

U*(B + C)U = B + C.

First note that

<u(i), [A,B] u(j)> = (a(i) - a(j)) <u(i), Bu(j)>.

On the other hand, since A and B only act on the Hilbert space for the particle, we also have

```<u(i), [A,B] u(j)> = <u(i) ⊗ v, [A,B] u(j) ⊗ v>

= <u(i) ⊗ v, [A,B+C] u(j) ⊗ v>

= (a(i) - a(j))  <u(i) ⊗ v, (B+C) u(j) ⊗ v>.
```

It follows that if a(i) - a(j) isn't zero,

```<u(i), Bu(j)> = <u(i) ⊗ v, (B+C) u(j) ⊗ v>

= <u(i) ⊗ v, U*(B + C)U u(j) ⊗ v>

= <u(i) ⊗ v(i), (B + C) u(j) ⊗ v(j)>

= <u(i), Bu(j)> <v(i), v(j)> + <u(i), u(j)> <v(i), C v(j)>
```

but the second term vanishes since u(i) are a basis of eigenvectors and u(i) and u(j) correspond to different eigenvalues, so

<u(i), Bu(j)> = <u(i), Bu(j)> <v(i), v(j)>

which means that either <v(i), v(j)> = 1, hence v(i) = v(j) (since they are unit vectors), so that no measurement has really been done, OR that <u(i), B u(j)> = 0, which means (if true for all i,j) that A commutes with B.

So, we have proved the result, using one extra assumption that I didn't mention at the start, namely that the eigenvalues a(i) are distinct.

