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Classical limits of Hilbert bimodules as symplectic dual pairs 作为交映对偶的希尔伯特双模的经典极限
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-05-21 DOI: 10.1142/s0129055x24500260
Benjamin H. Feintzeig, Jer Steeger

Hilbert bimodules are morphisms between C*-algebraic models of quantum systems, while symplectic dual pairs are morphisms between Poisson geometric models of classical systems. Both of these morphisms preserve representation-theoretic structures of the relevant types of models. Previously, it has been shown that one can functorially associate certain symplectic dual pairs to Hilbert bimodules through strict deformation quantization. We show that, in the inverse direction, strict deformation quantization also allows one to functorially take the classical limit of a Hilbert bimodule to reconstruct a symplectic dual pair.

希尔伯特双模是量子系统 C* 代数模型之间的变形,而交映对偶是经典系统泊松几何模型之间的变形。这两种变形都保留了相关类型模型的表示理论结构。在此之前,已经有研究表明,通过严格的变形量子化,我们可以把某些交映对偶与希尔伯特双模子函数化地联系起来。我们证明,从反方向来看,严格变形量子化也允许人们从希尔伯特双模子的经典极限出发,以扇形方式重构交映对偶。
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引用次数: 0
Scattering theory for some non-self-adjoint operators 一些非自相加算子的散射理论
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-05-15 DOI: 10.1142/s0129055x24500235
Nicolas Frantz
<p>We consider a non-self-adjoint <span><math altimg="eq-00001.gif" display="inline" overflow="scroll"><mi>H</mi></math></span><span></span> acting on a complex Hilbert space. We suppose that <span><math altimg="eq-00002.gif" display="inline" overflow="scroll"><mi>H</mi></math></span><span></span> is of the form <span><math altimg="eq-00003.gif" display="inline" overflow="scroll"><mi>H</mi><mo>=</mo><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub><mo stretchy="false">+</mo><mi>C</mi><mi>W</mi><mi>C</mi></math></span><span></span> where <span><math altimg="eq-00004.gif" display="inline" overflow="scroll"><mi>C</mi></math></span><span></span> is a bounded, positive definite and relatively compact with respect to <span><math altimg="eq-00005.gif" display="inline" overflow="scroll"><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span><span></span>, and <span><math altimg="eq-00006.gif" display="inline" overflow="scroll"><mi>W</mi></math></span><span></span> is bounded. We suppose that <span><math altimg="eq-00007.gif" display="inline" overflow="scroll"><mi>C</mi><msup><mrow><mo stretchy="false">(</mo><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub><mo stretchy="false">−</mo><mi>z</mi><mo stretchy="false">)</mo></mrow><mrow><mo stretchy="false">−</mo><mn>1</mn></mrow></msup><mi>C</mi></math></span><span></span> is uniformly bounded in <span><math altimg="eq-00008.gif" display="inline" overflow="scroll"><mi>z</mi><mo>∈</mo><mi>ℂ</mi><mo stretchy="false">∖</mo><mi>ℝ</mi></math></span><span></span>. We define the regularized wave operators associated to <span><math altimg="eq-00009.gif" display="inline" overflow="scroll"><mi>H</mi></math></span><span></span> and <span><math altimg="eq-00010.gif" display="inline" overflow="scroll"><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span><span></span> by <span><math altimg="eq-00011.gif" display="inline" overflow="scroll"><msub><mrow><mi>W</mi></mrow><mrow><mo stretchy="false">±</mo></mrow></msub><mo stretchy="false">(</mo><mi>H</mi><mo>,</mo><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub><mo stretchy="false">)</mo><mo>:</mo><mo>=</mo><msub><mrow><mstyle><mtext mathvariant="normal">s-lim</mtext></mstyle></mrow><mrow><mi>t</mi><mo>→</mo><mi>∞</mi></mrow></msub><msup><mrow><mi>e</mi></mrow><mrow><mo stretchy="false">±</mo><mi>i</mi><mi>t</mi><mi>H</mi></mrow></msup><msub><mrow><mi>r</mi></mrow><mrow><mo stretchy="false">∓</mo></mrow></msub><mo stretchy="false">(</mo><mi>H</mi><mo stretchy="false">)</mo><msub><mrow><mi mathvariant="normal">Π</mi></mrow><mrow><mstyle><mtext mathvariant="normal">p</mtext></mstyle></mrow></msub><msup><mrow><mo stretchy="false">(</mo><msup><mrow><mi>H</mi></mrow><mrow><mo stretchy="false">⋆</mo></mrow></msup><mo stretchy="false">)</mo></mrow><mrow><mo>⊥</mo></mrow></msup><msup><mrow><mi>e</mi></mrow><mrow><mo stretchy="false">∓</mo><mi>i</mi><mi>t</mi><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub><
