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Solitary wave solution, traveling wave solution and other solutions of variable-coefficients Chiral Schrodinger equation 变系数手性薛定谔方程的孤波解、行波解及其他解
IF 1.8 3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-12-01 DOI: 10.1142/s0219887824501007
Liu Yang, Ben Gao
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引用次数: 0
Generalized cutoff for late time acceleration and inflation: the cosmology of holographic fluid 广义时间加速和膨胀的截止:全息流体的宇宙学
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-10 DOI: 10.1142/s0219887824500841
Altaibayeva Aziza, Surajit Chattopadhyay
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引用次数: 0
Non-Hermitian two-dimensional harmonic oscillator in noncommutative phase-space 非交换相空间中的非厄米二维谐振子
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-10 DOI: 10.1142/s0219887824500853
Emanonfi Elias N'Dolo
In this paper, we extend the result of [Andreas Fring et al J. Phys. A 43, 345401 (2010)] in noncommutative phase-space (NCPS). We compute the non-Hermitian Hamiltonian of a harmonic oscillator in NCPS. We construct a new P T-symmetry in noncommutative phase-space and prove that the system does not possess a broken P T-regime. We then compute the eigenvalue spectrum of the non-Hermitian Hamiltonian of the system.
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引用次数: 0
Backlund Transformations of Multi-Component Boussinesq and Degasperis-Procesi Equations 多分量Boussinesq和Degasperis-Procesi方程的背景变换
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-09 DOI: 10.1142/s021988782450066x
Lixiang Zhang, Chuanzhong Li, Haifeng Wang
The finding of new integrable coupling systems has become an important area of research in mathematical physics and their study will aid in the classification of multi-component integrable systems. A basic method for generating integrable coupling systems is algebraic expansion, for example, the Frobenius algebra, the Lie algebra, the superalgebra, and so on. In this paper, we introduce a Frobenius Boussinesq equation based on the Frobenius algebra, and then we present a Lax pair of it. It follows that we give a Bäcklund transformation of the Frobenius Boussinesq equation. Furthermore, the lattice equation of the Frobenius Boussinesq equation is presented by using three Bäcklund transformations, and then obtain the exact solutions. Additionally, we obtain the conservation laws of the Frobenius Boussinesq equation via the Bäcklund transformation. Strongly coupled and weakly coupled systems physically represent strong and weak interactions, respectively. In this paper, we introduce a weakly coupled Degasperis–Procesi (DP) equation, and construct a Lax pair of it. In addition, the Bäcklund transformation and superposition principle are applied to investigate the weakly coupled DP equation. We also obtain the conservation laws of the weakly coupled DP equation. Then, we introduce a strongly coupled DP equation, and use the same method to study the strongly coupled DP equation. The exact solutions of these two equations are obtained. Moreover, we introduce a [Formula: see text]-DP equation. Considering the superposition principle, we obtain the solution of an associated [Formula: see text]-DP equation by using Bäcklund transformations. These new multi-component integrable systems can enrich the existing integrable models and possibly describe new nonlinear phenomena.
新的可积耦合系统的发现已成为数学物理研究的一个重要领域,它的研究将有助于多组分可积系统的分类。代数展开是生成可积耦合系统的一种基本方法,如Frobenius代数、Lie代数、超代数等。本文引入了基于Frobenius代数的Frobenius Boussinesq方程,并给出了它的Lax对。由此,我们给出了Frobenius Boussinesq方程的Bäcklund变换。在此基础上,对Frobenius Boussinesq方程进行了三次Bäcklund变换,得到了其格方程的精确解。此外,我们通过Bäcklund变换得到了Frobenius Boussinesq方程的守恒定律。强耦合和弱耦合系统在物理上分别表示强相互作用和弱相互作用。本文引入了一类弱耦合Degasperis-Procesi (DP)方程,并构造了它的Lax对。此外,应用Bäcklund变换和叠加原理对弱耦合DP方程进行了研究。我们还得到了弱耦合DP方程的守恒定律。然后,我们引入了强耦合DP方程,并用同样的方法研究了强耦合DP方程。得到了这两个方程的精确解。此外,我们还引入了一个[公式:见文本]-DP方程。根据叠加原理,利用Bäcklund变换,得到了一个相关联的[公式:见文]-DP方程的解。这些新的多分量可积系统可以丰富现有的可积模型,并可能描述新的非线性现象。
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引用次数: 0
Bianchi Type-V Space Time with Tsallis Holographic Dark Energy 比安奇v型时空与Tsallis全息暗能量
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-08 DOI: 10.1142/s0219887824500634
A. Narasimharao, D. Neelima
In this paper, using the framework of Saez–Ballester theory, Bianchi Type-V metric Tsallis holographic dark energy models with interacting and non-interacting elements have been constructed. To obtain solutions for the model, we used correlation between metric potentials and varying deceleration parameters. There is additional discussion of the models’ physical characteristics and behavior.
