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Bloch–Landau–Zener Oscillations in Moiré Lattices 莫尔格中的Bloch-Landau-Zener振荡
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-15 DOI: 10.1002/prop.70039
Sergey K. Ivanov, Yaroslav V. Kartashov, Vladimir V. Konotop

A theory of two-dimensional Bloch–Landau–Zener (BLZ) oscillations of wavepackets in incommensurate moiré lattices under the influence of a weak linear gradient is developed. Unlike periodic systems, aperiodic lattices lack translational symmetry and therefore do not exhibit a conventional band-gap structure. Instead, they feature a mobility edge, above which (in the optical context) all modes become localized. When a linear gradient is applied to a moiré lattice, it enables energy transfer between two or several localized modes, leading to the oscillatory behavior referred to as BLZ oscillations. This phenomenon represents simultaneous tunneling in real space and propagation constant (energy) space, and it arises when quasi-resonance condition for propagation constants and spatial proximity of interacting modes (together constituting a selection rule) are met. The selection rule is controlled by the linear gradient, whose amplitude and direction play a crucial role in determining the coupling pathways and the resulting dynamics. A multimode model describing BLZ oscillations in the linear regime is derived, and effects of both attractive and repulsive nonlinearities on their dynamics are analyzed. The proposed framework can be readily extended to other physical systems, including cold atoms and Bose–Einstein condensates in aperiodic potentials.

本文提出了在弱线性梯度作用下,不对称波格中波包的二维Bloch-Landau-Zener振荡理论。与周期系统不同,非周期晶格缺乏平移对称性,因此不表现出传统的带隙结构。相反,它们具有移动边缘,在此之上(在光学环境中)所有模式都本地化。当一个线性梯度被应用到一个莫尔格栅,它使两个或几个局部模式之间的能量转移,导致振荡行为被称为BLZ振荡。这种现象是在实空间和传播常数(能量)空间同时隧穿的现象,当传播常数和相互作用模式的空间接近性(共同构成一个选择规则)满足准共振条件时就会出现。选择规则由线性梯度控制,其振幅和方向在决定耦合路径和产生的动力学中起着至关重要的作用。推导了描述BLZ线性振荡的多模态模型,分析了吸引和排斥非线性对其动力学的影响。所提出的框架可以很容易地扩展到其他物理系统,包括冷原子和非周期势的玻色-爱因斯坦凝聚。
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引用次数: 0
Black Hole in the Quantum Oppenheimer–Snyder Model: Long Lived Modes and the Overtones' Behavior 量子奥本海默-斯奈德模型中的黑洞:长寿命模式和泛音的行为
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-11 DOI: 10.1002/prop.70038
Antonina F. Zinhailo

A quantum-corrected black hole metric has been derived in [Lewandowski et al., Phys. Rev. Lett. 130 (2023) 10, 101501] within the context of the quantum Oppenheimer–Snyder model inspired by loop quantum cosmology. Using the Frobenius method, we have obtained precise values for the fundamental quasinormal modes and the first few overtones for scalar and electromagnetic perturbations. Our results reveal that, unlike the fundamental mode, the overtones exhibit high sensitivity to quantum corrections, leading to qualitatively new spectral behavior. Notably, our findings suggest that modes with real oscillation frequencies approaching zero appear in the spectrum. The existence of arbitrarily long-lived modes, known as quasi-resonances is also demonstrated.

