首页 > 最新文献

物理最新文献

英文 中文
IF:
Theoretical Analysis on QCD Ghost Dark Energy in the DGP Braneworld DGP 边界中 QCD 幽灵暗能量的理论分析
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S020228932470052X
Sibo Zhang, Weiqiang Yang

We study the evolution of a QCD ghost dark energy model under two branches of the DGP braneworld, and this model is distinguished from the (Lambda)CDM model by diagnostic methods of Statefinder hierarchy and Om((z)). Through the derivation of the evolution equation of the energy density parameters, the deceleration parameters and the equation-of-state (EoS) parameter, it can be proved that in both noninteractive and interactive scenarios (specifically, including (Q_{1}=3Hxirho_{textrm{de}},Q_{2}=3Hxirho_{textrm{dm}},Q_{3}=3Hxi(rho_{textrm{de}}+rho_{textrm{dm}}))), this model can well describe the evolution rule of today’s universe. In the later stage of the evolution of the universe, the main component of the universe changed from dark matter to dark energy, and the universe gradually transitioned from decelerating expansion to accelerating expansion, and it will not end up with a big rip in the future. And in the self-accelerating branch of the DGP braneworld, the accelerated expansion of the universe occurred earlier. In order to distinguish the QCD model from the (Lambda)CDM model, we adopted two diagnostic methods, namely, the Statefinder diagnostic and the Om diagnostic. From their respective diagnostic images, it can be seen that these two diagnostic methods cannot only effectively distinguish the QCD model from (Lambda)CDM, but also directly reflect that the coupling parameters (xi) have a certain impact on the dark energy model. It can also eliminate the degeneracy of different coupling parameters under the same interaction.

{"title":"Theoretical Analysis on QCD Ghost Dark Energy in the DGP Braneworld","authors":"Sibo Zhang,&nbsp;Weiqiang Yang","doi":"10.1134/S020228932470052X","DOIUrl":"10.1134/S020228932470052X","url":null,"abstract":"<p>We study the evolution of a QCD ghost dark energy model under two branches of the DGP braneworld, and this model is distinguished from the <span>(Lambda)</span>CDM model by diagnostic methods of Statefinder hierarchy and Om(<span>(z)</span>). Through the derivation of the evolution equation of the energy density parameters, the deceleration parameters and the equation-of-state (EoS) parameter, it can be proved that in both noninteractive and interactive scenarios (specifically, including <span>(Q_{1}=3Hxirho_{textrm{de}},Q_{2}=3Hxirho_{textrm{dm}},Q_{3}=3Hxi(rho_{textrm{de}}+rho_{textrm{dm}}))</span>), this model can well describe the evolution rule of today’s universe. In the later stage of the evolution of the universe, the main component of the universe changed from dark matter to dark energy, and the universe gradually transitioned from decelerating expansion to accelerating expansion, and it will not end up with a big rip in the future. And in the self-accelerating branch of the DGP braneworld, the accelerated expansion of the universe occurred earlier. In order to distinguish the QCD model from the <span>(Lambda)</span>CDM model, we adopted two diagnostic methods, namely, the Statefinder diagnostic and the Om diagnostic. From their respective diagnostic images, it can be seen that these two diagnostic methods cannot only effectively distinguish the QCD model from <span>(Lambda)</span>CDM, but also directly reflect that the coupling parameters <span>(xi)</span> have a certain impact on the dark energy model. It can also eliminate the degeneracy of different coupling parameters under the same interaction.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"82 - 98"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529927","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
A Theory of Gravity in Minkowski Space 闵科夫斯基空间引力理论
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S0202289324700506
Naman Kumar

We propose a theory of gravity in Minkowski space. The basic idea is that the presence of mass affects the world line of particles in flat Minkowski background. Although General Relativity is in complete agreement with observations so far, the theory discussed in this paper can solve some of the conceptual difficulties of GR, such as the energy problem, that is at the core of constructing this theory. We also discuss the cosmic expansion of the present universe and comment on the early universe. Furthermore, we demonstrate how the flatness problem and horizon problem are solved within this framework. As it will become clear, this is a theory of principle and not a theory of construction.

