Annales Henri Poincaré最新文献_第10页

Inverse Source Problem for the Boltzmann Equation in Cosmology 宇宙学中玻尔兹曼方程的逆源问题

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-02-08 DOI: 10.1007/s00023-025-01543-5

Yiran Wang

引用次数: 0

Classifying Bulk-Edge Anomalies in the Dirac Hamiltonian 狄拉克哈密顿量中块边异常的分类

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-02-03 DOI: 10.1007/s00023-025-01541-7

Hansueli Jud, Clément Tauber

引用次数: 0

Unitarity and Strong Graded Locality of Holomorphic Vertex Operator Superalgebras with Central Charge at Most 24 中心电荷最多为24的全纯顶点算子超代数的统一性和强梯度局部性

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-30 DOI: 10.1007/s00023-025-01542-6

Tiziano Gaudio

引用次数: 0

From Quantum Curves to Topological String Partition Functions II 从量子曲线到拓扑弦配分函数2

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-29 DOI: 10.1007/s00023-025-01538-2

Ioana Coman, Pietro Longhi, Jörg Teschner

引用次数: 0

Secular Growths and Their Relation to Equilibrium States in Perturbative QFT 摄动QFT中长期增长及其与平衡态的关系

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-22 DOI: 10.1007/s00023-024-01526-y

Stefano Galanda, Nicola Pinamonti, Leonardo Sangaletti

{"title":"Secular Growths and Their Relation to Equilibrium States in Perturbative QFT","authors":"Stefano Galanda, Nicola Pinamonti, Leonardo Sangaletti","doi":"10.1007/s00023-024-01526-y","DOIUrl":"10.1007/s00023-024-01526-y","url":null,"abstract":"<div><p>In the perturbative treatment of interacting quantum field theories, if the interaction Lagrangian changes adiabatically in a finite interval of time, secular growths may appear in the truncated perturbative series also when the interaction Lagrangian density is returned to be constant. If this happens, the perturbative approach does not furnish reliable results in the evaluation of scattering amplitudes or expectation values. In this paper we show that these effects can be avoided for adiabatically switched-on interactions, if the spatial support of the interaction is compact and if the background state is suitably chosen. We start considering equilibrium background states and show that, when thermalisation occurs (interaction Lagrangian of spatial compact support), secular effects are avoided. Furthermore, no secular effects pop up if the limit where the Lagrangian is supported everywhere in space is taken after thermalisation (large time limit), in contrast to the reversed order. This result is generalized showing that if the interaction Lagrangian is spatially compact, secular growths are avoided for generic background states which are only invariant under time translation and to states whose explicit dependence of time is not too strong. Finally, as an application, the presented theorems are used to study a complex scalar and a Dirac field, on a background KMS state, in a classical external electromagnetic potential and the contribution to the two point-function given by a generic loop diagram arising from a second order perturbative expansion.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"26 11","pages":"4141 - 4203"},"PeriodicalIF":1.3,"publicationDate":"2025-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-024-01526-y.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145248331","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Wick Rotation of Linearized Gravity in Gaussian Time and Calderón Projectors 高斯时间和Calderón投影仪中线性化重力的灯芯旋转

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-20 DOI: 10.1007/s00023-025-01539-1

Christian Gérard, Simone Murro, Michał Wrochna

引用次数: 0

Decoherence is an Echo of Anderson Localization in Open Quantum Systems 退相干是开放量子系统中安德森局域化的一种回波

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-18 DOI: 10.1007/s00023-024-01528-w

Frederik Ravn Klausen, Simone Warzel

引用次数: 0

On the Existence of Charged Electrostatic Black Holes in Arbitrary Topology 关于任意拓扑中带电静电黑洞的存在性

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-16 DOI: 10.1007/s00023-024-01534-y

Martín Reiris

{"title":"On the Existence of Charged Electrostatic Black Holes in Arbitrary Topology","authors":"Martín Reiris","doi":"10.1007/s00023-024-01534-y","DOIUrl":"10.1007/s00023-024-01534-y","url":null,"abstract":"<div><p>The general classification of <span>(3+1)</span>-static black hole solutions of the Einstein equations, with or without matter, is central in general relativity and important in geometry. In the realm of <span>(textrm{S}^{1})</span>-symmetric <i>vacuum</i> spacetimes, a recent classification proved that, without restrictions on the topology or the asymptotic behavior, black hole solutions can be only of three kinds: (i) Schwarzschild black holes, (ii) Boost black holes or (iii) Myers–Korotkin–Nicolai black holes, each one having its distinct asymptotic and topological type. In contrast to this, very little is known about the general classification of <span>(textrm{S}^{1})</span>-symmetric static <i>electrovacuum</i> black holes although examples show that, on the large picture, there should be striking differences with respect to the vacuum case. A basic question then is whether or not there are charged analogs to the static vacuum black holes of types (i), (ii) and (iii). In this article, we prove the remarkable fact that, while one can ‘charge’ the Schwarzschild solution (resulting in a Reissner–Nordström spacetime) preserving the asymptotic, one cannot do the same to the Boosts and to the Myers–Korotkin–Nicolai solutions: The addition of a small or large electric charge, if possible at all, would transform entirely their asymptotic behavior. In particular, such vacuum solutions cannot be electromagnetically perturbed. The results of this paper are consistent but go far beyond the works of Karlovini and Von Unge on periodic analogs of the Reissner–Nordström black holes. The type of result as well as the techniques used is based on comparison geometry a la Bakry–Émery and appears to be entirely novel in this context. The findings point to a complex interplay between asymptotic, topology and charge in spacetime dimension <span>(3+1)</span>, markedly different from what occurs in higher dimensions.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"26 11","pages":"4051 - 4069"},"PeriodicalIF":1.3,"publicationDate":"2025-01-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145248325","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

Asymptotic Decay for Defocusing Semilinear Wave Equations on Schwarzschild Spacetimes 史瓦西时空上离焦半线性波动方程的渐近衰减

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-15 DOI: 10.1007/s00023-025-01537-3

He Mei, Dongyi Wei, Shiwu Yang

引用次数: 0

Effective Polaron Dynamics of an Impurity Particle Interacting with a Fermi Gas 杂质粒子与费米气体相互作用的有效极化子动力学

IF 1.3 3区物理与天体物理

Annales Henri Poincaré Pub Date : 2025-01-13 DOI: 10.1007/s00023-024-01532-0

Duc Viet Hoang, Peter Pickl

引用次数: 0