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Dynamical localization for a random scattering zipper 随机散射拉链的动态定位
IF 1.4 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-30 DOI: 10.1007/s11005-025-01952-x
Hakim Boumaza, Amine Khouildi

This article establishes a proof of dynamical localization for a random scattering zipper model. The scattering zipper operator is the product of two unitary by blocks operators, multiplicatively perturbed on the left and right by random unitary phases. One of the operator is shifted so that this configuration produces a random 5-diagonal by blocks unitary operator. To prove the dynamical localization for this operator, we use the fractional moments method. We first prove the continuity and strict positivity of the Lyapunov exponents in an annulus around the unit circle, which leads to the exponential decay of a power of the norm of the products of transfer matrices. We then establish an explicit formula of the coefficients of the finite resolvent in terms of the coefficients of the transfer matrices using Schur’s complement. From this, we deduce, through two reduction results, the exponential decay of the resolvent, from which we get the dynamical localization.

本文建立了随机散射拉链模型的动态局部化证明。散射拉链算子是两个酉by块算子的乘积,它们在左右两边被随机的酉相相乘摄动。其中一个运算符被移位,使得这个配置产生一个随机的5-对角块酉运算符。为了证明该算子的动态定位,我们使用分数阶矩方法。首先证明了单位圆周围环上Lyapunov指数的连续性和严格正性,从而导致了传递矩阵乘积范数幂的指数衰减。然后,我们利用Schur补建立了一个用传递矩阵系数表示的有限解析系数的显式公式。在此基础上,通过两个约简结果推导出解的指数衰减,从而得到动力学局域化。
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引用次数: 0
Lorentzian metric spaces and GH-convergence: the unbounded case 洛伦兹度量空间与gh收敛:无界情况
IF 1.4 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-29 DOI: 10.1007/s11005-025-01941-0
A. Bykov, E. Minguzzi, S. Suhr

We introduce a notion of Lorentzian metric space which drops the boundedness condition from our previous work and argue that the properties defining our spaces are minimal. In fact, they are defined by three conditions given by (a) the reverse triangle inequality for chronologically related events, (b) Lorentzian distance continuity and relative compactness of chronological diamonds, and (c) a distinguishing condition via the Lorentzian distance function. By adding a countably generating condition, we confirm the validity of desirable properties for our spaces including the Polish property. The definition of (pre)length space given in our previous work on the bounded case is generalized to this setting. We also define a notion of Gromov–Hausdorff convergence for Lorentzian metric spaces and prove that (pre)length spaces are GH-stable. It is also shown that our (sequenced) Lorentzian metric spaces bring a natural quasi-uniformity (resp. quasi-metric). Finally, an explicit comparison with other recent constructions based on our previous work on bounded Lorentzian metric spaces is presented.

我们引入了洛伦兹度量空间的概念,它抛弃了我们以前工作中的有界性条件,并论证了定义我们空间的性质是最小的。事实上,它们是由以下三个条件定义的:(a)时间相关事件的逆三角形不等式,(b)时间钻石的洛伦兹距离连续性和相对紧性,以及(c)通过洛伦兹距离函数的区分条件。通过添加可数生成条件,我们确认了空间的理想性质的有效性,包括波兰性质。在我们之前关于有界情况的工作中给出的(预)长度空间的定义推广到这种情况。我们还定义了Lorentzian度量空间的Gromov-Hausdorff收敛的概念,并证明了(预)长度空间是gh稳定的。本文还证明了我们的(有序的)洛伦兹度量空间具有自然的拟均匀性。非对称度量)。最后,与其他基于我们之前关于有界洛伦兹度量空间的工作的最新构造进行了明确的比较。
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引用次数: 0
The factorial growth of topological recursion 拓扑递归的阶乘增长
IF 1.4 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-28 DOI: 10.1007/s11005-025-01950-z
Gaëtan Borot, Bertrand Eynard, Alessandro Giacchetto

We show that the n-point, genus-g correlation functions of topological recursion on any regular spectral curve with simple ramifications grow at most like ((2g - 2 + n)!) as (g rightarrow infty ), which is the expected growth rate. This provides, in particular, an upper bound for many curve counting problems in large genus and serves as a preliminary step for a resurgence analysis.