我们提出了一种闵科夫斯基空间引力理论。其基本思想是,质量的存在会影响平面闵科夫斯基背景中粒子的世界线。虽然广义相对论与迄今为止的观测结果完全一致,但本文讨论的理论可以解决广义相对论在概念上的一些难题,如能量问题,而这正是构建这一理论的核心所在。我们还讨论了当前宇宙的宇宙膨胀,并对早期宇宙进行了评论。此外,我们还演示了如何在这一框架内解决平面问题和视界问题。我们将清楚地看到,这是一个原理理论,而不是一个构造理论。
{"title":"A Theory of Gravity in Minkowski Space","authors":"Naman Kumar","doi":"10.1134/S0202289324700506","DOIUrl":"10.1134/S0202289324700506","url":null,"abstract":"<p>We propose a theory of gravity in Minkowski space. The basic idea is that the presence of mass affects the world line of particles in flat Minkowski background. Although General Relativity is in complete agreement with observations so far, the theory discussed in this paper can solve some of the conceptual difficulties of GR, such as the energy problem, that is at the core of constructing this theory. We also discuss the cosmic expansion of the present universe and comment on the early universe. Furthermore, we demonstrate how the flatness problem and horizon problem are solved within this framework. As it will become clear, this is a theory of principle and not a theory of construction.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"64 - 70"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529928","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
Projective Collineation in Space-Times of Pseudo-Symmetric Type
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S0202289324700452
Uday Chand De, Krishnendu De

This article deals with an investigation of projective collineations in pseudo-symmetric type space-times. First we deduce that if a pseudo-Ricci symmetric space-time admits a projective collineation whose associated vector field is a special projective vector field, then the space-time represents a stiff matter fluid. Also, we establish that if a pseudo-projective symmetric space-time admits a projective collineation whose associated vector field is a projective vector field, then the space-time becomes an Einstein space-time. Finally, we illustrate that if a pseudo-projective symmetric space-time admits a non-affine projective vector field, then the space-time becomes a perfect fluid space-time.

{"title":"Projective Collineation in Space-Times of Pseudo-Symmetric Type","authors":"Uday Chand De,&nbsp;Krishnendu De","doi":"10.1134/S0202289324700452","DOIUrl":"10.1134/S0202289324700452","url":null,"abstract":"<p>This article deals with an investigation of projective collineations in pseudo-symmetric type space-times. First we deduce that if a pseudo-Ricci symmetric space-time admits a projective collineation whose associated vector field is a special projective vector field, then the space-time represents a stiff matter fluid. Also, we establish that if a pseudo-projective symmetric space-time admits a projective collineation whose associated vector field is a projective vector field, then the space-time becomes an Einstein space-time. Finally, we illustrate that if a pseudo-projective symmetric space-time admits a non-affine projective vector field, then the space-time becomes a perfect fluid space-time.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"22 - 27"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143530029","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
SH wave in two-layered structure of functionally graded viscoelastic and monoclinic media under the influence of an interior point source 内部点源影响下功能分级粘弹性和单斜介质两层结构中的 SH 波
IF 2.8 3区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-02 DOI: 10.1140/epjp/s13360-025-06086-6
Nirakara Pradhan, Santanu Manna, Sapan Kumar Samal, Shalini Saha

This paper investigates the propagation characteristics of SH-type waves originating from a point source situated at the interface of a unique structure comprising a functionally graded viscoelastic (FGV) layer of finite depth overlying a functionally graded monoclinic (FGM) half-space. The upper viscoelastic layer exhibits a hyperbolic gradient property in its material constants, while an exponential gradient property characterizes the lower monoclinic half-space. Employing the Fourier transform and Green’s function method to account for surface and interfacial boundary conditions, a dispersion relation for the SH-type waves is derived. The obtained dispersion relation for the gradient layered structures reveals a complex interplay between wave phenomena and material properties. Numerical analysis is performed to illustrate the theoretical results for various gradient parameter values, demonstrating a significant influence on dispersion curves, phase velocity, group velocity, and wave number. This understanding holds paramount importance for seismic imaging, geological resource exploration, and the design of resilient infrastructure, thereby fostering innovation in geophysics and engineering.

