Anatomy of bubbling solutions
Kostas Skenderis, Marika Taylor

TL;DR
This paper analyzes the holographic duals of LLM bubbling solutions, showing how phase space distributions determine vevs of 1/2 BPS operators in N=4 SYM and confirming their agreement with field theory calculations.
Contribution
It demonstrates that phase space distributions in LLM solutions determine vevs of 1/2 BPS operators, with explicit holographic calculations matching field theory results.
Findings
Vevs of operators up to dimension 4 are extracted holographically.
Phase space distribution determines vevs to leading order in large N.
Exact agreement with field theory expressions is confirmed.
Abstract
We present a comprehensive analysis of holography for the bubbling solutions of Lin-Lunin-Maldacena. These solutions are uniquely determined by a coloring of a 2-plane, which was argued to correspond to the phase space of free fermions. We show that in general this phase space distribution does not determine fully the 1/2 BPS state of N=4 SYM that the gravitational solution is dual to, but it does determine it enough so that vevs of all single trace 1/2 BPS operators in that state are uniquely determined to leading order in the large N limit. These are precisely the vevs encoded in the asymptotics of the LLM solutions. We extract these vevs for operators up to dimension 4 using holographic renormalization and KK holography and show exact agreement with the field theory expressions.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum Chromodynamics and Particle Interactions
