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Representation up to Homotopy and Hom-Lie Algebroid Modules 到同伦和同李代数模的表示
IF 0.9 Q4 MATHEMATICS Pub Date : 2020-01-02 DOI: 10.1080/1726037X.2020.1788817
S. Merati, M. R. Farhangdoost, A.R. Attari Polsangi
Abstract In this paper we introduce the concept of hom-Lie algebroid modules and hom-Lie algebroids. Then we show the correspondence between hom-Lie algebroid modules and representation up to homotopy of hom-Lie algebroids. Because of the effective role of representation theory and Lie algebraic structures in particle physics, we show the correspondence between bi-graded hom-Lie algebraic modules and hom-Lie algebraist. At the end, we study some properties of representation up to homotopy, using the language of hom-Lie algebroid modules.
摘要本文介绍了hom李代数体模和hom李算法体的概念。然后我们给出了hom-Lie代数体模与hom-Lie算法体的表示之间的对应关系。由于表示论和李代数结构在粒子物理学中的有效作用,我们展示了二阶hom-Lie代数模与hom-Lie算子之间的对应关系。最后,利用hom-Lie代数体模的语言,研究了表示到同伦论的一些性质。
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引用次数: 1
Dynamics Of Frw Type Kaluza-Klein Mhrde Cosmological Model In Self-Creation Theory 自我创造理论中Frw型Kaluza-Klein Mhrde宇宙学模型的动力学
IF 0.9 Q4 MATHEMATICS Pub Date : 2020-01-02 DOI: 10.1080/1726037X.2020.1774158
T. Vinutha, K. S. Sri Kavya
ABSTRACT In this work, we have studied Friedmann–Robertson–Walker type Kaluza–Klein universe filled with pressureless matter and modified holographic Ricci dark energy in the frame work of Barber’s self-creation theory. While solving field equations we have considered hybrid expansion law of average scale factor. Also we have studied differences between open, flat and closed models. We have calculated some physical properties such as deceleration parameter(q), EoS parameter(ωde ), spatial volume(V ), expansion scalar(θ). The physical and geometrical aspects of the statefinder parameters(r, s) and ωde − ω ′ de plane are also discussed. In ω de− ω ′ de plane discussion we have observed that the flat model lies in freezing region and the closed model lies in thawing region. Also we have observed that for flat model ωde crosses the phantom divide line( i.e. ωde = -1) and shows quintom like behavior. Among the three models the flat model is in good agreement with recent observational data.
本研究在Barber自我创造理论的框架下,研究了充满无压物质和修正全息Ricci暗能量的friedman - robertson - walker型Kaluza-Klein宇宙。在求解场方程时,考虑了平均尺度因子的混合展开律。我们还研究了开放、平坦和封闭模型之间的差异。我们计算了一些物理性质,如减速参数(q), EoS参数(ωde),空间体积(V),膨胀标量(θ)。还讨论了定位仪参数(r, s)和ωde - ωde平面的物理和几何方面。在ω de−ω de平面讨论中,我们观察到平面模型位于冻结区,封闭模型位于解冻区。此外,我们还观察到,对于平面模型,ωde穿过幻相分割线(即ωde = -1),并显示出类似琴的行为。在三种模式中,平面模式与近期观测资料吻合较好。
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引用次数: 1
Characteristic of pointwise-recurrent maps on a dendrite 枝晶上逐点递归映射的特征
IF 0.9 Q4 MATHEMATICS Pub Date : 2020-01-02 DOI: 10.1080/1726037X.2020.1779971
G. Su, T. Sun, Caihong Han, Bin Qin
Abstract Let f be a continuous map on a dendrite D with f (D) = D. Denote by R(f ) and AP (f ) the set of recurrent points and the set of almost periodic points of f , respectively, and denote by ω(x, f ), Λ(x, f ), Γ(x, f ) and Ω(x, f ) the set of ω-limit points, the set of α-limit points, the set of γ-limit points and the set of weak ω-limit points of x under f , respectively. In this paper, we show that the following statements are equivalent: (1) D = R(f ). (2) D = AP (f ). (3) Ω(x, f ) = ω(x, f ) for any x ∈ D. (4) Ω(x, f ) = Γ(x, f ) for any x ∈ D. (5) f is equicontinuous. (6) [c, d] ⊄ Ω(x, f ) for any c, d,x ∈ D with c ≠ (7) Ω(x, f ) is minimal for any x ∈ D. (8) Card(Λ − 1(x, f ) ∩ (D−End(D))) < ∞ for any x ∈ D, where Λ − 1(x, f ) = {y : x ∈ Λ(y, f )}, End(D) is the set of endpoints of D and Card(A) is the cardinal number of set A. (9) If x ∈ Λ(y, f ) with x, y ∈ D, then y ∈ ω(x, f ). (10) Map h : x → ω(x, f ) (x ∈ D) is continuous and for any x, y ∈ D with x ∉ ω(y, f ), ω(x, f ) ≠ ω(y, f ). Besides, we also study characteristic of pointwise-recurrent maps on a dendrite with the number of branch points being finite.