我们考虑一个作用于复数希尔伯特空间的非自相加 H。我们假设 H 是 H=H0+CWC 形式,其中 C 是有界、正定且相对于 H0 紧凑的,W 是有界的。我们假设 C(H0-z)-1C 在 z∈ℂ∖ℝ 中均匀有界。我们用 W±(H,H0)定义与 H 和 H0 相关的正则化波算子:=s-limt→∞e±itHr∓(H)Πp(H⋆)⊥e∓itH0,其中Πp(H⋆)是投影到与 H⋆的特征值相关的所有广义特征空间的直和上,r∓是一个有理函数,用于正则化 H 的 "入射/出射频谱奇异性"。我们证明了正则化波算子的存在并研究了其性质。特别是,我们证明了如果 H 没有任何谱奇异性,它们就是渐近完全的。
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We suppose that &lt;span&gt;&lt;math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; is of the form &lt;span&gt;&lt;math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;+&lt;/mo&gt;&lt;mi&gt;C&lt;/mi&gt;&lt;mi&gt;W&lt;/mi&gt;&lt;mi&gt;C&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; where &lt;span&gt;&lt;math altimg=\"eq-00004.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;C&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; is a bounded, positive definite and relatively compact with respect to &lt;span&gt;&lt;math altimg=\"eq-00005.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;, and &lt;span&gt;&lt;math altimg=\"eq-00006.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;W&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; is bounded. We suppose that &lt;span&gt;&lt;math altimg=\"eq-00007.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;C&lt;/mi&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;−&lt;/mo&gt;&lt;mi&gt;z&lt;/mi&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;−&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mi&gt;C&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; is uniformly bounded in &lt;span&gt;&lt;math altimg=\"eq-00008.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;z&lt;/mi&gt;&lt;mo&gt;∈&lt;/mo&gt;&lt;mi&gt;ℂ&lt;/mi&gt;&lt;mo stretchy=\"false\"&gt;∖&lt;/mo&gt;&lt;mi&gt;ℝ&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;. We define the regularized wave operators associated to &lt;span&gt;&lt;math altimg=\"eq-00009.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; and &lt;span&gt;&lt;math altimg=\"eq-00010.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; by &lt;span&gt;&lt;math altimg=\"eq-00011.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;W&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;±&lt;/mo&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;mo&gt;,&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;mo&gt;:&lt;/mo&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;s-lim&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;t&lt;/mi&gt;&lt;mo&gt;→&lt;/mo&gt;&lt;mi&gt;∞&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;e&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;±&lt;/mo&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;mi&gt;t&lt;/mi&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;r&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;∓&lt;/mo&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi mathvariant=\"normal\"&gt;Π&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;p&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;⋆&lt;/mo&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo&gt;⊥&lt;/mo&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mi&gt;e&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo stretchy=\"false\"&gt;∓&lt;/mo&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;mi&gt;t&lt;/mi&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;H&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;","PeriodicalId":54483,"journal":{"name":"Reviews in Mathematical Physics","volume":"67 1","pages":""},"PeriodicalIF":1.8,"publicationDate":"2024-05-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141146867","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Renormalization on the DFR quantum spacetime DFR 量子时空的重正化
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-05-08 DOI: 10.1142/s0129055x24600055
Juan F. López, Andrés F. Reyes-Lega

