Annals of Physics最新文献

Shadows for Kerr–Sen–Taub–NUT black holes with Manko–Ruiz parameter

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-04-07 DOI: 10.1016/j.aop.2025.170015

Haryanto M. Siahaan

引用次数: 0

Shot-noise power from a topological superconductor with chiral symmetry

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-04-04 DOI: 10.1016/j.aop.2025.170013

Marília S.M. Barros, Isacc A. Saturno Junior, Edson M. Alves, Edivan A. da Silva, Ailton F. Macedo Junior, Antonio R. de C. Romaguera, Anderson L.R. Barbosa

引用次数: 0

Cosmic acceleration driven by dark matter self-interactions: A phenomenological treatment

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-04-04 DOI: 10.1016/j.aop.2025.170012

A. Kazım Çamlıbel

引用次数: 0

Landau levels for a non-relativistic spin 1/2 particle in a cosmic string spacetime

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-28 DOI: 10.1016/j.aop.2025.170011

M.D. de Oliveira, Alexandre G.M. Schmidt

引用次数: 0

Reflections of topological properties in the planar-Hall response for semimetals carrying pseudospin-1 quantum numbers 携带伪ospin-1 量子数的半金属在平面-霍尔响应中的拓扑特性反映

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-28 DOI: 10.1016/j.aop.2025.170010

Firdous Haidar, Ipsita Mandal

{"title":"Reflections of topological properties in the planar-Hall response for semimetals carrying pseudospin-1 quantum numbers","authors":"Firdous Haidar, Ipsita Mandal","doi":"10.1016/j.aop.2025.170010","DOIUrl":"10.1016/j.aop.2025.170010","url":null,"abstract":"<div><div>We continue our investigations of the nature of the linear-response tensors in planar-Hall and planar-thermal Hall configurations, involving three-dimensional nodal-point semimetals, by considering here nodes hosting pseudospin-1 quasiparticles. Such systems exemplify multifold semimetals, as they have three bands crossing at a nodal point. We derive the explicit expressions of the electric, thermoelectric, and thermal coefficients, when the nodes are subjected to the combined influence of an electric field (and/or temperature gradient) and a weak (i.e., nonquantizing) magnetic field. In order to have a complete description, we consider the effects of the Berry curvature and the orbital magnetic moment on an equal footing, both of which originate from the underlying topological features of the bandstructure. Going beyond our previous works, we determine the out-of-plane response comprising the intrinsic anomalous-Hall and the Lorentz-force-contributed currents, and chalk out the effects of internode scatterings as well. Our theoretical explorations shed light on the mechanisms of transport in multifold semimetals, which are being investigated in contemporary experiments.</div></div>","PeriodicalId":8249,"journal":{"name":"Annals of Physics","volume":"478 ","pages":"Article 170010"},"PeriodicalIF":3.0,"publicationDate":"2025-03-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143759236","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

Spontaneous emission in a coupled cavity array featuring random-dimer disorder

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-25 DOI: 10.1016/j.aop.2025.170009

Mariana O. Monteiro, Guilherme M.A. Almeida, Francisco A.B.F. de Moura

引用次数: 0

Vacuum state perturbed by an oscillon: Composite configurations in ϕ4 model

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-24 DOI: 10.1016/j.aop.2025.170008

Fabiano C. Simas , Eduardo da Hora

引用次数: 0

Impact of extended gravity theories on accretion dynamics and observables in black hole

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-22 DOI: 10.1016/j.aop.2025.170006

Shahid Chaudhary , Shahi Rome , Muhammad Danish Sultan , Ahmadjon Abdujabbarov , Awatef Abidi , Yousef Mohammad Alanazi , Abdulrahman Bin Jumah

{"title":"Impact of extended gravity theories on accretion dynamics and observables in black hole","authors":"Shahid Chaudhary , Shahi Rome , Muhammad Danish Sultan , Ahmadjon Abdujabbarov , Awatef Abidi , Yousef Mohammad Alanazi , Abdulrahman Bin Jumah","doi":"10.1016/j.aop.2025.170006","DOIUrl":"10.1016/j.aop.2025.170006","url":null,"abstract":"<div><div>We examine a thin accretion disk surrounding a static, spherically symmetric black hole within the framework of Einstein–Gauss–Bonnet massive gravity theory. Our focus is on the motion of particles in circular orbits around the black hole in this spacetime. Specifically, we study the geodesic motion of particles confined to the equatorial plane, which contributes to the formation of the thin accretion disk, to explore their innermost stable circular orbits and energy flux distribution. To provide a comprehensive analysis of our study, we present density plots of the effective potential, specific energy, angular momentum, angular velocity, and radiation flux. The contour plots reveal that the massive gravity and Gauss–Bonnet parameters significantly influence the gravitational pull and energy dissipation within the accretion disk. These effects have important implications for the observational properties of black holes in extended gravity theories, impacting the disk’s brightness and thermal spectrum. Utilizing the well-established Novikov–Thorne model for accretion, we investigate the impact of Gauss–Bonnet and massive gravity parameters on the direct and secondary images of the black hole’s accretion disk at various observation angles. Notably, we observe significant deviations from standard black hole solutions, such as Schwarzschild or Reissner–Nordstrm.</div></div>","PeriodicalId":8249,"journal":{"name":"Annals of Physics","volume":"477 ","pages":"Article 170006"},"PeriodicalIF":3.0,"publicationDate":"2025-03-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143685067","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

Scaling of Fock space propagator in quasiperiodic many-body localizing systems

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-22 DOI: 10.1016/j.aop.2025.170001

Soumi Ghosh , Jagannath Sutradhar , Subroto Mukerjee , Sumilan Banerjee

{"title":"Scaling of Fock space propagator in quasiperiodic many-body localizing systems","authors":"Soumi Ghosh , Jagannath Sutradhar , Subroto Mukerjee , Sumilan Banerjee","doi":"10.1016/j.aop.2025.170001","DOIUrl":"10.1016/j.aop.2025.170001","url":null,"abstract":"<div><div>Recently many-body localized systems have been treated as a hopping problem on a Fock space lattice with correlated disorder, where the many-body eigenstates exhibit multi-fractal character. The many-body propagator in Fock space has been shown to be useful for capturing this multifractality and extracting a Fock-space localization length for systems with random disorder in real space. Here we study a one-dimensional interacting system of spinless Fermions in the presence of a deterministic quasiperiodic potential using the Fock-space propagator. From the system-size scaling of the self-energy associated with the diagonal elements and the scaling of the off-diagonal elements of the propagator, we extract fractal characteristics and FS localization lengths, respectively, which behave similarly to that in the random system. We compute the sample-to-sample fluctuations of the typical self-energy and the off-diagonal propagator over different realizations of the potential and show that the fluctuations in the self-energy distinguish quasiperiodic and random systems, whereas the fluctuations of the off-diagonal elements cannot demarcate the two types of potential. In particular, for the random system, the sample-to-sample fluctuations of the self-energy exhibits a distinct transition or sharp crossover within the thermal phase in the form of a peak whose height increases with system size. Such a feature is completely absent in the quasiperiodic system.</div></div>","PeriodicalId":8249,"journal":{"name":"Annals of Physics","volume":"478 ","pages":"Article 170001"},"PeriodicalIF":3.0,"publicationDate":"2025-03-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143704920","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

More on analytically approximate solution to quadratic gravity

IF 3 3区物理与天体物理

Annals of Physics Pub Date : 2025-03-22 DOI: 10.1016/j.aop.2025.170007

Seyed Naseh Sajadi, Supakchai Ponglertsakul

引用次数: 0