{"title":"SH wave in two-layered structure of functionally graded viscoelastic and monoclinic media under the influence of an interior point source","authors":"Nirakara Pradhan,&nbsp;Santanu Manna,&nbsp;Sapan Kumar Samal,&nbsp;Shalini Saha","doi":"10.1140/epjp/s13360-025-06086-6","DOIUrl":"10.1140/epjp/s13360-025-06086-6","url":null,"abstract":"<div><p>This paper investigates the propagation characteristics of SH-type waves originating from a point source situated at the interface of a unique structure comprising a functionally graded viscoelastic (FGV) layer of finite depth overlying a functionally graded monoclinic (FGM) half-space. The upper viscoelastic layer exhibits a hyperbolic gradient property in its material constants, while an exponential gradient property characterizes the lower monoclinic half-space. Employing the Fourier transform and Green’s function method to account for surface and interfacial boundary conditions, a dispersion relation for the SH-type waves is derived. The obtained dispersion relation for the gradient layered structures reveals a complex interplay between wave phenomena and material properties. Numerical analysis is performed to illustrate the theoretical results for various gradient parameter values, demonstrating a significant influence on dispersion curves, phase velocity, group velocity, and wave number. This understanding holds paramount importance for seismic imaging, geological resource exploration, and the design of resilient infrastructure, thereby fostering innovation in geophysics and engineering.</p></div>","PeriodicalId":792,"journal":{"name":"The European Physical Journal Plus","volume":"140 3","pages":""},"PeriodicalIF":2.8,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529952","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
Existence of a Local Classical Solution to the Einstein-Scalar System in Higher Dimensions
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S0202289324700440
Mirda Prisma Wijayanto, Fiki Taufik Akbar, Bobby Eka Gunara

We study the existence of a local classical solution to the Einstein-Scalar equations in higher dimensions. We reduce the problem to a single first-order integro-differential equation. Then, we employ the contraction mapping in the appropriate Banach space. Using the Banach fixed theorem, we show that there exists a unique fixed point, which is the solution to the main problem. Finally, for given initial data, we prove the existence of a local classical solution.

我们研究了高维度爱因斯坦-斯卡拉方程的局部经典解的存在性。我们将问题简化为一个一阶积分微分方程。然后,我们在适当的巴拿赫空间中使用收缩映射。利用巴拿赫定点定理,我们证明存在一个唯一的定点,它就是主问题的解。最后,对于给定的初始数据,我们证明了局部经典解的存在。
{"title":"Existence of a Local Classical Solution to the Einstein-Scalar System in Higher Dimensions","authors":"Mirda Prisma Wijayanto,&nbsp;Fiki Taufik Akbar,&nbsp;Bobby Eka Gunara","doi":"10.1134/S0202289324700440","DOIUrl":"10.1134/S0202289324700440","url":null,"abstract":"<p>We study the existence of a local classical solution to the Einstein-Scalar equations in higher dimensions. We reduce the problem to a single first-order integro-differential equation. Then, we employ the contraction mapping in the appropriate Banach space. Using the Banach fixed theorem, we show that there exists a unique fixed point, which is the solution to the main problem. Finally, for given initial data, we prove the existence of a local classical solution.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"13 - 21"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143530028","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
Machine learning analysis of anomalous diffusion 异常扩散的机器学习分析
IF 2.8 3区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-02 DOI: 10.1140/epjp/s13360-025-06138-x
Wenjie Cai, Yi Hu, Xiang Qu, Hui Zhao, Gongyi Wang, Jing Li, Zihan Huang

The rapid advancements in machine learning have made its application to anomalous diffusion analysis both essential and inevitable. This review systematically introduces the integration of machine learning techniques for enhanced analysis of anomalous diffusion, focusing on two pivotal aspects: single trajectory characterization via machine learning and representation learning of anomalous diffusion. We extensively compare various machine learning methods, including both classical machine learning and deep learning, used for the inference of diffusion parameters and trajectory segmentation. Additionally, platforms such as the anomalous diffusion challenge that serve as benchmarks for evaluating these methods are highlighted. On the other hand, we outline three primary strategies for representing anomalous diffusion: the combination of predefined features, the feature vector from the penultimate layer of neural network, and the latent representation from the autoencoder, analyzing their applicability across various scenarios. This investigation paves the way for future research, offering valuable perspectives that can further enrich the study of anomalous diffusion and advance the application of artificial intelligence in statistical physics and biophysics.

