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arXiv 2409.08709hep-th
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来自$T^2$形变可解扇区的类时边界$dS_4$全息性

Timelike-bounded $dS_4$ holography from a solvable sector of the $T^2$ deformation

Eva Silverstein, Gonzalo Torroba

AI总结:

本研究将$T\bar T$类形变方法推广到高维,通过$CFT_3$的受限$T^2$形变定义$dS_4$的有限$N$可解扇区,结合形变算法捕捉局域体激发,构建了类时边界$dS_4$的全息描述。

摘要:

近期研究利用$T\bar T$类形变的易处理性,构建了包含$dS_3$在内的三维体时空的类时边界区域。该方法将问题拆分为两部分:一个捕捉最具熵性能带的可解理论,以及一个处理额外效应和精细结构的调谐算法。我们指出该方法可直接推广到更高维度,且不需要完整$T^2$算符(文献[1]中定义的$T\bar T$的高维类比)的因子化。\n\n聚焦于$dS_4$,我们首先通过${S}^2\times \mathbb{R}$上$CFT_3$的受限$T^2$形变,定义了有限$N$下的可解理论,其中$T$被替换为其在对称均匀态中呈现的形式,仅包含对角能量密度$E/V$和压强(-$dE/dV$)分量。这定义了$dS_4/\text{deformed-CFT}_3$的一个有限$N$可解扇区,捕捉了径向几何和熵主导能带的计数,将Gibbons-Hawking熵重现为态计数。\n\n为准确捕捉包含引力子在内的$dS_4$的局域体激发,我们直接类比文献[2]中近期提出的含体物质的$dS_3$情形,构建了一种形变算法。该算法以可解形变的无穷小作用作为调节器起步。完整的微观理论通过在每一步添加$T^2$和其他算符的重整化版本构建,这些算符通过与适用的体局域计算匹配来定义,包括从$AdS_4/CFT_3$到$dS_4$的提升(这在M理论的双曲紧化中是可行的)。体局域算法的细节依赖于边界条件的选择;我们总结了这些条件在广义相对论及其他领域的现状,并以柱形Dirichlet条件为例说明了我们的方法,该条件可通过我们的有限量子理论实现紫外完备。

英文摘要:

Recent research has leveraged the tractability of $T\bar T$ style deformations to formulate timelike-bounded patches of three-dimensional bulk spacetimes including $dS_3$. This proceeds by breaking the problem into two parts: a solvable theory that captures the most entropic energy bands, and a tuning algorithm to treat additional effects and fine structure. We point out that the method extends readily to higher dimensions, and does not require factorization of the full $T^2$ operator (the higher dimensional analogue of $T\bar T$ defined in [1]). Focusing on $dS_4$, we first define a solvable theory at finite $N$ via a restricted $T^2$ deformation of the $CFT_3$ on ${S}^2\times \mathbb{R}$, in which $T$ is replaced by the form it would take in symmetric homogeneous states, containing only diagonal energy density $E/V$ and pressure (-$dE/dV$) components. This defines a finite-N solvable sector of $dS_4/\text{deformed-CFT}_3$, capturing the radial geometry and count of the entropically dominant energy band, reproducing the Gibbons-Hawking entropy as a state count. To accurately capture local bulk excitations of $dS_4$ including gravitons, we build a deformation algorithm in direct analogy to the case of $dS_3$ with bulk matter recently proposed in [2]. This starts with an infinitesimal stint of the solvable deformation as a regulator. The full microscopic theory is built by adding renormalized versions of $T^2$ and other operators at each step, defined by matching to bulk local calculations when they apply, including an uplift from $AdS_4/CFT_3$ to $dS_4$ (as is available in hyperbolic compactifications of M theory). The details of the bulk-local algorithm depend on the choice of boundary conditions; we summarize the status of these in GR and beyond, illustrating our method for the case of the cylindrical Dirichlet condition which can be UV completed by our finite quantum theory.

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