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Introduction to Cosmic F- and D-Strings

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String Theory: From Gauge Interactions to Cosmology

Part of the book series: NATO Science Series II: Mathematics, Physics and Chemistry ((NAII,volume 208))

Abstract

In these lectures I discuss the possibility that superstrings of cosmic length might exist and be observable. I first review the original idea of cosmic strings arising as gauge theory solitons, and discuss in particular their network properties and the observational bounds that rule out cosmic strings as the principal origin of structure in our universe. I then consider cosmic superstrings, including the ‘fundamental’ F-strings and also D-strings and strings arising from wrapped branes. I discuss the conditions under which these will exist and be observable, and ways in which different kinds of string might be distinguished. We will see that each of these issues is model-dependent, but that some of the simplest models of inflation in string theory do lead to cosmic superstrings. Moreover, these could be the first objects seen in gravitational wave astronomy, and might have distinctive network properties.

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Authors and Affiliations

  1. KITP, University of California, Santa Barbara, CA, USA

    Joseph Polchinski

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  1. Joseph Polchinski
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Editors and Affiliations

  1. Université Pierre et Marie Curie, Paris, France

    Laurent Baulieu  & Boris Pioline  & 

  2. University of Amsterdam, The Netherlands

    Jan de Boer

  3. Hebrew University, Jerusalem, Israel

    Eliezer Rabinovici

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Polchinski, J. (2005). Introduction to Cosmic F- and D-Strings. In: Baulieu, L., de Boer, J., Pioline, B., Rabinovici, E. (eds) String Theory: From Gauge Interactions to Cosmology. NATO Science Series II: Mathematics, Physics and Chemistry, vol 208. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3733-3_10

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