Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2004-12-20
Phys.Lett.B619:17-25,2005
Physics
High Energy Physics
High Energy Physics - Theory
16 pages
Scientific paper
10.1016/j.physletb.2005.05.047
In the context of a cosmological string model describing the propagation of strings in a time-dependent Robertson-Walker background space-time, we show that the asymptotic acceleration of the Universe can be identified with the square of the string coupling. This allows for a direct measurement of the ten-dimensional string coupling using cosmological data. We conjecture that this is a generic feature of a class of non-critical string models that approach asymptotically a conformal (critical) sigma model whose target space is a four-dimensional space-time with a dilaton background that is linear in sigma-model time. The relation between the cosmic acceleration and the string coupling does not apply in critical strings with constant dilaton fields in four dimensions.
Ellis John
Mavromatos Nick E.
Nanopoulos Dimitri V.
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