抽象让f是一个连续的地图与f (D) =树突D D表示R (f)和美联社(f)复发的设置点和f的组几乎周期点,分别表示,ω(x, f),Λ(x, f),Γ(x, f)和Ω(x, f)的集合ω极限点,α的极限点,γ的极限点和弱ω的极限点的x在f,分别。本文证明了下列表述是等价的:(1)D = R(f)。D = AP (f)。(3)对于任意x∈d Ω(x, f) = Ω(x, f);(4)对于任意x∈d Ω(x, f) = Γ(x, f); (5) f是等连续的。(6) (c, d)⊄Ω(x, f)对任何c, d, x∈d c≠(7)Ω(x, f)是最小的x∈d(8)卡(Λ−1 (x, f)∩(d−结束(d))) <∞任何x∈d,Λ−1 f (x) = {y: x∈Λ(y, f)}, (d)是一组端点的d和卡(A)是集的基数A(9)如果x∈Λ(y, f)与x, y∈d,那么y∈ω(x, f)。(10)映射h: x→ω(x, f) (x∈D)是连续的,且对于任意x, y∈D,∈x∈D,∈x∈x∈f,∈x∈f≠ω(y, f)。此外,我们还研究了分支点数目有限的树突上的点向循环映射的特性。
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引用次数: 1
Submersions of Contact CR-Submanifolds of Generalized Quasi Sasakian Manifolds 广义拟sasaki流形的接触cr -子流形的淹没
IF 0.9 Q4 MATHEMATICS Pub Date : 2020-01-02 DOI: 10.1080/1726037X.2020.1796247
M. Siddiqi
Abstract In this paper, we discuss some properties of almost contact metric submersion of contact CR-submanifolds of generalized quasi-Sasakian manifold and derive some results based on their curvatures’s differential geometry. We also study de-Rham cohomology of CR-submanifold of generalized quasi-Sasakian manifold under the submersion.
本文讨论了广义拟sasaki流形的接触cr -子流形的几乎接触度量淹没的一些性质,并基于它们的曲率微分几何得到了一些结果。我们还研究了广义拟sasaki流形在淹没下cr -子流形的de-Rham上同调。
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引用次数: 1
On Differential Geometric Formulations of Slow Invariant Manifold Computation: Geodesic Stretching and Flow Curvature 慢不变流形计算的微分几何公式:测地线拉伸和流动曲率
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-12-02 DOI: 10.1080/1726037X.2022.2060909
D. Lebiedz, Johannes Poppe
Abstract The theory of slow invariant manifolds (SIMs) is the foundation of various model-order reduction techniques for dissipative dynamical systems with multiple time-scales, e.g. in chemical kinetic models. The construction of SIMs and many approximation methods exploit the restrictive requirement of an explicit time-scale separation parameter. Most of those methods are also not formulated covariantly, i.e. in terms of tensorial constructions. We propose an intrinsically coordinate-free differential geometric approximation criterion approximating normally attracting invariant manifolds (NAIMs). We translate some ideas behind existing approximation approaches, the stretching based diagnostics (SBD) and the flow curvature method (FCM) to tensors of Riemannian geometry, specifically to spacetime curvature in extended phase space. For that purpose we derive from flow-generating smooth vector fields a metric tensor such that the original dynamical system is a geodesic flow on a Riemannian manifold. We apply the resulting method to test models.
