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20 - Introduction

from Part 3 - String theory

Michael Dine
Affiliation:
University of California, Santa Cruz
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Summary

String theory was stumbled on, more or less, by accident. In the late 1960s, string theories were first proposed as theories of the strong interactions. It was quickly realized, however, that, while hadronic physics has a number of string-like features, string theories were not suitable for a detailed description. In their simplest form, string theories have massless spin-2 particles and more than four dimensions of space–time, hardly features of the strong interactions. But a small group of theorists appreciated that the presence of a spin-2 particle implied that these theories were generally covariant and explored them through the 1970s and early 1980s, as possible theories of quantum gravity. Like field theories, the number of possible string theories seemed to be infinite, while, unlike field theories, there was reason to believe that these theories did not suffer from ultraviolet divergences. In the 1980s, however, studies of anomalies in higher dimensions suggested that all string theories with chiral fermions and gauge interactions suffered from quantum anomalies. But in 1984 it was shown that the anomalies cancel for two choices of gauge group. It was quickly recognized that the non-anomalous string theories do come close to unifying gravity and the Standard Model of particle physics. Many questions remained. Beginning in 1995, great progress was made in understanding the deeper structure of these theories. All the known string theories were understood to be different limits of some larger structure. As string theories still provide the only framework in which one can do systematic computations of quantum gravity effects, many workers use the term “string theory” to refer to some underlying structure which unifies quantum mechanics, gravity and gauge interactions.

String theory has provided us with many insights into what a fundamental theory of gravity and gauge interactions might look like, but there is still much we do not understand. We cannot really begin a course of action by enunciating some great principle and seeing what follows. We might, for example, have imagined that the underlying theory would be a string field theory, whose basic objects would create and annihilate strings. Some set of organizing principles would determine the action for this system, and the rest would be a problem of working out the consequences.

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Supersymmetry and String Theory
Beyond the Standard Model
, pp. 289 - 294
Publisher: Cambridge University Press
Print publication year: 2016

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  • Introduction
  • Michael Dine, University of California, Santa Cruz
  • Book: Supersymmetry and String Theory
  • Online publication: 18 December 2015
  • Chapter DOI: https://doi.org/10.1017/CBO9781107261426.023
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  • Introduction
  • Michael Dine, University of California, Santa Cruz
  • Book: Supersymmetry and String Theory
  • Online publication: 18 December 2015
  • Chapter DOI: https://doi.org/10.1017/CBO9781107261426.023
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Introduction
  • Michael Dine, University of California, Santa Cruz
  • Book: Supersymmetry and String Theory
  • Online publication: 18 December 2015
  • Chapter DOI: https://doi.org/10.1017/CBO9781107261426.023
Available formats
×