Baby Universes from Thermal Pure States in SYK
SYK中热纯态产生的婴儿宇宙
Martin Sasieta, Brian Swingle, Alejandro Vilar López
AI总结 通过SYK热纯态构造闭合婴儿宇宙的二维全息模型,利用JT引力黑洞内部和Maldacena-Qi相变,研究大N下AdS区域与婴儿宇宙间的纠缠。
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- 8 pages, 4 figures. v2: minor edits, journal version
我们构造了一个简单的二维全息模型,描述一个闭合的“婴儿”宇宙。婴儿宇宙时空起源于Jackiw-Teitelboim (JT)引力中的黑洞内部。全息描述是两个Sachdev-Ye-Kitaev (SYK)模型的低温热纯态。该态的构造依赖于一个重物质算符的插入,它支撑婴儿宇宙,同时依赖于黑洞相和空Anti de Sitter (AdS)相之间的一级热相变。对于相变,我们采用了两个耦合SYK系统的Maldacena-Qi相变的一个版本。由于大量轻体场,AdS区域与婴儿宇宙之间的体纠缠在相变以下保持O(N)。这种纠缠可以通过对SYK耦合进行粗粒化来定义。
We construct a simple two-dimensional holographic model of a closed "baby" universe. The baby universe spacetime originates from the black hole interior in Jackiw-Teitelboim (JT) gravity. The holographic description is a low-temperature thermal pure state of two Sachdev-Ye-Kitaev (SYK) models. The construction of the state relies on the insertion of a heavy matter operator, which supports the baby universe, together with a first-order thermal phase transition between a black hole phase and an empty Anti de Sitter (AdS) phase. For the transition, we employ a version of the Maldacena-Qi phase transition of two coupled SYK systems. The bulk entanglement between the AdS region and the baby universe remains O(N) below the transition, owing to the large number of light bulk fields. This entanglement admits a definition through coarse-graining over SYK couplings.