一个量子校正的黑洞度量已经在[Lewandowski et al., Phys]中得到。在受环量子宇宙学启发的量子奥本海默-施耐德模型的背景下。通讯,130(2023),10,101501。利用Frobenius方法,我们得到了准正态模的精确值以及标量和电磁扰动的前几个泛音。我们的研究结果表明,与基本模式不同,泛音对量子修正表现出高灵敏度,从而导致定性的新光谱行为。值得注意的是,我们的研究结果表明,在频谱中出现了实际振荡频率接近零的模态。还证明了任意长寿命模式的存在,称为准共振。
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引用次数: 0
Issue Information: Fortschritte der Physik 9–10 / 2025 检索日期:2015-09-10。
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-09 DOI: 10.1002/prop.70043
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引用次数: 0
Traversable Wormholes in f ( R ) $f(R)$ Gravity: Influence of Global Monopole Charge and Energy Conditions f(R)$ f(R)$重力中的可穿越虫洞:全球单极子电荷和能量条件的影响
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-08 DOI: 10.1002/prop.70034
Hamna Asad, Muhammad Yousaf, Ujala Zafar, Javlon Rayimbaev, Adilbek Dauletov
<p>In this manuscript, the properties of topologically charged Morris–Thorne wormholes (WHs) are investigated within the framework of <span></span><math> <semantics> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> <annotation>$f(R)$</annotation> </semantics></math> gravity, which modifies general relativity by introducing a generic function of Ricci scalar <span></span><math> <semantics> <mi>R</mi> <annotation>$R$</annotation> </semantics></math>. The study primarily focuses on how different choices of shape functions influence the physical characteristics of WH models under consideration. To explore the viability of such WHs, the field equations in <span></span><math> <semantics> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> <annotation>$f(R)$</annotation> </semantics></math> gravity are solved by considering an anisotropic energy-momentum tensor (EMT). A key aspect of this investigation is the analysis of the matter content supporting these WHs, particularly whether it satisfies or violates the classical energy conditions, such as the Null, Weak, and Strong Energy Conditions. Unlike traditional WH solutions, which often require exotic matter with negative energy density, this study aims to examine the possibility of sustaining these structures with non-exotic matter. Also, the influence of the global monopole charge are explored and the correction terms arising from <span></span><math> <semantics> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> <annotation>$f(R)$</annotation> </semantics></math> modifications on the energy conditions, providing insights into their role in determining the physical plausibility of these WHs. The repulsive or attractive nature of the WHs is assessed by calculating the anisotropy parameter, which measures the deviation from isotropic pressure conditions. The results indicate that the global monopole parameter and the modifications introduced by <span></span><math> <semantics> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> <annotation>$f(R)$</annotation> </semantics></math> gravity significantly affect the energy conditions, thereby controlling the physical viability of these WHs. This study contributes to a deeper understanding of traversable WHs in alternative gravity theories, potentially offering new avenues for theoretical and astrophysical research into exot
本文在f(R)$ f(R)$引力的框架下研究了拓扑带电的Morris-Thorne虫洞(WHs)的性质,通过引入Ricci标量R$ R$的一般函数对广义相对论进行了修正。本研究主要关注形状函数的不同选择如何影响所考虑的WH模型的物理特性。为了探索这种WHs的可行性,通过考虑各向异性能量动量张量(EMT)来求解f(R)$ f(R)$重力中的场方程。这项研究的一个关键方面是分析支持这些WHs的物质含量,特别是它是否满足或违反经典能量条件,如零、弱和强能量条件。与传统的WH解决方案不同,传统的WH解决方案通常需要负能量密度的外来物质,而本研究旨在研究用非外来物质维持这些结构的可能性。此外,还探讨了全球单极子电荷的影响以及f(R)$ f(R)$修正对能量条件产生的修正项,从而深入了解它们在确定这些WHs的物理合理性方面的作用。通过计算各向异性参数来评估水阱的排斥或吸引性质,该参数测量了与各向同性压力条件的偏差。结果表明,全局单极子参数和f(R)$ f(R)$重力引入的修正显著影响能量条件,从而控制这些黑洞的物理生存能力。这项研究有助于在替代引力理论中更深入地理解可穿越的WHs,可能为奇异时空结构的理论和天体物理学研究提供新的途径。
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引用次数: 0
Linear Flux Origins of κ $kappa$ -Geometry: From Lie Non-Commutativity to 3-Lie Nambu Space κ $kappa$ -几何的线性通量原点:从Lie非交换性到3-Lie Nambu空间
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-01 DOI: 10.1002/prop.70036
Mir Faizal, Arshid Shabir

Linear background fluxes offer a unified origin for non-commutative and non-associative geometries in string and M-theory. Revisiting the open string with a linearly varying Kalb–Ramond field, we recover kappa-Minkowski space as a Jordanian deformation of Poincaré symmetry. Lifting the construction to an open M2-brane in a linear three-form background yields a kappa-Nambu triple bracket that realises the three-Lie algebra of the Bagger–Lambert–Gustavsson model and exposes an underlying quasi-Hopf two-algebra. A Bopp-shift quantisation reveals that isotropic potentials are unaltered at leading order, whereas anisotropic ones receive Planck-suppressed corrections, and gerbe holonomy discretises the deformation scale. Inspired by the membrane bracket, we build a cubic-matrix extension of the BFSS model whose higher-Lie structure supplies the long-missing five-brane central charge and reproduces the expected N3$N^{3}$ energy scaling of coincident M5-branes. These results establish linear fluxes as the minimal ingredients that interpolate smoothly from Moyal to Lie and Nambu deformations, providing concrete, anomaly-free models for non-associative field theories and five-brane dynamics.