An approach to renormalization of scalar fields on the Doplicher–Fredenhagen–Roberts (DFR) quantum spacetime is presented. The effective nonlocal theory obtained through the use of states of optimal localization for the quantum spacetime is reformulated in the language of (perturbative) Algebraic Quantum Field Theory. The structure of the singularities associated to the nonlocal kernel that codifies the effects of non-commutativity is analyzed using the tools of microlocal analysis.

本文提出了一种在多普勒-弗里登哈根-罗伯茨(DFR)量子时空中对标量场进行重正化的方法。用(微扰)代数量子场论的语言重新表述了通过使用量子时空最优局域化状态获得的有效非局域理论。使用微局域分析工具分析了与编码非交换性效应的非局域核相关的奇点结构。
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引用次数: 0
Perturbation theory and canonical coordinates in celestial mechanics 天体力学中的扰动理论和典型坐标
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-04-17 DOI: 10.1142/s0129055x24300061
Gabriella Pinzari

KAM theory owes most of its success to its initial motivation: the application to problems of celestial mechanics. The masterly application was offered by Arnold in the 60s who worked out a theorem, that he named the “Fundamental Theorem” (FT), especially designed for the planetary problem. However, FT could be really used at that purpose only when, about 50 years later, a set of coordinates constructively taking the invariance by rotation and close-to-integrability into account was used. Since then, some progress has been done in the symplectic assessment of the problem, and here we review such results.

KAM 理论的成功主要归功于其最初的动机:应用于天体力学问题。60 年代,阿诺德提出了一个专门用于行星问题的定理,并将其命名为 "基本定理"(FT)。然而,只有在大约 50 年后,一套建设性地考虑到旋转不变性和近似可动性的坐标被使用时,FT 才能真正用于这一目的。从那时起,对该问题的交映评估取得了一些进展,在此我们对这些成果进行回顾。
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引用次数: 0
Feynman checkers: External electromagnetic field and asymptotic properties 费曼跳棋外部电磁场和渐近特性
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-04-13 DOI: 10.1142/s0129055x2450017x
Fedor Ozhegov

In this paper, we study Feynman checkers, one of the most elementary models of electron motion. It is also known as a one-dimensional quantum walk or an Ising model at an imaginary temperature. We add the simplest non-trivial electromagnetic field and find the limits of the resulting model for small lattice step and large time, analogous to the results by Narlikar from 1972 and Grimmet–Jason–Scudo from the 2000s. It turns out that the limits in the model with the added field are obtained from the ones without field by mass renormalization. Also, we find an exact solution of the resulting model.

本文研究的是费曼跳棋,它是最基本的电子运动模型之一。它也被称为一维量子行走或虚温下的伊辛模型。我们加入了最简单的非三维电磁场,并找到了由此产生的模型在小晶格步长和大时间下的极限,类似于 1972 年的 Narlikar 和 2000 年代的 Grimmet-Jason-Scudo 的结果。结果表明,有附加场的模型的极限是通过质量重正化从无附加场的模型中得到的。此外,我们还找到了由此模型的精确解。
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引用次数: 0
Some contributions to k-contact Lagrangian field equations, symmetries and dissipation laws 对 k 接触拉格朗日场方程、对称性和耗散定律的一些贡献
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-04-13 DOI: 10.1142/s0129055x24500193
Xavier Rivas, Modesto Salgado, Silvia Souto

It is well known that k-contact geometry is a suitable framework to deal with non-conservative field theories. In this paper, we study some relations between solutions of the k-contact Euler–Lagrange equations, symmetries, dissipation laws and Newtonoid vector fields. We review the k-contact Euler–Lagrange equations written in terms of k-vector fields and sections and provide new results relating the solutions in both approaches. We also study different kinds of symmetries depending on the structures they preserve: natural (preserving the Lagrangian function), dynamical (preserving the solutions), and k-contact (preserving the underlying geometric structures) symmetries. For some of these symmetries, we provide Noether-like theorems relating symmetries and dissipation laws. We also analyze the relation between k-contact symmetries and Newtonoid vector fields. Throughout the paper, we will use the damped vibrating string as our main illustrative example.

