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On the conformal anomaly from higher derivative gravity in AdS/CFT correspondence.(English)Zbl 0952.81053

Summary: We follow Witten’s proposal in the calculation of conformal anomaly from \((d+1)\)-dimensional higher derivative gravity via AdS/CFT correspondence. It is assumed that some \(d\)-dimensional conformal field theories have a description in terms of above \((d + 1)\)-dimensional higher derivative gravity which includes not only the Einstein term and cosmological constant but also curvature squared terms. The explicit expression for two-dimensional and four-dimensional anomalies is found, it contains higher derivative corrections. In particular, it is shown that not only Einstein gravity but also theory with the Lagrangian \(L= aR^2+ bR_{\mu\nu} R^{\mu\nu}+ \Lambda\) (even when \(a= 0\) or \(b= 0\)) is five-dimensional bulk theory for \(d= 4\) \(N= 4\) super-Yang-Mills theory in AdS/CFT correspondence. Similarly, the \(d+ 1= 3\) theory with (or without) Einstein term may describe \(d= 2\) scalar or spinor CFT’s. That gives new versions of bulk side which may be useful in different aspects. As application of our general formalism we find next-to-leading corrections to the conformal anomaly of \(N= 2\) supersymmetric theory from \(d= 5\) AdS higher derivative gravity (low energy string effective action).

MSC:

81T50 Anomalies in quantum field theory
81T30 String and superstring theories; other extended objects (e.g., branes) in quantum field theory
81T60 Supersymmetric field theories in quantum mechanics
83E30 String and superstring theories in gravitational theory

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References:

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This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.
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