慢不变流形(slow invariant manifold, SIMs)理论是多种多时标耗散动力系统模型降阶技术的基础,如化学动力学模型。SIMs的构造和许多近似方法利用了明确的时间尺度分离参数的限制性要求。这些方法中的大多数也不是协变的,即在张量结构方面。提出了一种近似常吸引不变流形的本质无坐标微分几何逼近准则。我们将现有的近似方法,基于拉伸的诊断(SBD)和流动曲率方法(FCM)背后的一些思想转化为黎曼几何的张量,特别是扩展相空间中的时空曲率。为此,我们从产生流的光滑向量场中导出一个度量张量,使得原始动力系统是黎曼流形上的测地线流。我们将得到的方法应用于测试模型。
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引用次数: 0
Yamabe Solitons On (LCS) n -Manifolds (LCS) n -流形上的Yamabe孤子
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-09-14 DOI: 10.1080/1726037X.2020.1868100
Soumendu Roy, S. Dey, A. Bhattacharyya
Abstract The object of the present paper is to study some properties of (LCS) n -manifolds whose metric is Yamabe soliton. We establish some characterization of (LCS) n -manifolds when the soliton becomes steady. Next we have studied some certain curvature conditions of (LCS) n -manifolds admitting Yamabe solitons. Lastly we construct a 3-dimensional (LCS) n -manifold satisfying the results.
摘要本文研究了度规为Yamabe孤子的(LCS) n流形的一些性质。建立了n -流形在孤子稳定时的一些表征。其次,我们研究了允许Yamabe孤子的(LCS) n -流形的某些曲率条件。最后构造了一个满足上述结果的三维n流形。
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引用次数: 15
Lyapunov Exponents for Quantum Channels: An Entropy Formula and Generic Properties 量子通道的Lyapunov指数:一个熵公式和一般性质
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-08-22 DOI: 10.1080/1726037X.2021.2014635
Jader E. Brasil, J. Knorst, A. Lopes
Abstract We denote by Mk the set of k by k matrices with complex entries. We consider quantum channels φL of the form: given a measurable function L: Mk → Mk and a measure µ on Mk we define the linear operator φL : Mk → Mk , by the law ρ → φL (ρ) = ∫ Mk L(v)ρL(v)† dµ(v). In a previous work, the authors show that for a fixed measure µ the Φ-Erg property is generic on the function L (also irreducibility). Here we will show that the purification property is also generic on L for a fixed µ. Given L and µ there are two related stochastic processes: one takes values on the projective space P (ℂ k ) and the other on matrices in Mk . The Φ-Erg property and the purification condition are the nice hypothesis for the discrete time evolution given by the natural transition probability. In this way it will follow that generically on L, if ∫ |L(v)|2 log |L(v)| dµ(v) < ∞, the Lyapunov exponents ∞ > γ 1 ≥ γ 2 ≥ … ≥ γk ≥ −∞ are well defined. In a previous work, the concepts of entropy of a channel and Gibbs channel were presented; and also an example (associated to a stationary Markov chain) in which this definition of entropy (for a quantum channel) matches the Kolmogorov-Shanon definition of entropy. We estimate here the larger Lyapunov exponent for the mentioned example and we show that it is equal to −1/2 h, where h is the entropy of the associated Markov invariant probability.
我们用Mk表示含有复元素的k × k矩阵的集合。给出一个可测函数L: Mk→Mk和一个测度μ on Mk,根据ρ→φL (ρ) =∫Mk L(v)ρL(v)†dµ(v)的定律,定义了线性算子φL: Mk→Mk。在之前的工作中,作者证明了对于一个固定测度µ,Φ-Erg性质在函数L上是泛型的(也是不可约的)。这里我们将证明,对于固定µ,L上的纯化性质也是一般的。给定L和µ,有两个相关的随机过程:一个取射影空间P (k)上的值,另一个取Mk中的矩阵上的值。Φ-Erg性质和净化条件是由自然跃迁概率给出的离散时间演化的良好假设。由此可以得出,一般在L上,如果∫|L(v)|2 log |L(v)| dµ(v) <∞,则Lyapunov指数∞> γ 1≥γ 2≥…≥γk≥−∞是有定义的。在前人的研究中,提出了通道熵和吉布斯通道熵的概念;还有一个例子(与固定马尔可夫链相关),其中熵的定义(用于量子通道)与柯尔莫戈洛夫-香农熵的定义相匹配。我们在这里估计较大的李雅普诺夫指数对于上面提到的例子,我们表明它等于- 1/2 h,其中h是相关的马尔可夫不变概率的熵。
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引用次数: 4
Kaluza Klein Type FRW Cosmological Model With Extended Chaplygin Gas 扩展Chaplygin气体的Kaluza Klein型FRW宇宙学模型
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-07-03 DOI: 10.1080/1726037X.2019.1651491
G. S. Khadekar, N. Ramtekkar
Abstract In this paper we consider the extended Chaplygin gas equation of state as a model of dark energy for which it recovers barotropic fluids with quadratic equation of state. We obtain scale factor dependence energy density and Hubble expansion parameter for particular values of n, m and α. Similarly for arbitrary values of n, m and α we have discuss nature of cosmological parameters such as scale factor, Hubble expansion parameter, time dependent dark energy density and deceleration parameter in the framework of Kaluza Klein type FRW cosmological model. Further, we study stability of the model by using speed of sound and observe that the model is stable at late time.