机器学习的飞速发展使其在异常扩散分析中的应用变得必不可少。这篇综述系统地介绍了如何整合机器学习技术来增强异常扩散分析,重点关注两个关键方面:通过机器学习进行单一轨迹表征和异常扩散的表征学习。我们广泛比较了用于扩散参数推断和轨迹分割的各种机器学习方法,包括经典机器学习和深度学习。此外,我们还重点介绍了作为评估这些方法基准的异常扩散挑战等平台。另一方面,我们概述了表示异常扩散的三种主要策略:预定义特征的组合、来自神经网络倒数第二层的特征向量以及来自自动编码器的潜在表示,并分析了它们在各种场景中的适用性。这项研究为今后的研究铺平了道路,提供了宝贵的视角,可以进一步丰富异常扩散的研究,推动人工智能在统计物理和生物物理学中的应用。
{"title":"Machine learning analysis of anomalous diffusion","authors":"Wenjie Cai,&nbsp;Yi Hu,&nbsp;Xiang Qu,&nbsp;Hui Zhao,&nbsp;Gongyi Wang,&nbsp;Jing Li,&nbsp;Zihan Huang","doi":"10.1140/epjp/s13360-025-06138-x","DOIUrl":"10.1140/epjp/s13360-025-06138-x","url":null,"abstract":"<div><p>The rapid advancements in machine learning have made its application to anomalous diffusion analysis both essential and inevitable. This review systematically introduces the integration of machine learning techniques for enhanced analysis of anomalous diffusion, focusing on two pivotal aspects: single trajectory characterization via machine learning and representation learning of anomalous diffusion. We extensively compare various machine learning methods, including both classical machine learning and deep learning, used for the inference of diffusion parameters and trajectory segmentation. Additionally, platforms such as the anomalous diffusion challenge that serve as benchmarks for evaluating these methods are highlighted. On the other hand, we outline three primary strategies for representing anomalous diffusion: the combination of predefined features, the feature vector from the penultimate layer of neural network, and the latent representation from the autoencoder, analyzing their applicability across various scenarios. This investigation paves the way for future research, offering valuable perspectives that can further enrich the study of anomalous diffusion and advance the application of artificial intelligence in statistical physics and biophysics.</p></div>","PeriodicalId":792,"journal":{"name":"The European Physical Journal Plus","volume":"140 3","pages":""},"PeriodicalIF":2.8,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529951","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
Observational Study of the Deceleration Parameter in (boldsymbol{f(R,L_{m})}) Theory of Gravity (boldsymbol{f(R,L_{m})}) 中减速参数的观测研究引力理论
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S0202289324700518
Bhupendra Kumar Shukla, D. Sofuoğlu, A. Beesham, Ala Ouguergouz, Shashi Narayan Shukla

We investigate the implications of the modified gravity theory (f(R,L_{m})) on the cosmological evolution. By examining the nonlinear model (f(R,L_{m})={R}/{2}+(alpha R+1)L_{m}), we explore the impact of a nonminimal coupling between curvature and matter on the cosmic expansion. Using a parametrized deceleration parameter dependent on the redshift (z), we analyze the Friedmann–Lemaître–Robertson–Walker (FLRW) universe in the (f(R,L_{m})) framework. Through observational constraints derived from Cosmic Chronometers (CC), Type Ia Supernovae (SNIa), and Baryon Acoustic Oscillations (BAO), we perform a detailed comparison with the standard (Lambda)CDM model. Our results show that the (f(R,L_{m})) model is consistent with observational data, but deviations from the (Lambda)CDM model emerge in its geometric structure, highlighting the potential of (f(R,L_{m})) gravity in explaining the dark energy and cosmic acceleration.

