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arXiv 2302.03041hep-thgr-qc
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全息与无关算符

Holography and Irrelevant Operators

Chih-Kai Chang, Christian Ferko, Savdeep Sethi

AI总结:

本文从引力角度探讨了三维线性膨胀子渐近时空的全息猜想,提出十维超引力解以实现场论与引力参数的精确对应,验证了 $T \overline{T}$ 形变特有的平方根结构,并探讨了形变过大时闭弦快子的潜在作用。

摘要:

我们从引力角度探讨了涉及三维中线性膨胀子渐近的时空的全息猜想。全息对偶与由 $T \overline{T}$ 形变的单迹类似物形变的对称积共形场论(CFT)具有一些共同性质。我们提出了十维超引力的解,这些解从内部的 BTZ 黑洞插值到无穷远处的线性膨胀子时空或平坦空间。这使得场论参数与引力参数能够精确对应。这些解明显表现出 $T \overline{T}$ 形变共形场论特有的平方根结构。我们使用协变相空间形式计算了这些时空的质量,并发现对于无自旋黑洞的情况,结果与平方根公式一致。我们还讨论了当形变参数过大且真空变得不稳定时,闭弦快子可能发挥的作用。

英文摘要:

We explore the holographic proposal involving spacetimes with linear dilaton asymptotics in three dimensions from a gravity perspective. The holographic dual shares some properties with a symmetric product conformal field theory deformed by a single-trace analogue of the $T \overline{T}$ deformation. We present solutions of ten-dimensional supergravity which interpolate from BTZ black holes in the interior to either a linear dilaton spacetime near infinity, or to flat space. This allows a precise identification of field theory parameters with gravity parameters. The solutions manifestly exhibit the square root structure that is characteristic of $T \overline{T}$-deformed conformal field theories. We compute the mass of the spacetimes using the covariant phase space formalism and find agreement with the square root formula for the case of black holes without spin. We also discuss whether closed string tachyons might play a role when the deformation parameter becomes too large and the vacuum becomes unstable.

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