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International Journal of Geometric Methods in Modern Physics最新文献

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Plasma-Infused Solitary Waves: Unraveling Novel Dynamics with the Camassa-Holm Equation 注入等离子体的孤波:利用卡马萨-霍姆方程揭示新的动力学原理
Pub Date : 2024-02-02 DOI: 10.1142/s0219887824501469
Chanyuan Wang, Reem Altuijri, A. Abdel‐Aty, K. Nisar, Mostafa M. A. Khater
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引用次数: 0
On the N-waves hierarchy with constant boundary conditions spectral properties 关于具有恒定边界条件光谱特性的 N 波层次结构
Pub Date : 2024-01-31 DOI: 10.1142/S0219887824400152
V. Gerdjikov, G. Grahovski
The paper is devoted to $N$-wave equations with constant boundary conditions related to symplectic Lie algebras. We study the spectral properties of a class of Lax operators $L$, whose potentials $Q(x,t)$ tend to constants $Q_pm$ for $xto pm infty$. For special choices of $Q_pm$ we outline the spectral properties of $L$, the direct scattering transform and construct its fundamental analytic solutions. We generalise Wronskian relations for the case of CBC -- this allows us to analyse the mapping between the scattering data and the $x$-derivative of the potential $Q_x$. Next, using the Wronskian relations we derive the dispersion laws for the $N$-wave hierarchy and describe the NLEE related to the given Lax operator.
本文主要讨论与交映李代数有关的具有恒定边界条件的 $N$ 波方程。我们研究了一类拉克斯算子$L$的谱性质,其势$Q(x,t)$在$xto pm infty$时趋于常数$Q_pm$。对于 $Q_pm$ 的特殊选择,我们概述了 $L$ 的谱特性、直接散射变换并构建了其基本解析解。我们为 CBC 的情况概括了 Wronskian 关系--这使我们能够分析散射数据与势 $Q_x$ 的 $x$ 衍函数之间的映射。接下来,我们利用沃伦斯基关系推导出了 $N$ 波层次的频散规律,并描述了与给定拉克斯算子相关的 NLEE。
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引用次数: 0
Characterizations of η-ρ-Einstein solitons in spacetimes and f(ℛ)-gravity η-ρ-爱因斯坦孤子在时空和 f(ℛ)- 引力中的特征
Pub Date : 2024-01-26 DOI: 10.1142/s021988782450141x
Uday Chand De, Arpan Sardar, F. Mofarreh
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引用次数: 0
Generating f(R,𝒢) gravity from Type IV singular bouncing cosmology 从 IV 型奇异弹跳宇宙学生成 f(R,𝒢)引力
Pub Date : 2024-01-19 DOI: 10.1142/s0219887824501408
G. C. Assolohou, C. Ainamon, C. D. Akowanou, M. Ganiou, M. Houndjo
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引用次数: 0
Intermediate inflation through Nojiri-Odintsov holographic dark fluid with the cosmological settings of Kaniadakis 通过野尻-奥丁佐夫全息暗流与卡尼达基斯的宇宙学设置实现中间膨胀
Pub Date : 2024-01-18 DOI: 10.1142/s0219887824501330
Sanjeeda Sultana, S. Chattopadhyay
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引用次数: 0
Cosmic expansion history analysis with Hubble parametrization in Qn gravity 利用 Qn 引力中的哈勃参数分析宇宙膨胀史
Pub Date : 2024-01-18 DOI: 10.1142/S021988782450138X
M. Koussour, N. Myrzakulov
We propose a specialized parameterization for the Hubble parameter, inspired by $Lambda$CDM cosmology, to investigate the cosmic expansion history of the Universe. This parameterization is employed to analyze the Universe's late-time behavior within the context of $Q^n$ gravity, where $Q$ represents non-metricity. By using data from 57 Hubble data points, 1048 supernova (SNe) data points, and 6 baryon acoustic oscillation (BAO) data points, we determine the optimal values for the model parameters. Additionally, we explore three distinct cosmological models based on the parameter $n$, specifically when it takes on the values of $0.55$, $1.5$, and $2.0$. The results of our analysis indicate that our proposed parameterization, along with the associated models for different values of $n$, predicts an accelerated cosmic expansion phase.
受$Lambda$CDM宇宙学的启发,我们为哈勃参数提出了一个专门的参数化,以研究宇宙的膨胀历史。采用这种参数化方法,可以在$Q^n$引力(其中$Q$代表非度量)的背景下分析宇宙的晚期行为。通过使用来自 57 个哈勃数据点、1048 个超新星(SNe)数据点和 6 个重子声振荡(BAO)数据点的数据,我们确定了模型参数的最佳值。此外,我们还根据参数 $n$,特别是当参数取值为 0.55$、1.5$ 和 2.0$ 时,探索了三种不同的宇宙学模型。我们的分析结果表明,我们提出的参数化,以及不同 $n$ 值的相关模型,预测了一个加速的宇宙膨胀阶段。
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引用次数: 0
Geometric methods in quantum information and entanglement variational principle 量子信息中的几何方法和纠缠变分原理
Pub Date : 2024-01-18 DOI: 10.1142/s0219887824400103
Daniele Iannotti, A. Hamma
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引用次数: 0
Position-dependent mass from noncommutativity and its statistical descriptions 来自非交换性的位置质量及其统计描述
Pub Date : 2024-01-18 DOI: 10.1142/s0219887824501378
Latévi M. Lawson, K. Amouzouvi, K. Sodoga, K. Beltako
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引用次数: 0
Generalized Relativistic Transformations in Clifford Spaces and their Physical Implications 克利福德空间中的广义相对论变换及其物理意义
Pub Date : 2024-01-18 DOI: 10.1142/s0219887824501354
C. Perelman
A brief introduction of the Extended Relativity Theory in Clifford Spaces ( C - space) paves the way to the explicit construction of the generalized relativistic transformations of the Clifford multivector-valued coordinates in C -spaces. The most general transformations furnish a full mixing of the grades of the multivector-valued coordinates. The transformations of the multivector-valued momenta follow leading to an invariant generalized mass M in C -spaces which differs from m . No longer the proper mass appearing in the relativistic dispersion relation E 2 − ⃗p · ⃗p = m 2 remains invariant under the generalized relativistic transformations. It is argued how this finding might shed some light into the cosmological constant problem, dark energy, and dark matter. We finalize with some concluding remarks about extending these transformations to phase spaces and about Born reciprocal relativity. An appendix is included with the most general (anti) commutators of the Clifford algebra multivector generators.
对克利福德空间(C 空间)中的广义相对论的简要介绍,为明确构建 C 空间中克利福德多矢量值坐标的广义相对论变换铺平了道路。最一般的变换提供了多矢量值坐标等级的全面混合。多矢量值矩的变换会导致 C 空间中的不变广义质量 M,它与 m 不同。在广义相对论变换下,相对论色散关系 E 2 - ⃗p - ⃗p = m 2 中出现的适当质量不再保持不变。我们论证了这一发现如何可能给宇宙常数问题、暗能量和暗物质带来一些启示。最后,我们对将这些变换扩展到相空间和玻恩互易相对论作了一些总结性评论。附录中包含了克利福德代数多向量生成器的最一般(反)换元。
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引用次数: 0
A Closed Universe with Hybrid Nonlocality 具有混合非位置性的封闭宇宙
Pub Date : 2024-01-18 DOI: 10.1142/s0219887824400127
Branko Dragovich
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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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