PART I
Introduction
CHAPTER 1
General Introduction
EVERETT AND HIS PROJECT
In July 2007, Nature celebrated the half-centenary of the âmany worldsâ interpretation of quantum mechanics with a splashy cover and a series of explanatory articles. That year, there were two international conferences dedicated to dissecting Hugh Everett IIIâs claim that the universe is completely quantum mechanical.1 Although the theorist had been dead for a quarter century, his controversial theory was alive and kicking.
First published in Reviews of Modern Physics in 1957 as âThe âRelative Stateâ Formulation of Quantum Mechanics,â the theory was not labeled âmany worldsâ until 1970, and then, not by Everett, but by his enthusiastic supporter, physicist Bryce S. DeWitt. Today, the Everett interpretation is one of a handful of contenders for explaining the structure of the quantum universeâwhether or not its âbranchingâ motion is interpreted as a metaphor for the linear evolution of the universal state or as modeling idealized or ontologically real worlds.
Everett was only 27 years old when he developed his theory, which would become his doctoral dissertation at Princeton. More interested in military game theory than theoretical physics, Everett never published another word on quantum mechanics. And yet his dissertation has stood the test of time and disbelief. Something in Everettâs work has continued to resonate with physicists and philosophers alike so that, despite his many critics, three generations of researchers have returned to Everettâs strange, counterintuitive theory, trying to find language to capture the quantum universe described mathematically by his pure wave mechanics.
This volume presents the two previously published versions of his theory, Everettâs long and short theses, alongside a selected collection of his unpublished works and correspondence, which illuminate how Everett and his contemporaries struggled to answer questions that remain with us today.
Everett developed his interpretation of quantum mechanics, his relative-state formulation of pure wave mechanics, while a graduate student in physics at Princeton University. Matriculating in the fall of 1953, he began writing down his idea a year later. A detailed presentation of the theory, the long thesis, was submitted by Everett to John Archibald Wheeler, his doctoral thesis advisor, in January 1956. It was circulated in April of that year to several prominent physicists, including Niels Bohr.2
The long thesis was Everettâs earlier, more detailed formulation and discussion of his theory, whereas the short thesis was a highly redacted and refocused version of the long thesis, reworked under the direction of Wheeler to soften the force of Everettâs attack on the orthodox Copenhagen interpretation.
The back story is that Wheeler had spent considerable effort in May 1956 trying to convince Niels Bohr and his colleagues at the Institute for Theoretical Physics in Copenhagen, Denmark, that Everettâs work should not be taken as a fatal threat to their understanding of quantum mechanics. His efforts were in vain and, with his doctoral degree in limbo due to Wheelerâs reluctance to accept his long thesis without a nod of approval from Bohr, Everett left Princeton and took a job outside of academics as a military operations researcher in Washington, D.C., in June 1956.
During the winter of 1957, he and Wheeler rewrote the long thesis, cutting about 75 percent of it, to make it, in Wheelerâs phrase, âjavelin proof.â3 Subsequently, Everettâs doctoral thesis (1957a), the short thesis, was accepted in March 1957, and a nearly identical paper (1957b) was published by Reviews of Modern Physics in July of that year. Bryce S. DeWitt and Neill Graham (1973) later published an updated version of Everettâs long thesis in their volume entitled The Many-Worlds Interpretation of Quantum Mechanics.4
Although Everettâs notes and correspondence indicate that he continued to be interested in the conceptual problems of quantum mechanics and in the interpretation and reception of his model of pure wave mechanics, he did not play an active role in the public debates surrounding his theory in the 1970s. He died of a heart attack in 1982 without writing any further systematic presentation of it. For many years, his long and short theses remained the primary evidence for how he had intended his formulation of quantum mechanics to work.
In 2007, the investigative journalist Peter Byrne was invited by Everettâs son, Mark Everett, to open a dozen cardboard boxes that had been stored for many years in his basement. The boxes contained numerous items of scientific interest, including correspondence about the theory with Niels Bohr, Norbert Wiener, Wheeler, and other prominent physicists. Hundreds of pages of handwritten and typed and retyped drafts of the long thesis document Everettâs thought process as he formulated his theory from the fall of 1954 through the winter of 1956. Importantly, three âminipapersâ give an overview of Everettâs basic arguments as of September 1955. This newly discovered material helps to illuminate his previously published work, often in striking ways.
