Gravity and compactified branes in matrix models
arXiv:1202.6306 · doi:10.1007/JHEP07(2012)156
Abstract
A mechanism for emergent gravity on brane solutions in Yang-Mills matrix models is exhibited. Newtonian gravity and a partial relation between the Einstein tensor and the energy-momentum tensor can arise from the basic matrix model action, without invoking an Einstein-Hilbert-type term. The key requirements are compactified extra dimensions with extrinsic curvature M^4 x K \subset R^D and split noncommutativity, with a Poisson tensor θ^{ab} linking the compact with the noncompact directions. The moduli of the compactification provide the dominant degrees of freedom for gravity, which are transmitted to the 4 noncompact directions via the Poisson tensor. The effective Newton constant is determined by the scale of noncommutativity and the compactification. This gravity theory is well suited for quantization, and argued to be perturbatively finite for the IKKT model. Since no compactification of the target space is needed, it might provide a way to avoid the landscape problem in string theory.
35 pages. V2: substantially revised and improved, conclusion weakened. V3: some clarifications, published version. V4: minor correction
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- On the Phase Structure of Commuting Matrix Models
- Near commuting multi-matrix models
- Brane compactifications and 4-dimensional geometry in the IKKT model
- One-loop stabilization of the fuzzy four-sphere via softly broken SUSY
- Dirac equation on coordinate dependent noncommutative space-time
- The curvature of branes, currents and gravity in matrix models
- Influences of the coordinate dependent noncommutative space on charged and spin currents