本文利用Saez-Ballester理论的框架,构造了具有相互作用和非相互作用元素的Bianchi - v型度量Tsallis全息暗能量模型。为了得到模型的解,我们使用了度量势和不同减速参数之间的相关性。另外还讨论了模型的物理特性和行为。
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引用次数: 0
Anisotropic Strange Quintessence Stars in Modified f(R, ϕ) Theory of Gravity 修正f(R, φ)引力理论中的各向异性奇异精星
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-07 DOI: 10.1142/s0219887824400036
Adnan Malik, Tayyaba Naz, Ayesha Tariq, Z. Yousaf, Ali H. Alkhaldi, M. Umair Shahzad
This paper investigated the anisotropic quintessence stars in the [Formula: see text] theory of gravity, where [Formula: see text] is the Ricci scalar and [Formula: see text] is the scalar potential. We investigated the field equations of the [Formula: see text] theory of gravity by using the Krori–Barua technique. We have determined that all the obtained solutions are free from central singularity and potentially stable. The observed values of mass and radius of the different strange stars Her X1, SAXJ1808.4-3658, and 4U1820-30 have been used to calculate the values of unknown constants in the Krori and Barua metric. The physical phenomena of stars, such as energy density, pressure components, anisotropy, sound speeds, equation of state parameters, energy conditions and redshift have been investigated in detail.
本文研究了[公式:见文]引力理论中的各向异性精星,其中[公式:见文]为里奇标量,[公式:见文]为标量势。我们用Krori-Barua技术研究了引力理论的场方程。我们已经确定所有得到的解都不存在中心奇点,并且具有潜在的稳定性。利用不同奇异恒星Her X1、SAXJ1808.4-3658和4U1820-30的质量和半径观测值,计算了Krori和Barua度规中的未知常数值。详细研究了恒星的能量密度、压力分量、各向异性、声速、状态参数方程、能量条件和红移等物理现象。
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引用次数: 0
Anisotropies and modified gravity theories in stellar and substellar objects 恒星和亚恒星天体的各向异性和修正引力理论
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-07 DOI: 10.1142/s0219887824300022
Shaswata Chowdhury
In several classes of modified gravity theories, extra degrees of freedom are not completely screened in the interiors of stellar and substellar objects. In such theories, the hydrostatic equilibrium condition inside these objects is altered. Moreover, the interior structures of these objects might have a small pressure anisotropy induced by several physical phenomena, including rotation and magnetic fields. All these effects, both individually and collectively, induce changes in predicted stellar observables. Such changes have an impact on different phases of the stellar life cycle, starting from its birth to its death, covering almost all the branches of the Hertzsprung-Russell diagram. The aim of this work is to systematically review the current literature on the topic. We discuss the main results and constraints obtained on a class of modified gravity theories.
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引用次数: 0
Gauge CPT: A Review and Use in Constructing New Affine Connections 测量CPT:在构建新的仿射连接中的回顾与应用
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-07 DOI: 10.1142/s0219887824300034
Kurt Koltko
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引用次数: 0
Cosmography for Various Parametrizations of Dark Energy Equation of State 暗能量状态方程各种参数化的宇宙学
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-04 DOI: 10.1142/s0219887824500518
Alok Sardar, Tanusree Roy, Ujjal Debnath
The concept of dark energy (DE) emerged as a result of confirming the accelerated expansion of the universe. Since then, numerous models have been developed to explore the origin and nature of DE. In this study, we investigate several recent cosmological models (Models 1–9) based on the parametrization of the DE equation of state. Our analysis focuses on a homogeneous, isotropic flat universe comprising DE, dark matter (DM), and radiation. We assume the separate conservation of the dark components (DE and DM) and radiation. By employing various parametrizations of [Formula: see text], we derive the corresponding Hubble function [Formula: see text]. To understand the cosmic expansion history of the universe in a model-independent manner, we employ cosmography as an approach. We express important cosmographic parameters such as deceleration, jerk, snap, and lerk parameters in terms of the Hubble rate [Formula: see text] and its derivative up to the fourth order. Additionally, we examine the statefinder parameter and [Formula: see text] diagnostics to distinguish between different types of DE models. Finally, we compare the physical interpretations of these diagnostic parameters with the standard [Formula: see text]CDM model to assess the viability of each model.
暗能量(DE)的概念是在确认宇宙加速膨胀的结果中出现的。从那时起,人们开发了许多模型来探索DE的起源和本质。在本研究中,我们研究了基于DE状态方程参数化的几种最新宇宙学模型(模型1-9)。我们的分析集中在一个均匀的,各向同性的平坦宇宙,包括暗物质(DM)和辐射。我们假设暗成分(DE和DM)和辐射的单独守恒。通过对[公式:见文]的各种参数化,我们推导出相应的哈勃函数[公式:见文]。为了以独立于模型的方式理解宇宙的宇宙膨胀历史,我们采用宇宙学作为一种方法。我们用哈勃速率(公式:见文本)及其四阶导数来表示重要的宇宙学参数,如减速、急转、急转和勒克参数。此外,我们检查了状态查找器参数和[公式:见文本]诊断,以区分不同类型的DE模型。最后,我们将这些诊断参数的物理解释与标准[公式:见文本]CDM模型进行比较,以评估每个模型的可行性。
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引用次数: 1
Cosmology of New Tsallis Holographic Dark Energy Based Reconstructed Models in Teleparallel Theories 远平行理论中基于新Tsallis全息暗能量重建模型的宇宙学
3区 物理与天体物理 Q2 PHYSICS, MATHEMATICAL Pub Date : 2023-11-04 DOI: 10.1142/s021988782450083x
Saira Waheed
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引用次数: 0
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International Journal of Geometric Methods in Modern Physics
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