众所周知,k-接触几何是处理非守恒场论的合适框架。在本文中,我们研究了 k-contact Euler-Lagrange 方程的解、对称性、耗散律和牛顿矢量场之间的一些关系。我们回顾了用 k 向量场和截面写成的 k-contact Euler-Lagrange 方程,并提供了与这两种方法的解相关的新结果。我们还根据对称性所保留的结构研究了不同类型的对称性:自然对称性(保留拉格朗日函数)、动力学对称性(保留解)和 k 接触对称性(保留底层几何结构)。对于其中一些对称性,我们提供了与对称性和耗散规律相关的诺特定理。我们还分析了 k 接触对称性与牛顿矢量场之间的关系。在整篇论文中,我们将以阻尼振动弦为例进行说明。
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引用次数: 0
Complex translation methods and its application to resonances for quantum walks 复杂平移方法及其在量子行走共振中的应用
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-04-10 DOI: 10.1142/s0129055x24500181
Kenta Higuchi, Hisashi Morioka

In this paper, some properties of resonances for multi-dimensional quantum walks are studied. Resonances for quantum walks are defined as eigenvalues of complex translated time evolution operators in the pseudo momentum space. For some typical cases, we show some results of existence or nonexistence of resonances. One is a perturbation of an elastic scattering of a quantum walk which is an analogue of classical mechanics. Another one is a shape resonance model which is a perturbation of a quantum walk with a non-penetrable barrier.

本文研究了多维量子漫步共振的一些特性。量子漫步的共振被定义为伪动量空间中复译时间演化算子的特征值。对于一些典型情况,我们展示了共振存在或不存在的一些结果。一种情况是量子行走的弹性散射扰动,这是经典力学的一种模拟。另一个是形状共振模型,它是量子漫步的扰动,带有不可穿透的障碍。
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引用次数: 0
Homotopical foundations of parametrized quantum spin systems 参数化量子自旋系统的同域基础
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-03-16 DOI: 10.1142/s0129055x24600031
Agnès Beaudry, Michael Hermele, Juan Moreno, Markus J. Pflaum, Marvin Qi, Daniel D. Spiegel

In this paper, we present a homotopical framework for studying invertible gapped phases of matter from the point of view of infinite spin lattice systems, using the framework of algebraic quantum mechanics. We define the notion of quantum state types. These are certain lax-monoidal functors from the category of finite-dimensional Hilbert spaces to the category of topological spaces. The universal example takes a finite-dimensional Hilbert space to the pure state space of the quasi-local algebra of the quantum spin system with Hilbert space at each site of a specified lattice. The lax-monoidal structure encodes the tensor product of states, which corresponds to stacking for quantum systems. We then explain how to formally extract parametrized phases of matter from quantum state types, and how they naturally give rise to -spaces for an operad we call the “multiplicative” linear isometry operad. We define the notion of invertible quantum state types and explain how the passage to phases for these is related to group completion. We also explain how invertible quantum state types give rise to loop-spectra. Our motivation is to provide a framework for constructing Kitaev’s loop-spectrum of bosonic invertible gapped phases of matter. Finally, as a first step toward understanding the homotopy types of the loop-spectra associated to invertible quantum state types, we prove that the pure state space of any UHF algebra is simply connected.

