论文标题
HyperCube上的混乱
Chaos on the hypercube
论文作者
论文摘要
我们分析了最初由Parisi引入的$ d $维度超纤维(HC)晶格模型的光谱特性。该模型的u(1)量规链路产生了恒定幅度$ ϕ $的磁通量,但通过超立方体的面部随机取向。 HC模型也可以作为$ 2D $交互的Majorana Fermions的模型写入,具有让人联想到Maldacena-QI(MQ)模型的光谱流,其频谱为$ ϕ = 0 $,实际上与MQ模型的耦合项相吻合。正如Parisi所显示的那样,在$ 1/d $的领先顺序上,该模型的频谱密度由Q-热矿多项式的密度函数给出,这也是双尺度sachdev-ye-kitaev模型的光谱密度。巴黎通过将HC模型的矩映射到和弦图上的$ q $加权总和来证明这一点。我们指出,HC模型的转向矩也可以映射到和弦图上的加权总和,以从领先时刻降下的方式。 HC模型具有磁反转对称性,取决于磁通量穿过HyperCube的面的大小和方向。该对称性的固定量子数的光谱表现出从$ ϕ = 0 $的常规光谱向混乱的光谱的过渡,其光谱统计数据由高斯单位合奏(GUE)给出,以$ ϕ $的较大值。对于小磁通量,基态被覆盖并接近热菲尔德双重(TFD)状态。
We analyze the spectral properties of a $d$-dimensional HyperCubic (HC) lattice model originally introduced by Parisi. The U(1) gauge links of this model give rise to a magnetic flux of constant magnitude $ϕ$ but random orientation through the faces of the hypercube. The HC model, which also can be written as a model of $2d$ interacting Majorana fermions, has a spectral flow that is reminiscent of the Maldacena-Qi (MQ) model, and its spectrum at $ϕ=0$, actually coincides with the coupling term of the MQ model. As was already shown by Parisi, at leading order in $1/d$ , the spectral density of this model is given by the density function of the Q-Hermite polynomials, which is also the spectral density of the double-scaled Sachdev-Ye-Kitaev model. Parisi demonstrated this by mapping the moments of the HC model to $Q$-weighted sums on chord diagrams. We point out that the subleading moments of the HC model can also be mapped to weighted sums on chord diagrams, in a manner that descends from the leading moments. The HC model has a magnetic inversion symmetry that depends on both the magnitude and the orientation of the magnetic flux through the faces of the hypercube. The spectrum for fixed quantum number of this symmetry exhibits a transition from regular spectra at $ϕ=0$ to chaotic spectra with spectral statistics given by the Gaussian Unitary Ensembles (GUE) for larger values of $ϕ$. For small magnetic flux, the ground state is gapped and is close to a Thermofield Double (TFD) state.