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Stabilization of Extra Dimensions at Tree Level

Scott Watson, Robert Brandenberger

TL;DR

The paper addresses why string-theoretic extra dimensions remain compact by analyzing winding and momentum modes on a time-dependent background at weak coupling and tree-level in $\alpha'$, showing stabilization of six internal dimensions at the self-dual radius $R=1$. It derives and uses T-duality to relate winding/momentum contributions to the background evolution, demonstrating a robust stabilization mechanism that drives the internal space to $R=1$ while the three large dimensions expand. The results hinge on balancing negative pressure from winding and positive pressure from momentum modes, with the dilaton playing a crucial role in maintaining a weak-coupling regime. The work aligns with earlier qualitative arguments and highlights the need for a dilaton potential and higher-order corrections to bridge to late-time FRW cosmology.

Abstract

By considering the effects of string winding and momentum modes on a time dependent background, we find a method by which six compact dimensions become stabilized naturally at the self-dual radius while three dimensions grow large.

Stabilization of Extra Dimensions at Tree Level

TL;DR

The paper addresses why string-theoretic extra dimensions remain compact by analyzing winding and momentum modes on a time-dependent background at weak coupling and tree-level in , showing stabilization of six internal dimensions at the self-dual radius . It derives and uses T-duality to relate winding/momentum contributions to the background evolution, demonstrating a robust stabilization mechanism that drives the internal space to while the three large dimensions expand. The results hinge on balancing negative pressure from winding and positive pressure from momentum modes, with the dilaton playing a crucial role in maintaining a weak-coupling regime. The work aligns with earlier qualitative arguments and highlights the need for a dilaton potential and higher-order corrections to bridge to late-time FRW cosmology.

Abstract

By considering the effects of string winding and momentum modes on a time dependent background, we find a method by which six compact dimensions become stabilized naturally at the self-dual radius while three dimensions grow large.

Paper Structure

This paper contains 5 sections, 17 equations, 2 figures.

Figures (2)

  • Figure 1: Here we take the six small dimensions to be at the self-dual radius and with vanishing expansion rate initially, $b_{0}=1$ and $\dot{\nu}_{0}=0$. We find that the dimensions remain stable at the self-dual point regardless of the behavior of the dilaton and of the three large dimensions. These are shown in the figure for the initial values $\lambda_{0}=3$, $\dot{\lambda}_{0}=0.5$, and $\phi_{0}=-3$. However, this result holds for generic initial values as long as we respect the weak coupling limit (i.e. $g_{s}<<1$). Note that we are using Planck units.
  • Figure 2: We consider initial values of $b(t)$ away from the self-dual radius and find oscillations about the self-dual radius which are damped by the dilaton and by the evolution of the large dimensions. This is again a generic result. Here we present the evolution for the following initial data: $\dot{\lambda}_{0} = .500, \phi_{0} = -3.00, \dot{\phi}_{0} = .380, \lambda_{0} = 3.00, \dot{\nu}_{0} = 0, \nu_{0} = 0$$\dot{\lambda}_{0} = .500, \phi_{0} = -3.00, \dot{\phi}_{0} = -.020, \lambda_{0} = 3.00, \dot{\nu}_{0} = -.100, \nu_{0} = .010$$\dot{\lambda}_{0} = .500, \phi_{0} = -3.00, \dot{\phi}_{0} = -.008, \lambda_{0} = 3.00, \dot{\nu}_{0} = -.100, \nu_{0} = .500$