摘要本文将扩展的Chaplygin气体状态方程视为暗能量模型,用二次状态方程来恢复正压流体。对于n、m和α的特定值,我们获得了与比例因子相关的能量密度和哈勃展开参数。类似地,对于任意值的n、m和α,我们在Kaluza-Klein型FRW宇宙学模型的框架下讨论了宇宙学参数的性质,如比例因子、哈勃膨胀参数、随时间变化的暗能量密度和减速参数。此外,我们利用声速研究了模型的稳定性,并观察到模型在后期是稳定的。
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引用次数: 0
On a Multifractal Pressure for Countable Markov Shifts 关于可数Markov位移的多重分形压力
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-07-03 DOI: 10.1080/1726037X.2019.1668150
A. Mesón, F. Vericat
Abstract In a recent article [J. d' Analyse Math 131, 207, 2017], Olsen intoduced a generalized notion of multifractal pressure, and also a multifractal dynamical zeta function, which essentilly consists in considering not all configurations, but those which are ”multifractally relevant”. In this way more precise information about the multifractal spectrum analyzed is encoded by the multifractal pressure and the multifratcal zeta function. He applied the theory for dynamical systems modelled by finite alphabet shifts, in particular for self conformal iterated systems. Here we continue with this line considering dynamical systems given by countable Markov shifts.
摘要在最近的一篇文章[J.d'Analyze Math 1312072017]中,Olsen引入了多重分形压力的广义概念,以及多重分形动态ζ函数,该函数本质上不包括所有配置,而是考虑那些“多重分形相关”的配置。以这种方式,关于所分析的多重分形谱的更精确的信息由多重分形压力和多重分形ζ函数编码。他将该理论应用于由有限字母移位建模的动力学系统,特别是自共形迭代系统。在这里,我们继续这条线,考虑由可数马尔可夫位移给出的动力系统。
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引用次数: 1
Cosmological Application in Kaluza-Klein Theory: Generalized Sudden Singularity Kaluza-Klein理论中的宇宙学应用:广义突发性奇点
IF 0.9 Q4 MATHEMATICS Pub Date : 2019-07-03 DOI: 10.1080/1726037X.2019.1668147
Rupali Wanjari, G. S. Khadekar
Abstract In this paper, we considered the cosmological application by taking G and Λ to be a function of t in Kaluza-Klein cosmology. We use the Taylor’s expansion of cosmological function Λ(t), up to the first order of time t and evaluated the cosmological parameters by using the modified equation of state of the form p = −ρ − f (ρ), where f (ρ) = αρ. The analytical properties of R(t), ρ(t) and H(t) are investigated and it is observed that from the solutions of the field equations, the generalized sudden singularity occurs at a finite time in the framework of Kaluza-Klein theory of gravitation.
摘要在本文中,我们通过将G和∧作为Kaluza-Klein宇宙学中t的函数来考虑宇宙学的应用。我们使用宇宙学函数∧(t)的泰勒展开,直到时间t的一阶,并通过使用形式为p=-ρ−f(ρ)的修正状态方程来评估宇宙学参数,其中f(ρ)=αρ。研究了R(t)、ρ(t)和H(t)的解析性质,并从场方程的解中观察到,在Kaluza-Klein引力理论的框架下,广义突然奇异性在有限时间内发生。
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引用次数: 0
期刊
Journal of Dynamical Systems and Geometric Theories
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