2003
DOI: 10.1016/s0550-3213(02)01092-1
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Non-Abelian T-duality in pre-big-bang cosmology

Abstract: We study the impact of non-Abelian T-duality transformations on a string based cosmological model. The implementation of the pre-big-bang scenario is investigated. We found a region of the dual phase where such a picture is possible. 1

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Cited by 4 publications
(4 citation statements)
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“…where f cd b are structure coefficients of the Lie algebra of the group G and ĝb are coordinates of the Abelian group G. Equations ( 24)-( 26) then become the Buscher formulas for non-Abelian T-duality (see [18][19][20]). The dual tensor (21) in this case can be written as…”
Section: Dual Tensor Fieldmentioning
confidence: 99%
See 1 more Smart Citation
“…where f cd b are structure coefficients of the Lie algebra of the group G and ĝb are coordinates of the Abelian group G. Equations ( 24)-( 26) then become the Buscher formulas for non-Abelian T-duality (see [18][19][20]). The dual tensor (21) in this case can be written as…”
Section: Dual Tensor Fieldmentioning
confidence: 99%
“…Applications of non-Abelian duality in cosmology, more precisely on FLRW metrics, can be found e.g. in [21].…”
Section: Introductionmentioning
confidence: 99%
“…These results may have interesting applications in the context of the Pre-Big Bang scenario, in particular in relation with the graceful exit problem. Also, the equivalence between bulk and brane duality might be extended by means of non-Abelian T-dualities [20,21] or to more general string backgrounds. We think that all these aspects deserve further investigations.…”
Section: Discussionmentioning
confidence: 99%
“…where g, h ∈ G, g, h ∈ G. The map h : R 2 → G that we need for this transformation is the solution to the equations (9,10). The equation ( 12) then defines the Poisson-Lie transformation between the solution of the equations of motion of the original sigma model and its dual.…”
Section: Elements Of Poisson-lie T-dual Sigma Modelsmentioning
confidence: 99%