我们研究了修正引力理论(f(R,L_{m}))对宇宙学演化的影响。通过研究非线性模型(f(R,L_{m})={R}/{2}+(alpha R+1)L_{m}),我们探索了曲率与物质之间的非最小耦合对宇宙膨胀的影响。利用一个依赖于红移((z))的参数化减速参数,我们在(f(R,L_{m}))框架内分析了弗里德曼-勒梅特-罗伯逊-沃克(FLRW)宇宙。通过从宇宙计时器(CC)、Ia型超新星(SNIa)和重子声学振荡(BAO)得到的观测约束,我们与标准的CDM模型进行了详细的比较。我们的结果表明,(f(R,L_{m}))模型与观测数据是一致的,但是在其几何结构上出现了与(Lambda)CDM模型的偏差,突出了(f(R,L_{m}))引力在解释暗能量和宇宙加速度方面的潜力。
{"title":"Observational Study of the Deceleration Parameter in (boldsymbol{f(R,L_{m})}) Theory of Gravity","authors":"Bhupendra Kumar Shukla,&nbsp;D. Sofuoğlu,&nbsp;A. Beesham,&nbsp;Ala Ouguergouz,&nbsp;Shashi Narayan Shukla","doi":"10.1134/S0202289324700518","DOIUrl":"10.1134/S0202289324700518","url":null,"abstract":"<p>We investigate the implications of the modified gravity theory <span>(f(R,L_{m}))</span> on the cosmological evolution. By examining the nonlinear model <span>(f(R,L_{m})={R}/{2}+(alpha R+1)L_{m})</span>, we explore the impact of a nonminimal coupling between curvature and matter on the cosmic expansion. Using a parametrized deceleration parameter dependent on the redshift <span>(z)</span>, we analyze the Friedmann–Lemaître–Robertson–Walker (FLRW) universe in the <span>(f(R,L_{m}))</span> framework. Through observational constraints derived from Cosmic Chronometers (CC), Type Ia Supernovae (SNIa), and Baryon Acoustic Oscillations (BAO), we perform a detailed comparison with the standard <span>(Lambda)</span>CDM model. Our results show that the <span>(f(R,L_{m}))</span> model is consistent with observational data, but deviations from the <span>(Lambda)</span>CDM model emerge in its geometric structure, highlighting the potential of <span>(f(R,L_{m}))</span> gravity in explaining the dark energy and cosmic acceleration.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"71 - 81"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529931","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
Cosmological Models Based on an Asymmetric Scalar Higgs Doublet with Potential Interactions between Components 基于非对称标量希格斯双星与各成分间潜在相互作用的宇宙学模型
IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-03-02 DOI: 10.1134/S0202289324700439
Yu. G. Ignat’ev, A. R. Samigullina

Cosmological models based on an asymmetric scalar Higgs doublet (the canonical (Phi) and phantom (phi) fields) with potential interaction between the components are proposed. A qualitative analysis of the corresponding dynamic systems is performed, and their transformation properties with respect to similarity transformations of fundamental constants are revealed. The asymptotic behavior of this class of cosmological models near cosmological singularities is investigated. Numerical simulations reveal a number of interesting features of these models, in particular, the possibility of a fairly long “waiting phase,” during which the Universe is almost Euclidean, as well as the presence of bounce points, near which there occur strong oscillations of the scalar potentials.

{"title":"Cosmological Models Based on an Asymmetric Scalar Higgs Doublet with Potential Interactions between Components","authors":"Yu. G. Ignat’ev,&nbsp;A. R. Samigullina","doi":"10.1134/S0202289324700439","DOIUrl":"10.1134/S0202289324700439","url":null,"abstract":"<p>Cosmological models based on an asymmetric scalar Higgs doublet (the canonical <span>(Phi)</span> and phantom <span>(phi)</span> fields) with potential interaction between the components are proposed. A qualitative analysis of the corresponding dynamic systems is performed, and their transformation properties with respect to similarity transformations of fundamental constants are revealed. The asymptotic behavior of this class of cosmological models near cosmological singularities is investigated. Numerical simulations reveal a number of interesting features of these models, in particular, the possibility of a fairly long “waiting phase,” during which the Universe is almost Euclidean, as well as the presence of bounce points, near which there occur strong oscillations of the scalar potentials.</p>","PeriodicalId":583,"journal":{"name":"Gravitation and Cosmology","volume":"31 1","pages":"1 - 12"},"PeriodicalIF":1.2,"publicationDate":"2025-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143529932","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"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
Evaluation of kinetic freeze-out properties in different relativistic heavy-ion collision systems at (sqrt{s_{NN}}=200) GeV 在 (sqrt{s_{NN}}=200) GeV 下评估不同相对论重离子碰撞系统的动力学冻结特性
IF 2.8 3区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-03-01 DOI: 10.1140/epjp/s13360-025-06119-0
Muhammad Waqas, Muhammad Ajaz, Jihane Ben Slimane, Murad Badshah, Haifa I. Alrebdi, Abd Al Karim Haj Ismail