在本文中,我们从无限自旋晶格系统的角度,利用代数量子力学的框架,提出了研究物质可逆间隙相的同调框架。我们定义了量子态类型的概念。它们是从有限维希尔伯特空间范畴到拓扑空间范畴的某些涣散单调函数。通用范例将有限维希尔伯特空间ℋ转换为量子自旋系统准局部代数的纯态空间,其希尔伯特空间ℋ位于指定晶格的每个位置。单轴结构编码了状态的张量乘积,相当于量子系统的堆积。然后,我们解释了如何从量子态类型中正式提取参数化的物质相,以及它们如何自然地为我们称之为 "乘法 "线性等距操作数的操作数产生ℰ∞空间。我们定义了可逆量子态类型的概念,并解释了这些类型的相位传递与群完备的关系。我们还解释了可逆量子态类型如何产生环谱。我们的动机是为构建基塔耶夫的玻色可逆间隙物质相的环谱提供一个框架。最后,作为理解与可逆量子态类型相关的环谱同调类型的第一步,我们证明了任何超高频代数的纯态空间都是简单连接的。
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引用次数: 0
Lattice Green functions for pedestrians: Exponential decay 行人的格点绿色函数指数衰减
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-03-12 DOI: 10.1142/s0129055x2430005x
Wojciech Dybalski, Alexander Stottmeister, Yoh Tanimoto

The exponential decay of lattice Green functions is one of the main technical ingredients of the Bałaban’s approach to renormalization. We give here a self-contained proof, whose various ingredients were scattered in the literature. The main sources of exponential decay are the Combes–Thomas method and the analyticity of the Fourier transforms. They are combined using a renormalization group equation and the method of images.

格点格林函数的指数衰减是巴瓦班重正化方法的主要技术要素之一。我们在此给出一个自足的证明,其各种成分散见于文献中。指数衰减的主要来源是康伯斯-托马斯方法和傅立叶变换的解析性。我们使用重正化群方程和图像方法将它们结合起来。
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引用次数: 0
A result about the classification of quantum covariance matrices based on their eigenspectra 基于量子协方差矩阵特征谱的量子协方差矩阵分类结果
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2024-03-11 DOI: 10.1142/s0129055x2460002x
Arik Avagyan

The set of covariance matrices of a continuous-variable quantum system with a finite number of degrees of freedom is a strict subset of the set of real positive-definite matrices (PDMs) due to Heisenberg’s uncertainty principle. This has the implication that, in general, not every orthogonal transform of a quantum covariance matrix (CM) produces a PDM that obeys the uncertainty principle. A natural question thus arises, to find the set of quantum covariance matrices consistent with a given eigenspectrum. For the special class of pure Gaussian states the set of quantum covariance matrices with a given eigenspectrum consists of a single orbit of the action of the orthogonal symplectic group. The eigenspectrum of a CM of a state in this class is composed of pairs that each multiply to one. Our main contribution is finding a non-trivial class of eigenspectra with the property that the set of quantum covariance matrices corresponding to any eigenspectrum in this class are related by orthogonal symplectic transformations. We show that all non-degenerate eigenspectra with this property must belong to this class, and that the set of such eigenspectra coincides with the class of non-degenerate eigenspectra that identify the physically relevant thermal and squeezing parameters of a Gaussian state.

根据海森堡不确定性原理,具有有限自由度的连续可变量子系统的协方差矩阵集合是实正定矩阵(PDM)集合的严格子集。这意味着,一般来说,并非量子协方差矩阵(CM)的每一次正交变换都能产生符合不确定性原理的 PDM。因此,一个自然而然的问题出现了,即如何找到与给定特征谱一致的量子协方差矩阵集合。对于纯高斯态这一特殊类别,具有给定特征谱的量子协方差矩阵集合由正交交映组作用的单一轨道组成。该类态的 CM 的高光谱由各乘以一的一对组成。我们的主要贡献是找到了一类非难性的高光谱,该类中任何高光谱所对应的量子协方差矩阵集合都是通过正交交映变换相关联的。我们证明,所有具有这一性质的非退化高光谱都必须属于这一类,而且这类高光谱的集合与确定高斯状态的物理相关热参数和挤压参数的非退化高光谱的集合重合。
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引用次数: 0
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Reviews in Mathematical Physics
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