线性背景通量为弦和m理论中的非交换和非关联几何提供了一个统一的原点。重新考察具有线性变化的Kalb-Ramond场的开放弦,我们将kappa-Minkowski空间恢复为poincar对称的约旦变形。将结构提升到线性三形式背景中的开放m2膜,产生kappa-Nambu三重支架,实现了Bagger-Lambert-Gustavsson模型的三李代数,并暴露了潜在的准hopf二代数。bopp位移量化表明,各向同性电位在阶上不变,而各向异性电位则受到普朗克抑制的修正,并且gerbe完整度使变形尺度离散。受膜支架的启发,我们建立了BFSS模型的立方矩阵扩展,该模型的高李结构提供了长期缺失的五膜中心电荷,并再现了一致的m5膜的预期n3 $N^{3}$能量标度。这些结果建立了线性通量作为从Moyal到Lie和Nambu变形平滑插值的最小成分,为非关联场论和五膜动力学提供了具体的,无异常的模型。
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引用次数: 0
Coherence, Transport, and Chaos in 1D Bose–Hubbard Model: Disorder vs. Stark Potential 一维玻色-哈伯德模型中的相干性、输运和混沌:无序与斯塔克势
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-20 DOI: 10.1002/prop.70035
Asad Ali, M.I. Hussain, Saif Al-Kuwari, M. T. Rahim, H. Kuniyil, Seyed Mohammad Hosseiny, Jamileh Seyed-Yazdi, Hamid Arian Zad, Saeed Haddadi

Quantum coherence and phase transitions are studied in a finite one-dimensional Bose–Hubbard model using exact diagonalization under thermal fluctuations, a Stark potential, and disorder. The condensate fraction, superfluid fraction, visibility, number fluctuations, and the 1$ell _1$-norm of coherence are computed to characterize the Mott insulator–superfluid transition. Although finite-size effects prevent a sharp transition, ground-state properties reveal signatures of quantum criticality. Thermal fluctuations can enhance coherence via tunneling, a Stark potential promotes localization, and disorder suppresses global superfluidity while preserving local coherence. These results highlight how disorder, tilt, and temperature reshape coherence and offer insights for quantum simulation and strongly correlated phases. For systems up to six sites with unit filling, a spectral analysis is also performed through the metric mean gap ratio (MGR). However, limited statistics due to the small system size and computational constraints prevent a complete characterization of quantum chaos, yielding only approximate signatures.

