Tom Banks et al JCAP06(2003)001 doi:10.1088/1475-7516/2003/06/001
Tom Banks, Michael Dine, P J Fox and E Gorbatov
Show affiliationsThe decay constant of the QCD axion is required by observation to be small compared with the Planck scale. In theories of `natural inflation' and certain proposed anthropic solutions of the cosmological constant problem it would be interesting to obtain a large decay constant for axion-like fields from microscopic physics. String theory is the only context in which one can sensibly address this question. Here we survey a number of periodic fields in string theory in a variety of string vacua. In some examples, the decay constant can be parametrically larger than the Planck scale but the effective action then contains appreciable harmonics of order fA/Mp. As a result, these fields are no better inflaton candidates than Planck scale axions.
14.80.Mz Axions and other Nambu-Goldstone bosons (Majorons, familons, etc.)
Issue 06 (June 2003)
Received 2 April 2003, accepted for publication 4 May 2003
Published 11 June 2003
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