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Quantum gravity at a large number of dimensions

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arxiv hep-th/0310263 v2 pith:LCARSPML submitted 2003-10-28 hep-th gr-qchep-ph

classification hep-thgr-qchep-ph
keywords theoryeffectivefieldgravitylarge-limitwillexpansion
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abstract

We consider the large-$D$ limit of Einstein gravity. It is observed that a consistent leading large-$D$ graph limit exists, and that it is built up by a subclass of planar diagrams. The graphs in the effective field theory extension of Einstein gravity are investigated in the same context, and it is seen that an effective field theory extension of the basic Einstein-Hilbert theory will not upset the latter leading large-$D$ graph limit, {\it i.e.}, the same subclass of planar diagrams will dominate at large-$D$ in the effective field theory. The effective field theory description of large-$D$ quantum gravity limit will be renormalizable, and the resulting theory will thus be completely well defined up to the Planck scale at $\sim 10^{19}$ GeV. The $(\frac1D)$ expansion in gravity is compared to the successful $(\frac1N)$ expansion in gauge theory (the planar diagram limit), and dissimilarities and parallels of the two expansions are discussed. We consider the expansion of the effective field theory terms and we make some remarks on explicit calculations of $n$-point functions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Higher-Dimensional Black Holes and Effective Field Theory

    hep-th 2024-12 conditional novelty 7.0 of 10

    Higher-dimensional spinning black holes generally have nonzero scalar tidal Love numbers, with patterns of zeroes in special limits, computed via point-particle EFT matching.

  2. Black hole evaporation and semiclassicality at large D

    hep-th 2019-08 conditional novelty 7.0 of 10

    At large spacetime dimension D, semiclassical black holes require entropy S_BH > (D/4π)^(D+3) log D, a bound stronger than the usual curvature and backreaction conditions.

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