Gravity and compactified branes in matrix models
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 \theta^{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.
Keywords
Cite
@article{arxiv.1202.6306,
title = {Gravity and compactified branes in matrix models},
author = {Harold Steinacker},
journal= {arXiv preprint arXiv:1202.6306},
year = {2014}
}
Comments
35 pages. V2: substantially revised and improved, conclusion weakened. V3: some clarifications, published version. V4: minor correction