Abstract:We propose a mechanism for stabilizing the size of the extra dimension in the
Randall-Sundrum scenario. The potential for the modulus field that sets the
size of the fifth dimension is generated by a bulk scalar with quartic
interactions localized on the two 3-branes. The minimum of this potential
yields a compactification scale that solves the hierarchy problem without fine
tuning of parameters.Comment: 8 pages, LaTeX; minor typo correcte
“…[15] -compare Figs. [5] and [6]. Since the value of r * c which induces the appearance of internal structure is lower in curved spacetime, we can infer that gravity tends to supress the presence of internal structure in braneword scenarios like the one here investigated.…”
Section: Internal Structurementioning
confidence: 87%
“…Our investigations are based on several recent works on branes [1,2,3,4,5,6,7,8,9], and it follows the lines of our former work on brane structure [15].…”
Section: Further Commentsmentioning
confidence: 99%
“…We focus mainly on generation of thick branes, their stability and internal structure, and our investigations follow several recent works on the subject [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15].…”
We investigate a system described by two real scalar fields coupled with gravity in (4, 1) dimensions in warped spacetime involving one extra dimension. The results show that the parameter which controls the way the two scalar fields interact induces the appearence of thick brane which engenders internal structure, driving the energy density to localize inside the brane in a very specific way.
“…[15] -compare Figs. [5] and [6]. Since the value of r * c which induces the appearance of internal structure is lower in curved spacetime, we can infer that gravity tends to supress the presence of internal structure in braneword scenarios like the one here investigated.…”
Section: Internal Structurementioning
confidence: 87%
“…Our investigations are based on several recent works on branes [1,2,3,4,5,6,7,8,9], and it follows the lines of our former work on brane structure [15].…”
Section: Further Commentsmentioning
confidence: 99%
“…We focus mainly on generation of thick branes, their stability and internal structure, and our investigations follow several recent works on the subject [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15].…”
We investigate a system described by two real scalar fields coupled with gravity in (4, 1) dimensions in warped spacetime involving one extra dimension. The results show that the parameter which controls the way the two scalar fields interact induces the appearence of thick brane which engenders internal structure, driving the energy density to localize inside the brane in a very specific way.
“…Goldberger and Wise proposed a simple stabilization mechanism for the distance between the branes [6]. They added to the original Randall-Sundrum model with brane tensions λ h = −λ v a scalar field Φ with bulk action…”
Section: Goldberger-wise Mechanism Of Brane Stabilizationmentioning
A set of consistency conditions is derived from Einstein equations for brane world scenarios with a spatially periodic internal space. In particular, the sum of the total tension of the flat branes and the non-negative integral of the gradient energy of the bulk scalars must vanish. This constraint allows us to make a simple consistency check of several models. We show that the two-brane Randall-Sundrum model satisfies this constraint, but it does not allow a generalization with smooth branes (domain walls), independently of the issue of supersymmetry. The Goldberger-Wise model of brane stabilization has to include the backreaction on the metric and the fine tuning of the cosmological constant to satisfy the constraints. We check that this is achieved in the DeWolfe-Freedman-Gubser-Karch scenario. Our constraints are automatically satisfied in supersymmetric brane world models.
“…Two interesting examples are: i) in brane world scenarios, scalar fields are thought to stabilize the fifth dimension (see e.g. [6]); ii) the energy of bulk scalar field(s) might flow onto or away from the brane universe and thereby modify the expansion dynamics.…”
We investigate cosmological consequences arising from the interaction between a homogeneous and isotropic brane-universe and the bulk. A Friedmann equation is derived which incorporates both the brane and bulk matter contributions, which are both assumed to be of arbitrary fluid form. In particular, new terms arise which describe the energy flow onto (or away from) the brane, as well as changes of the equation of state in the bulk. We discuss Randall-Sundrum type models as well as dilatonic domain walls and carefully consider the conditions for stabilizing the induced gravitational constant. Furthermore, consequences for cosmological perturbations are analyzed. We show that, in general, super-horizon amplitudes are not constant.
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