2017
DOI: 10.1016/j.nuclphysb.2017.08.004
|View full text |Cite
|
Sign up to set email alerts
|

Stabilization of moduli in spacetime with nested warping and the UED

Abstract: The absence, so far, of any graviton signatures at the LHC imposes severe constraints on the Randall-Sundrum scenario. Although a generalization to higher dimensions with nested warpings has been shown to avoid these constraints, apart from incorporating several other phenomenologically interesting features, moduli stabilization in such models has been an open question. We demonstrate here how both the moduli involved can be stabilized, employing slightly different mechanisms for the two branches of the theory… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
25
0

Year Published

2017
2017
2024
2024

Publication Types

Select...
8

Relationship

2
6

Authors

Journals

citations
Cited by 18 publications
(25 citation statements)
references
References 42 publications
0
25
0
Order By: Relevance
“…Any fluctuation about this stabilized value leads to a scalar degree of freedom, called the radion field. There have been numerous studies later on, regarding the details of the stabilization mechanism, corresponding collider signatures and of course, various generalizations, e.g., time dependent stabilization of the radion field (for a small sample of works see [14][15][16][17][18][19][20][21][22][23], and also the references therein).…”
Section: Introductionmentioning
confidence: 99%
“…Any fluctuation about this stabilized value leads to a scalar degree of freedom, called the radion field. There have been numerous studies later on, regarding the details of the stabilization mechanism, corresponding collider signatures and of course, various generalizations, e.g., time dependent stabilization of the radion field (for a small sample of works see [14][15][16][17][18][19][20][21][22][23], and also the references therein).…”
Section: Introductionmentioning
confidence: 99%
“…(5) and (6), this limit translates to a lower bound on Λ φ of a few TeVs. However, this bound can be relaxed considerably for models with more than one extra dimension [44][45][46]. In these classes of models, the mass of the graviton and its coupling to the SM fields are suppressed due to the presence of two scales in the theory, and Λ φ as low as 1 TeV is allowed.…”
Section: Theoretical and Experimental Constraintsmentioning
confidence: 99%
“…Thus, smarter generalizations are called for. Embedding the UED in a 6-dimensional warped space [26,27], for example, makes it possible to evade the relic density bounds by exploiting the s-channel annihilation channel with graviton mediated by a KK-graviton exchange. In this paper we offer a different solution, one that leads to a very rich collider phenomenology.…”
Section: Jhep01(2019)230mentioning
confidence: 99%