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Phys. Rev. Lett. 78, 2288–2291 (1997)

Cosmic Strings and the String Dilaton

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Thibault Damour
Institut des Hautes Etudes Scientifiques, F-91440 Bures sur Yvette, France
and DARC, CNRS-Observatoire de Paris, F-92195 Meudon, France

Alexander Vilenkin
Institute of Cosmology, Department of Physics and Astronomy, Tufts University, Medford, Massachusetts 02155

Received 3 October 1996; published in the issue dated 24 March 1997

The existence of a dilaton (or moduli) with gravitational-strength coupling to matter imposes stringent constraints on the allowed energy scale of cosmic strings, η. In particular, superheavy gauge strings with η1016GeV are ruled out unless the dilaton mass mφ100TeV, while the currently popular value mφ1TeV imposes the bound η≲3×1011GeV. Some nonstandard cosmological scenarios which can avoid these constraints are pointed out.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.78.2288
DOI:
10.1103/PhysRevLett.78.2288
PACS:
98.80.Cq, 11.25.-w, 11.27.+d