We present our analysis of the identified hadrons ((pi ^+), (K^+), and p) kinetic freeze-out properties in relativistic collisions at (sqrt{s_{NN}} = 200) GeV. We analyze the transverse momentum spectra of these hadrons across various collision systems, such as copper–copper ((Cu-Cu)), zirconium–zirconium ((Zr-Zr)), ruthenium–ruthenium ((Ru-Ru)), uranium–uranium ((U-U)), and gold–gold ((Au-Au)) collisions, in distinct centrality intervals at the same center-of-mass energy using the modified Hagedorn model with embedded flow. The freeze-out parameters, namely the kinetic freeze-out temperature ((T_0)), transverse flow velocity ((beta _T)), and the entropy-related parameter (n), are extracted. Taking (T_0) and (beta _T) as common, it is observed that in all the above collisions, (T_0), (beta _T), and the parameter n diminish toward the periphery and are greater in central collisions. However, (T_0) in central collisions across all the systems remains unchanged, indicating a phase transition from hadronic matter to quark–gluon plasma. Furthermore, the temperature required for the phase transition across various systems is different. Large systems exhibit a shift in the potential start of the phase transition in peripheral collisions, which is intriguing. We also observe a direct relation between the extracted parameters and the system’s size.

{"title":"Evaluation of kinetic freeze-out properties in different relativistic heavy-ion collision systems at (sqrt{s_{NN}}=200) GeV","authors":"Muhammad Waqas,&nbsp;Muhammad Ajaz,&nbsp;Jihane Ben Slimane,&nbsp;Murad Badshah,&nbsp;Haifa I. Alrebdi,&nbsp;Abd Al Karim Haj Ismail","doi":"10.1140/epjp/s13360-025-06119-0","DOIUrl":"10.1140/epjp/s13360-025-06119-0","url":null,"abstract":"<div><p>We present our analysis of the identified hadrons (<span>(pi ^+)</span>, <span>(K^+)</span>, and <i>p</i>) kinetic freeze-out properties in relativistic collisions at <span>(sqrt{s_{NN}} = 200)</span> GeV. We analyze the transverse momentum spectra of these hadrons across various collision systems, such as copper–copper (<span>(Cu-Cu)</span>), zirconium–zirconium (<span>(Zr-Zr)</span>), ruthenium–ruthenium (<span>(Ru-Ru)</span>), uranium–uranium (<span>(U-U)</span>), and gold–gold (<span>(Au-Au)</span>) collisions, in distinct centrality intervals at the same center-of-mass energy using the modified Hagedorn model with embedded flow. The freeze-out parameters, namely the kinetic freeze-out temperature (<span>(T_0)</span>), transverse flow velocity (<span>(beta _T)</span>), and the entropy-related parameter (<i>n</i>), are extracted. Taking <span>(T_0)</span> and <span>(beta _T)</span> as common, it is observed that in all the above collisions, <span>(T_0)</span>, <span>(beta _T)</span>, and the parameter <i>n</i> diminish toward the periphery and are greater in central collisions. However, <span>(T_0)</span> in central collisions across all the systems remains unchanged, indicating a phase transition from hadronic matter to quark–gluon plasma. Furthermore, the temperature required for the phase transition across various systems is different. Large systems exhibit a shift in the potential start of the phase transition in peripheral collisions, which is intriguing. We also observe a direct relation between the extracted parameters and the system’s size.</p></div>","PeriodicalId":792,"journal":{"name":"The European Physical Journal Plus","volume":"140 2","pages":""},"PeriodicalIF":2.8,"publicationDate":"2025-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143527629","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
Large fluctuations in NSPT computations: a lesson from O(N) non-linear sigma models NSPT 计算中的大波动:O(N) 非线性西格玛模型的启示
IF 4.2 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS Pub Date : 2025-03-01 DOI: 10.1140/epjc/s10052-025-13887-7
Paolo Baglioni, Francesco Di Renzo

