<p>We study the BPS states of <i>U</i> (<i>N</i>)<sub><i>k</i></sub> × <i>U</i> (1)<sub>−<i>k</i></sub> vector Chern-Simons theory on a sphere at weak coupling <i>λ</i> = <InlineEquation ID="IEq1"> <EquationSource Format="MATHML"><math display="inline"> <mfrac> <mi>N</mi> <mi>k</mi> </mfrac> </math></EquationSource> <EquationSource Format="TEX">\( \frac{N}{k} \)</EquationSource> </InlineEquation> ≪ 1, dual to an AdS<sub>4</sub> higher spin gravity. Higher spin currents are well known to be anomalous at <i>λ</i> ≠ 0. We show that these non-BPS higher spin particles form multi-particle ‘BPS bounds’ at low energy, and interpret them as a primordial form of small black hole states. We also construct a new heavy BPS operator at <i>N</i> = 2. We study the BPS phases of this system from the large <i>N</i> index at Planckian ‘temperatures’. The deconfined saddles at high temperature exist only above a threshold, similar to the BTZ black holes. The low temperature saddles are given by novel 2-cut eigenvalue distributions. Their phase transition involves subtle issues like the holomorphic anomaly and the background independence, whose studies we initiate. In particular, we obtain a lower bound on the critical temperature by studying the eigenvalue instantons.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

BPS phases and fortuity in higher spin holography

  • Seok Kim,
  • Jehyun Lee,
  • Siyul Lee,
  • Hyunwoo Oh

摘要

We study the BPS states of U (N)k × U (1)k vector Chern-Simons theory on a sphere at weak coupling λ = N k \( \frac{N}{k} \) ≪ 1, dual to an AdS4 higher spin gravity. Higher spin currents are well known to be anomalous at λ ≠ 0. We show that these non-BPS higher spin particles form multi-particle ‘BPS bounds’ at low energy, and interpret them as a primordial form of small black hole states. We also construct a new heavy BPS operator at N = 2. We study the BPS phases of this system from the large N index at Planckian ‘temperatures’. The deconfined saddles at high temperature exist only above a threshold, similar to the BTZ black holes. The low temperature saddles are given by novel 2-cut eigenvalue distributions. Their phase transition involves subtle issues like the holomorphic anomaly and the background independence, whose studies we initiate. In particular, we obtain a lower bound on the critical temperature by studying the eigenvalue instantons.