在有限一维玻色-哈伯德模型中,在热涨落、斯塔克势和无序下,利用精确对角化研究了量子相干性和相变。计算了凝聚分数、超流体分数、可见性、数波动和相干模的_1$ ell _1$ -范数来表征Mott绝缘体-超流体跃迁。虽然有限尺寸效应阻止了急剧转变,但基态性质揭示了量子临界的特征。热波动可以通过隧道效应增强相干性,斯塔克势促进局部化,无序抑制全局超流动性,同时保持局部相干性。这些结果突出了无序、倾斜和温度如何重塑相干性,并为量子模拟和强相关相提供了见解。对于多达六个站点的单位填充系统,还可以通过度量平均间隙比(MGR)进行光谱分析。然而,由于系统尺寸小和计算限制,有限的统计数据阻碍了量子混沌的完整表征,只能产生近似的特征。
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引用次数: 0
Framework for Estimating Cosmological Parameters using Observational Cosmology and Artificial Neural Networks in f ( R , T ) $f(R, T)$ Gravity f(R, T)$ f(R, T)$重力中使用观测宇宙学和人工神经网络估计宇宙学参数的框架
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-16 DOI: 10.1002/prop.70032
Lokesh Kumar Sharma, Anil Kumar Yadav, Suresh Parekh, Nafis Ahmad, A.M. Alshehri
<p>An exact solution of bulk viscous Bianchi I universe is proposed in <span></span><math> <semantics> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>,</mo> <mi>T</mi> <mo>)</mo> </mrow> <annotation>$f(R,T)$</annotation> </semantics></math> theory of gravity and its free parameters are probed using Bayesian MCMC and Artificial neural networks (ANNs) methods. In cosmology, analyzing observable evidence is critical for evaluating theoretical models of the universe. The ANNs are strong and adaptable computational tools for data modeling, and they have lately been used to analyze cosmic data. This study introduces ANNs and discusses their applications in cosmology. A general overview of neural networks is provided as well as technical specifics. Their capabilities in cosmological data modeling, numerical challenges, and star object categorization are demonstrated using three cases. ANNs provide intriguing properties that make them feasible options for data analysis in cosmological study. Parameters are estimated using a code called CoLFI, which combines the benefits of ANNs and can be used in any complex model parameter estimation across a variety of scientific domains. When the likelihood function is unmanageable or cosmological models are intricate and resource-intensive, CoLFI offers a more effective method of parameter estimation. The model provides a mechanism to explain the late-time acceleration of the universe by attributing it to modified gravitational dynamics and bulk viscous effects, rather than a distinct dark energy component. The transition Redshift from deceleration to acceleration phase is obtained as <span></span><math> <semantics> <mrow> <msub> <mi>z</mi> <mi>t</mi> </msub> <mo>=</mo> <mn>0</mn> <mo>.</mo> <msubsup> <mn>715</mn> <mrow> <mo>−</mo> <mn>0.022</mn> </mrow> <mrow> <mo>+</mo> <mn>0.019</mn> </mrow> </msubsup> </mrow> <annotation>$z_{t} = 0.715^{+0.019}_{-0.022}$</annotation> </semantics></math> and <span></span><math> <semantics> <mrow> <msub> <mi>z</mi> <mi>t</mi> </msub> <mo>=</mo> <mn>0</mn> <mo>.</mo> <msubsup> <mn>702</mn> <mrow> <mo>−</mo> <mn>0.009</mn
在f(R,T)$ f(R,T)$重力理论中提出了体积粘性Bianchi I宇宙的精确解,并利用贝叶斯MCMC和人工神经网络(ann)方法对其自由参数进行了探测。在宇宙学中,分析可观测证据对于评估宇宙的理论模型至关重要。人工神经网络是数据建模的强大且适应性强的计算工具,它们最近被用于分析宇宙数据。本文介绍了人工神经网络,并讨论了其在宇宙学中的应用。提供了神经网络的总体概述以及技术细节。它们在宇宙学数据建模、数值挑战和恒星对象分类方面的能力通过三个案例进行了演示。人工神经网络提供了有趣的特性,使其成为宇宙学研究中数据分析的可行选择。使用名为CoLFI的代码估计参数,该代码结合了人工神经网络的优点,可用于各种科学领域的任何复杂模型参数估计。当似然函数难以管理或宇宙模型复杂且资源密集时,CoLFI提供了一种更有效的参数估计方法。该模型提供了一种机制来解释宇宙的后期加速,将其归因于修正的引力动力学和体积粘性效应,而不是一个独特的暗能量成分。从减速阶段到加速阶段的过渡红移为zt = 0。715−0.022 +0.019 $z_{t} = 0.715^{+0.019}_{-0.022}$, z t = 0。z_{t} = 0.702^{+0.010}_{-0.009}$,分别由贝叶斯和ann方法得到。研究了模型的一些物理和几何特征。
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引用次数: 0
Recursive Relations for the S-matrix of Liouville Theory Liouville理论中s矩阵的递归关系
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-16 DOI: 10.1002/prop.70033
George Jorjadze, Lado Razmadze, Stefan Theisen

The relation between the vertex operators of the in and out fields in Liouville theory is analyzed. This is used to derive equations for the S-matrix, from which a recursive relation for the normal symbol of the S-matrix for discrete center-of-mass momenta is obtained. Its solution is expressed as multiple contour-integrals of a generalized Dotsenko–Fateev type. This agrees with the functional integral representation of the scattering matrix of Liouville theory, which had been proposed previously.