EVERETTâS TARGET: THE MEASUREMENT PROBLEM
In the long thesis, Everett directly attacked both the von NeumannâDirac and the Copenhagen formulations of quantum mechanics. He held that neither orthodox formulation could adequately describe what happened to a physical system when it was measured. Everett believed that the standard von NeumannâDirac collapse formulation of quantum mechanics, the version of the theory found in most textbooks, provided an incomplete and incoherent characterization of measurement and that Bohrâs formulation of the theory, called the Copenhagen interpretation, was even worse since it simply stipulated that the process of measurement could not be understood quantum mechanically. Wheeler, as his thesis advisor, wanted Everett to present his controversial theory in a way that he believed would be more easily received by the physics community. This led to the much shorter thesis that Everett defended for his Ph.D. The short thesis still expressed dissatisfaction with the conventional formulations of quantum mechanics, but it now characterized their inadequacies less as fundamental conceptual flaws and more as roadblocks to applying quantum mechanics to field theories and cosmology.
The problem with the standard collapse theory, according to Everett, was that it required observers always to be treated as external to the system described by the theory, one consequence of which was that it could not be used to provide a consistent physical description of the universe as a whole since the universe contains observers. More specifically, the standard collapse theory has two dynamical laws: one says that physical systems evolve in a linear, deterministic way when not measured, and the other says that physical systems evolve in a nonlinear random way when measured. But since the standard theory does not say what constitutes a measurement, it is at best incomplete. And if one takes measuring devices and observers to be described by the deterministic linear law (and why shouldnât they be insofar as they are constructed of simpler systems that each follow the linear deterministic law?), then the collapse theory is logically inconsistent. This is the notorious quantum measurement problem for the standard textbook formulation of quantum mechanics.
Everett was not alone in his dissatisfaction with the prevailing interpretation of quantum mechanics. Other notable discontents included Erwin Schrödinger, Albert Einstein, Boris Podolsky, Nathan Rosen, and David Bohm. Indeed, Bohm, who left Princeton just before Everett arrived,5 had devised a deterministic âhidden-variableâ formulation of quantum mechanics that addressed the quantum measurement problem and made the same empirical predictions as the conventional formulations for those experiments where they made coherent predictions at all. Everett, however, believed that his simpler approach rendered Bohmâs hidden variables âsuperfluous.â6
Everett tackled the measurement problem by promoting what he called âpure wave mechanics.â7 His formalism characterized the physical state of the universe with a âuniversal wave function,â which describs a superposition of possible classical states that evolves in a perfectly continuous and linear way. This is the simplest possible formulation of quantum mechanics, said Everett, because it entirely avoids the quantum measurement problem, and, unlike most other formulations of quantum mechanics, it can be put in a form that is compatible with the constraints of general relativity. In this sense, it provides an ideal quantum mechanical foundation for modern field theories. Everettâs theory is consequently one of the most popular formulations of quantum mechanics among both physicists and philosophers.
Going further than previous critics of the standard collapse postulate, Everettâs proposed solution to the measurement problem was to drop the random nonlinear dynamics from the standard collapse theory and take the resulting pure wave mechanics, governed by the time-dependent Schrödinger equation alone, as a complete physical theory. His goal was to deduce the empirical predictions of the standard collapse theory as the subjective experiences of observers who are themselves treated as physical systems described by the theory. He referred to pure wave mechanics with the interpretive apparatus provided by his fundamental principle of the relativity of quantum states as the relative-state formulation of quantum mechanics. It is, however, unclear precisely how Everett intended for the relative-state formulation to be understood. There is agreement among those who study Everettâs interpretation of quantum mechanics that his interpretation requires interpretation, and many people have attempted to explain exactly what he had in mind. Indeed, it is fair to say that most no-collapse interpretations of quantum mechanics have at one time or another either been directly attributed to Everett or suggested as charitable reconstructions.8
That said, the various many-worlds formulations of quantum mechanics have proven to be the most popular reconstructions of Everettâs theory. This way of understanding the relative-state formulation is largely due to Bryce DeWittâs energetic promotion in the early 1970s of what he called the EWG theory, for Everett, Wheeler, and DeWittâs student Neill Graham. Whereas Everett himself never mentioned many worlds or parallel universes in either version of his thesis, DeWittâs interpretation of Everett so captured peopleâs imagination that it remains the most popular understanding of Everettâs theory.9 Nonetheless, a half century after the theory was first published, much work continues to be done to formulate a clear and compelling many-worlds interpretation of pure wave mechanics. The most recent many-worlds interpretations characterize worlds as emergent entities that are roughly individuated by decoherence considerations.10
In the end, Everettâs remarkable achievement was in providing a compelling case that pure wave mechanics alone constitutes a complete and accurate physical theory and makes the same empirical predictions as the standard collapse theory. According to him, the quantum measurement problem was simply a misunderstanding generated by unnecessarily adding a postulate that measurement is special to a theory that works without that postulate. Although most researchers believe that Everett was not entirely successful in deriving the standard quantum mechanical predictions from the mathematics of pure wave mechanics alone, he got close enough to motivate many others to try filling in the details in his project. Because of the simplicity of the mathematical formalism, its universal scope, and its other theoretical virtues, the stakes are high in understan...