In the last three decades, numerical stochastic perturbation theory (NSPT) has proven to be an excellent tool for calculating perturbative expansions in theories such as Lattice QCD, for which standard, diagrammatic perturbation theory is known to be cumbersome. Despite the significant success of this stochastic method and the improvements made in recent years, NSPT apparently cannot be successfully implemented in low-dimensional models due to the emergence of huge statistical fluctuations: as the perturbative order gets higher, the signal to noise ratio is simply not good enough. This does not come as a surprise, but on very general grounds, one would expect that the larger the number of degrees of freedom, the less severe the fluctuations will be. By simulating 2D O(N) non-linear sigma models for different values of N, we show that indeed the fluctuations are tamed in the large N limit, meeting our expectations: for a large number of internal degrees of freedom (i.e. for large enough N), NSPT perturbative computation can be pushed to large perturbative orders n. By re-expressing our perturbative expansions as power series in the gN (’t Hooft) coupling, we show some evidence that at any given order n there is a tendency to gaussianity for the stochastic process distributions at large N. By summing our series, we can verify leading order results for the energy and its (field theoretic) variance in the large N limit. We finally establish general relationships between the various perturbative orders in the expansion of the (field theoretic) variance of a given observable and combinations of variances and covariances of given orders NSPT stochastic processes. Having established all this, we conclude discussing interesting applications of NSPT computations in the context of theories similar to O(N) (i.e. (CP(N-1)) models).

{"title":"Large fluctuations in NSPT computations: a lesson from O(N) non-linear sigma models","authors":"Paolo Baglioni,&nbsp;Francesco Di Renzo","doi":"10.1140/epjc/s10052-025-13887-7","DOIUrl":"10.1140/epjc/s10052-025-13887-7","url":null,"abstract":"<div><p>In the last three decades, numerical stochastic perturbation theory (NSPT) has proven to be an excellent tool for calculating perturbative expansions in theories such as Lattice QCD, for which standard, diagrammatic perturbation theory is known to be cumbersome. Despite the significant success of this stochastic method and the improvements made in recent years, NSPT apparently cannot be successfully implemented in low-dimensional models due to the emergence of huge statistical fluctuations: as the perturbative order gets higher, the signal to noise ratio is simply not good enough. This does not come as a surprise, but on very general grounds, one would expect that the larger the number of degrees of freedom, the less severe the fluctuations will be. By simulating 2<i>D</i> <i>O</i>(<i>N</i>) non-linear sigma models for different values of <i>N</i>, we show that indeed the fluctuations are tamed in the large <i>N</i> limit, meeting our expectations: for a large number of <i>internal</i> degrees of freedom (i.e. for large enough <i>N</i>), NSPT perturbative computation can be pushed to large perturbative orders <i>n</i>. By re-expressing our perturbative expansions as power series in the <i>gN</i> (’t Hooft) coupling, we show some evidence that at any given order <i>n</i> there is a tendency to gaussianity for the stochastic process distributions at large <i>N</i>. By summing our series, we can verify leading order results for the energy and its (field theoretic) variance in the large <i>N</i> limit. We finally establish general relationships between the various perturbative orders in the expansion of the (field theoretic) variance of a given observable and combinations of variances and covariances of given orders NSPT stochastic processes. Having established all this, we conclude discussing interesting applications of NSPT computations in the context of theories similar to <i>O</i>(<i>N</i>) (i.e. <span>(CP(N-1))</span> models).</p></div>","PeriodicalId":788,"journal":{"name":"The European Physical Journal C","volume":"85 2","pages":""},"PeriodicalIF":4.2,"publicationDate":"2025-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-13887-7.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143527662","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1