我们证明了拓扑递归的n点,属-g相关函数在任何具有简单分支的正则谱曲线上最多像((2g - 2 + n)!)一样增长为(g rightarrow infty ),这是预期的增长率。特别地,这为许多大属的曲线计数问题提供了一个上界,并作为复现分析的初步步骤。
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引用次数: 0
Some rigidity results for complete totally trapped submanifolds in generalized Robertson–Walker spacetimes 广义Robertson-Walker时空中完全俘获子流形的一些刚性结果
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-26 DOI: 10.1007/s11005-025-01947-8
M. Andrade, F. C. Cruz Jr., R. F. Figueira, E. A. Lima Jr.

In this work, we prove rigidity results for complete totally trapped spacelike submanifolds immersed in generalized Robertson–Walker spacetimes. In particular, we obtain uniqueness and non-existence results for totally trapped submanifolds. We use a maximum principle for the (infty )-Laplacian in order to get our results. We also present examples of totally trapped submanifolds in the Schwarzschild black hole spacetime and a surface which is trapped but it is not totally trapped in the product spacetime (-{mathbb {R}}times {mathbb {R}}times {mathbb {H}}^2).

在本文中,我们证明了浸没在广义Robertson-Walker时空中的完全完全俘获的类空子流形的刚性结果。特别地,我们得到了完全困子流形的唯一性和不存在性结果。为了得到我们的结果,我们使用了(infty ) -拉普拉斯函数的极大值原理。我们还给出了在史瓦西黑洞时空中完全被困子流形的例子,以及一个被困但不是完全被困在积时空(-{mathbb {R}}times {mathbb {R}}times {mathbb {H}}^2)中的表面。
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引用次数: 0
The heat flow conjecture for polynomials and random matrices 多项式和随机矩阵的热流猜想
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-26 DOI: 10.1007/s11005-025-01946-9
Brian C. Hall, Ching-Wei Ho

We study the evolution of the roots of a polynomial of degree N, when the polynomial itself is evolving according to the heat flow. We propose a general conjecture for the large-N limit of this evolution. Specifically, we propose (1) that the log potential of the limiting root distribution should evolve according to a certain first-order, nonlinear PDE, and (2) that the limiting root distribution at a general time should be the push-forward of the initial distribution under a certain explicit transport map. These results should hold for sufficiently small times, that is, until singularities begin to form. We offer three lines of reasoning in support of our conjecture. First, from a random matrix perspective, the conjecture is supported by a deformation theorem for the second moment of the characteristic polynomial of certain random matrix models. Second, from a dynamical systems perspective, the conjecture is supported by the computation of the second derivative of the roots with respect to time, which is formally small before singularities form. Third, from a PDE perspective, the conjecture is supported by the exact PDE satisfied by the log potential of the empirical root distribution of the polynomial, which formally converges to the desired PDE as (Nrightarrow infty ). We also present a “multiplicative” version of the the conjecture, supported by similar arguments. Finally, we verify rigorously that the conjectures hold at the level of the holomorphic moments.

我们研究了N次多项式的根的演化,当多项式本身根据热流演化时。我们提出了这种演化的大n极限的一般猜想。具体来说,我们提出(1)极限根分布的对数势应该按照一定的一阶非线性PDE演化;(2)一般时刻的极限根分布应该是在一定的显式传输映射下初始分布的推进。这些结果应该在足够小的时间内成立,也就是说,直到奇点开始形成。我们提供了三条推理线来支持我们的猜想。首先,从随机矩阵的角度出发,利用某些随机矩阵模型的特征多项式的二阶矩的变形定理来支持该猜想。其次,从动力系统的角度来看,该猜想得到根对时间的二阶导数计算的支持,在奇点形成之前,它的形式很小。第三,从PDE的角度来看,该猜想得到多项式经验根分布的对数势所满足的精确PDE的支持,其形式收敛到期望的PDE为(Nrightarrow infty )。我们还提出了一个“乘法”版本的猜想,由类似的论据支持。最后,我们严格地验证了这些猜想在全纯矩的水平上成立。
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引用次数: 0
Minimal velocity bound for Schrödinger-type operator with fractional powers 分数阶算子Schrödinger-type的最小速度界
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-24 DOI: 10.1007/s11005-025-01943-y
Atsuhide Ishida