分析了Liouville理论中内外场顶点算子之间的关系。利用这一方法推导出s矩阵的方程,得到离散质心动量s矩阵法向符号的递推关系。其解被表示为广义Dotsenko-Fateev型的多个轮廓积分。这与先前提出的Liouville理论中散射矩阵的泛函积分表示一致。
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引用次数: 0
A Deep Dive into Classical and Topological CFT Thermodynamics in Lifshitz and Hyperscaling Violating Black Holes 深入探讨经典和拓扑CFT热力学在Lifshitz和超尺度违反黑洞
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-14 DOI: 10.1002/prop.70030
Mohammad Ali S. Afshar, Mohammad Reza Alipour, Saeed Noori Gashti, Jafar Sadeghi

To effectively utilize the AdS/CFT correspondence, a precise set of rules must be established to guide the translation of computed quantities in the gravitational sector into their CFT counterparts, and vice versa. This framework is commonly referred to as the holographic dictionary. The formulation of such dictionaries opens a two-way gateway, allowing researchers to extend theoretical principles and findings from one domain into the other for further exploration and study. The development of a holographic dictionary for Lifshitz black holes and hyperscaling violation (HSV) models has provided an essential foundation for studying CFT thermodynamics and phase behavior of these black holes. Based on this framework, the study will investigate their thermodynamic properties using two distinct approaches. In the first step, the work adopts the classical and traditional method, identifying critical points to examine the behavior of the free energy function as a function of temperature near the critical boundary. By analyzing its behavior, the work will study phase transitions and then proceed to evaluate the stability of the models. In the next step, to compare both methodologies and highlight their equivalence—particularly demonstrating the accessibility of the topological method compared to the classical approach—the study will analyze phase behavior through the lens of topological charges.

为了有效地利用AdS/CFT对应,必须建立一套精确的规则来指导引力领域计算量与CFT对应量的转换,反之亦然。这个框架通常被称为全息字典。这种词典的制定打开了一个双向的门户,允许研究人员将理论原理和发现从一个领域扩展到另一个领域,以进一步探索和研究。Lifshitz黑洞全息字典和超尺度破坏(HSV)模型的开发为研究这些黑洞的CFT热力学和相行为提供了必要的基础。基于这个框架,本研究将使用两种不同的方法来研究它们的热力学性质。首先,本文采用经典方法和传统方法,确定临界边界附近的临界点,考察自由能函数随温度的变化规律。通过分析其行为,工作将研究相变,然后继续评估模型的稳定性。在下一步中,为了比较两种方法并强调它们的等效性,特别是展示拓扑方法与经典方法相比的可及性,研究将通过拓扑电荷的透镜分析相行为。
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引用次数: 0
Probing the Black Hole Interior with Holographic Entanglement Entropy and the Role of AdS/BCFT Correspondence 用全息纠缠熵探测黑洞内部及AdS/BCFT对应的作用
IF 7.8 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-14 DOI: 10.1002/prop.70031
Fabiano F. Santos

This work is explored the black hole information loss paradox, a fundamental challenge in theoretical physics. Insights are proposed using Holographic Entanglement Entropy (HEE) and the AdS/BCFT correspondence within Horndeski gravity. The work is revisited the time-dependent behavior of HEE to probe black hole interiors and examines its implications for the Page curve, which is described the entropy evolution of Hawking radiation. The relationship between conformal field theory (CFT) microstates and black hole thermodynamics through the AdS/BCFT correspondence is also discussed, suggesting that only a subset of microstates corresponds to black holes with smooth interiors, while others may involve firewalls. Black hole thermal entropy is extended to time-dependent entanglement entropy, offering a perspective on the interplay between quantum mechanics, thermodynamics, and gravity.

本工作探讨了黑洞信息损失悖论,这是理论物理学中的一个基本挑战。利用全息纠缠熵(HEE)和Horndeski引力中的AdS/BCFT对应,提出了新的见解。这项工作重新审视了HEE的时间依赖行为,以探测黑洞内部,并研究了它对霍金辐射熵演化所描述的Page曲线的影响。通过AdS/BCFT对应关系讨论了共形场论(CFT)微态与黑洞热力学之间的关系,表明只有一部分微态对应于内部光滑的黑洞,而其他微态可能涉及防火墙。黑洞热熵扩展到与时间相关的纠缠熵,提供了量子力学、热力学和引力之间相互作用的视角。
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引用次数: 0
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