2004
DOI: 10.1103/physrevd.70.106009
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Soft supersymmetry breaking on the brane

Abstract: We consider the low-energy description of 5D models of supergravity with boundaries comprizing a vector multiplet and the universal hypermultiplet in the bulk. We analyze the spontaneous breaking of supersymmetry induced by the vacuum expectation value of superpotentials on the boundary branes. When supersymmetry is broken, the moduli corresponding to the radion, the zero mode of the vector multiplet scalar field and the dilaton develop a potential in the effective action. We compute the resulting soft breakin… Show more

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Cited by 85 publications
(144 citation statements)
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References 58 publications
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“…As noted by other authors [7,10,11,12,14], it is straightforward to see that this produces the same differential equation in the bulk for the KK eigenfunctions as found in the usual RS scenario [18] and thus…”
Section: Kaluza-klein Formalismsupporting
confidence: 70%
See 1 more Smart Citation
“…As noted by other authors [7,10,11,12,14], it is straightforward to see that this produces the same differential equation in the bulk for the KK eigenfunctions as found in the usual RS scenario [18] and thus…”
Section: Kaluza-klein Formalismsupporting
confidence: 70%
“…[7,9,8,10,11,12,13,14]). In this paper we are interested in how the presence of the G-B term alters the detailed collider phenomenology of the RS model.…”
Section: Introductionmentioning
confidence: 99%
“…In the case of tracking-type quintessence potentials, usually considered in Chameleon scenarios, one needs small integer values of the index n ≥ O(1) in order to have the appropriate mass scale [56]. Therefore, s ∼ 2 can be seen as a typical value for Chameleon models.…”
Section: Parametrizing the Modifications Of Gravitymentioning
confidence: 99%
“…One possible loophole is if the solar system limits on the scalar coupling should not be applied to a cosmological situation because of the different spacetime backgrounds with very different scalar curvatures. This arises for example in chameleon scenarios [21]. The most stringent cosmological bounds on varying G arise from primordial nucleosynthesis and give ω −1 JBD < ∼ 3 × 10 −3 [22] (but see [23]).…”
Section: Beyond Scalar Fieldsmentioning
confidence: 99%