It is known in scattering theory that the minimal velocity bound plays a conclusive role in proving the asymptotic completeness of the wave operators. In this study, we prove the minimal velocity bound and other important estimates for the Schrödinger-type operator with fractional powers. We assume that the pairwise potential functions belong to broad classes that include long-range decay and Coulomb-type local singularities.

在散射理论中,已知最小速度界在证明波算符的渐近完备性方面起决定性作用。在本研究中,我们证明了分数次方Schrödinger-type算子的最小速度界和其他重要估计。我们假设成对势函数属于广义类,包括长程衰减和库仑型局部奇点。
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引用次数: 0
An integral representation for the Dirac propagator in the Reissner–Nordström geometry in Eddington–Finkelstein coordinates Eddington-Finkelstein坐标下Reissner-Nordström几何中狄拉克传播子的积分表示
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-24 DOI: 10.1007/s11005-025-01951-y
Felix Finster, Christoph Krpoun

The Cauchy problem for the massive Dirac equation is studied in the Reissner–Nordström geometry in horizon-penetrating Eddington–Finkelstein-type coordinates. We derive an integral representation for the Dirac propagator involving the solutions of the ordinary differential equations which arise in the separation of variables. Our integral representation describes the dynamics of Dirac particles outside and across the event horizon, up to the Cauchy horizon.

研究了在Reissner-Nordström几何中穿透水平的eddington - finkelstein型坐标系下质量狄拉克方程的Cauchy问题。我们导出了涉及常微分方程解的狄拉克传播子的积分表示。我们的积分表示描述了狄拉克粒子在视界之外和跨越视界直至柯西视界的动力学。
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引用次数: 0
Universal coarse geometry of spin systems 自旋系统的通用粗几何
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-23 DOI: 10.1007/s11005-025-01949-6
Ali Elokl, Corey Jones

The prospect of realizing highly entangled states on quantum processors with fundamentally different hardware geometries raises the question: to what extent does a state of a quantum spin system have an intrinsic geometry? In this paper, we propose that both states and dynamics of a spin system have a canonically associated coarse geometry, in the sense of Roe, on the set of sites in the thermodynamic limit. For a state (phi ) on an (abstract) spin system with an infinite collection of sites X, we define a universal coarse structure (mathcal {E}_{phi }) on the set X with the property that a state has decay of correlations with respect to a coarse structure (mathcal {E}) on X if and only if (mathcal {E}_{phi }subseteq mathcal {E}). We show that under mild assumptions, the coarsely connected completion ((mathcal {E}_{phi })_{con}) is stable under quasi-local perturbations of the state (phi ). We also develop in parallel a dynamical coarse structure for arbitrary quantum channels, and prove a similar stability result. We show that several order parameters of a state only depend on the coarse structure of an underlying spatial metric, and we establish a basic compatibility between the dynamical coarse structure associated with a quantum circuit (alpha ) and the coarse structure of the state (psi circ alpha ) where (psi ) is any product state.