I can't say that I really understand the argument, although it's easy enough to follow the math. I will have to ponder it more, but it is rather interesting, because it makes more precise (and general) the familiar notion that one can't measure absolute positions, due to the translation-invariance of the laws of physics; this translation invariance is of course what makes momentum be conserved. (What I just wrote makes me wonder if someone has shown a classical analog of the WAY theorem.)

```Chapter 1: Introduction to Quantum Physics

1-1. The downfall of classical concepts                             3
1-2. The rise of randomness                                         5
1-3. Polarized photons                                              7
1-4. Introducing the quantum language                               9
1-5. What is a measurement?                                        14
1-6. Historical remarks                                            18
1-7. Bibliography                                                  21

Chapter 2: Quantum Tests

2-1. What is a quantum system?                                      24
2-2. Repeatable tests                                               27
2-3. Maximal quantum tests                                          29
2-4. Consecutive tests                                              33
2-5. The principle of interference                                  36
2-6. Transition amplitudes                                          39
2-7. Appendix: Bayes's rule of statistical inference                45
2-8. Bibliography                                                   47

Chapter 3: Complex Vector Space

3-1. The superposition principle                                    48
3-2. Metric properties                                              51
3-3. Quantum expectation rule                                       54
3-4. Physical implementation                                        57
3-5. Determination of a quantum state                               58
3-6. Measurements and observables                                   62
3-7. Further algebraic properties                                   67
3-8. Quantum mixtures                                               72
3-9. Appendix: Dirac's notation                                     77
3-10. Bibliography                                                  78

Chapter 4: Continuous Variables

4-1. Hilbert space                                                  79
4-2. Linear operators                                               84
4-3. Commutators and uncertainty relations                          89
4-4. Truncated Hilbert space                                        95
4-5. Spectral theory                                                99
4-6. Classification of spectra                                     103
4-7. Appendix: Generalized functions                               106
4-8. Bibliography                                                  112

Chapter 5: Composite Systems

5-1. Quantum correlations                                          115
5-2. Incomplete tests and partial traces                           121
5-3. The Schmidt decomposition                                     123
5-4. Indistinguishable particles                                   126
5-5. Parastatistics                                                131
5-6. Fock space                                                    137
5-7. Second quantization                                           142
5-8. Bibliography                                                  147

Chapter 6: Bell's Theorem

6-1. The dilemma of Einstein, Podolsky, and Rosen                  148
6-2. Cryptodeterminism                                             155
6-3. Bell's inequalities                                           160
6-4. Some fundamental issues                                       167
6-5. Other quantum inequalities                                    173
6-6. Higher spins                                                  179
6-7. Bibliography                                                  185

Chapter 7: Contextuality

7-1. Nonlocality versus contextuality                              187
7-2. Gleason's theorem                                             190
7-3. The Kochen-Specker theorem                                    196
7-4. Experimental and logical aspects of inseparability            202
7-5. Appendix: Computer test for Kochen-Specker contradiction      209
7-6. Bibliography                                                  211

Chapter 8: Spacetime Symmetries

8-1. What is a symmetry?                                           215
8-2. Wigner's theorem                                              217
8-3. Continuous transformations                                    220
8-4. The momentum operator                                         225
8-5. The Euclidean group                                           229
8-6. Quantum dynamics                                              237
8-7. Heisenberg and Dirac pictures                                 242
8-8. Galilean invariance                                           245
8-9. Relativistic invariance                                       249
8-10. Forms of relativistic dynamics                               254
8-11. Space reflection and time reversal                           257
8-12. Bibliography                                                 259

Chapter 9: Information and Thermodynamics

9-1. Entropy                                                       260
9-2. Thermodynamic equilibrium                                     266
9-3. Ideal quantum gas                                             270
9-4. Some impossible processes                                     275
9-5. Generalized quantum tests                                     279
9-6. Neumark's theorem                                             285
9-7. The limits of objectivity                                     289
9-8. Quantum cryptography and teleportation                        293
9-9. Bibliography                                                  296

Chapter 10: Semiclassical Methods

10-1. The correspondence principle                                 298
10-2. Motion and distortion of wave packets                        302
10-3. Classical action                                             307
10-4. Quantum mechanics in phase space                             312
10-5. Koopman's theorem                                            317
10-6. Compact spaces                                               319
10-7. Coherent states                                              323
10-8. Bibliography                                                 330

Chapter 11: Chaos and Irreversibility

11-1. Discrete maps                                                332
11-2. Irreversibility in classical physics                         341
11-3. Quantum aspects of classical chaos                           347
11-4. Quantum maps                                                 351
11-5. Chaotic quantum motion                                       353
11-6. Evolution of pure states into mixtures                       369
11-7. Appendix: PostScript code for a map                          370
11-8. Bibliography                                                 371

Chapter 12: The Measuring Process

12-1. The ambivalent observer                                      373
12-2. Classical measurement theory                                 378
12-3. Estimation of a static parameter                             385
12-4. Time-dependent signals                                       387
12-5. Quantum Zeno effect                                          392
12-6. Measurements of finite duration                              400
12-7. The measurement of time                                      405
12-8. Time and energy complementarity                              413
12-9. Incompatible observables                                     417
12-10. Approximate reality                                         423
12-11. Bibliography                                                428
```

3) Loop representations, by Bernd Bruegmann, Max Planck Institute preprint, available as gr-qc 9312001.

This is a nice review article on loop representations of gauge theories. Anyone wanting to jump into the loop representation game would be well advised to start here.

4) The fate of black hole singularities and the parameters of the standard models of particle physics and cosmology, by Lee Smolin, available in LaTeX format as gr-qc/9404011.

This is about Smolin's "evolutionary cosmology" scenario, which I already discussed in week31. Let me just quote the abstract:

A cosmological scenario which explains the values of the parameters of the standard models of elementary particle physics and cosmology is discussed. In this scenario these parameters are set by a process analogous to natural selection which follows naturally from the assumption that the singularities in black holes are removed by quantum effects leading to the creation of new expanding regions of the universe. The suggestion of J. A. Wheeler that the parameters change randomly at such events leads naturally to the conjecture that the parameters have been selected for values that extremize the production of black holes. This leads directly to a prediction, which is that small changes in any of the parameters should lead to a decrease in the number of black holes produced by the universe. On plausible astrophysical assumptions it is found that changes in many of the parameters do lead to a decrease in the number of black holes produced by spiral galaxies. These include the masses of the proton, neutron, electron and neutrino and the weak, strong and electromagnetic coupling constants. Finally,this scenario predicts a natural time scale for cosmology equal to the time over which spiral galaxies maintain appreciable rates of star formation, which is compatible with current observations that Ω = .1-.2

© 1994 John Baez
baez@math.removethis.ucr.andthis.edu