在具有根本不同硬件几何形状的量子处理器上实现高度纠缠态的前景提出了一个问题:量子自旋系统的状态在多大程度上具有内在几何形状?在本文中,我们提出自旋系统的状态和动力学在热力学极限的位置集合上具有正则相关的粗糙几何,在Roe意义上。对于具有无穷个位置X的(抽象)自旋系统上的状态(phi ),我们定义了集合X上的一个通用粗结构(mathcal {E}_{phi }),其性质是当且仅当(mathcal {E}_{phi }subseteq mathcal {E})时,状态相对于X上的粗结构(mathcal {E})具有相关性衰减。我们证明了在温和的假设下,粗连接补全((mathcal {E}_{phi })_{con})在状态(phi )的准局部扰动下是稳定的。我们还并行开发了任意量子通道的动态粗结构,并证明了类似的稳定性结果。我们证明了一个状态的几个序参数只依赖于底层空间度量的粗结构,并且我们建立了与量子电路相关的动态粗结构(alpha )和状态的粗结构(psi circ alpha )之间的基本兼容性,其中(psi )是任何积态。
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引用次数: 0
Charges in light cones and quenched infrared radiation 光锥中的电荷和熄灭的红外辐射
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-21 DOI: 10.1007/s11005-025-01942-z
Detlev Buchholz, Fabio Ciolli, Giuseppe Ruzzi, Ezio Vasselli

The creation of electrically charged states and the resulting electromagnetic fields are considered in spacetime regions in which such experiments can actually be carried out, namely in future-directed light cones. Under the simplifying assumption of external charges, charged states are formed from neutral pairs of opposite charges, with one charge being shifted to light-like infinity. It thereby escapes observation. Despite the fact that this charge moves asymptotically at the speed of light, the resulting electromagnetic field has a well-defined energy operator that is bounded from below. Moreover, due to the spatiotemporal restrictions, the transverse electromagnetic field (the radiation) has no infrared singularities in the light cone. They are quenched and the observed radiation can be described by states in the Fock space of photons. The longitudinal field between the charges (giving rise to Gauss’s law) disappears for inertial observers in an instant. This is consistent with the fact that the underlying longitudinal photons do not manifest themselves as genuine particles. The results show that the restrictions of operations and observations to light cones, which are dictated by the arrow of time, amount to a Lorentz-invariant infrared cutoff.

带电状态的产生和由此产生的电磁场是在这样的实验实际上可以进行的时空区域,即在未来定向光锥中考虑的。在外部电荷的简化假设下,电荷态是由相反电荷的中性对形成的,其中一个电荷被移到类光无穷大。因此它逃避了观察。尽管电荷以光速渐近移动,但由此产生的电磁场具有一个定义良好的能量算符,它从下面有界。此外,由于时空的限制,横向电磁场(辐射)在光锥内不存在红外奇点。它们被淬灭,观测到的辐射可以用光子的Fock空间中的状态来描述。对于惯性观测者来说,电荷之间的纵向场(产生高斯定律)在瞬间消失了。这与潜在的纵向光子并不表现为真正的粒子这一事实是一致的。结果表明,操作和观测对光锥的限制是由时间箭头决定的,相当于洛伦兹不变的红外截止。
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引用次数: 0
The p-adic approximations of vertex functions via 3D mirror symmetry 三维镜像对称顶点函数的p进逼近
IF 1.3 3区 物理与天体物理 Q3 PHYSICS, MATHEMATICAL Pub Date : 2025-05-21 DOI: 10.1007/s11005-025-01944-x
Andrey Smirnov, Alexander Varchenko

Using the 3D mirror symmetry we construct a system of polynomials (textsf{T}_s(z)) with integral coefficients which solve the quantum differential equitation of (X=T^{*}operatorname {Gr}(k,n)) modulo (p^s), where p is a prime number. We show that the sequence (textsf{T}_s(z)) converges in the p-adic norm to the Okounkov’s vertex function of X as (srightarrow infty ). We prove that (textsf{T}_s(z)) satisfy Dwork-type congruences which lead to a new infinite product presentation of the vertex function modulo (p^s).

利用三维镜像对称构造了一个具有积分系数的多项式系统(textsf{T}_s(z)),求解了(X=T^{*}operatorname {Gr}(k,n))模(p^s)的量子微分方程,其中p为素数。我们证明了序列(textsf{T}_s(z))在p进范数收敛到X的Okounkov顶点函数(srightarrow infty )。我们证明了(textsf{T}_s(z))满足dwork型同余,从而得到顶点函数模(p^s)的一个新的无穷积表示。
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引用次数: 0
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Letters in Mathematical Physics
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