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Möbius group actions in the solvable chimera model 可解嵌合体模型中的莫比乌斯群作用
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-05-16 DOI: 10.1142/s0217979225400053
Vladimir Jaćimović, Aladin Crnkić

We study actions of Möbius group on two sub-populations in the solvable chimera model proposed by Abrams et al. Dynamics of global variables are given by two coupled Watanabe–Strogatz systems, one for each sub-population. At the first glance, asymptotic dynamics in the model seem to be very simple. For instance, in the stable chimera state distributions of oscillators perform a simple rotation after a certain (sufficiently large) moment. However, a closer look unveils that dynamics are subtler that what can be observed from evolution of densities of oscillators’ phases. In order to gain the full picture, one needs to investigate dynamics on the transformation group that acts on these densities. Such an approach emphasizes impact of the “hidden” variable that is not visible on macroscopic level. More precisely, we demonstrate that the chimera model is an intriguing example of the classical system that exhibits the holonomy in fiber bundles of the group of Möbius transformations.

我们研究了艾布拉姆斯等人提出的可解嵌合体模型中莫比乌斯群对两个子群的作用。全局变量的动力学由两个耦合的瓦塔纳贝-斯特罗加茨系统给出,每个子群一个。乍一看,该模型的渐近动力学似乎非常简单。例如,在稳定的嵌合体状态下,振荡器的分布在某个(足够大的)时刻后会发生简单的旋转。然而,仔细观察就会发现,与振荡器相位密度的演变相比,动态变化更为微妙。为了了解全貌,我们需要研究作用于这些密度的变换群的动力学。这种方法强调了宏观上不可见的 "隐藏 "变量的影响。更准确地说,我们证明了嵌合体模型是经典系统的一个有趣例子,它在莫比乌斯变换群的纤维束中表现出整体性。
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引用次数: 0
On the solutions of space-time fractional CBS and CBS-BK equations describing the dynamics of Riemann wave interaction 论描述黎曼波相互作用动力学的时空分数 CBS 和 CBS-BK 方程的解
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-05-08 DOI: 10.1142/s0217979225400016
A. K. Sahoo, A. K. Gupta, Aly R. Seadawy

In this paper, Kudryashov and modified Kudryashov methods are implemented for the first time to compute new exact traveling wave solutions of the space-time fractional (3+1)-dimensional Calogero–Bogoyavlenskii–Schiff (CBS) equation and Calogero–Bogoyavlenskii–Schiff and Bogoyavlensky Konopelchenko (CBS-BK) equation. With the help of wave transformation, the aforementioned fractional differential equations are converted into nonlinear ordinary differential equations. The purpose of this paper is to devise novel exact solutions for the space-time-fractional (3+1)-dimensional CBS and the space-time-fractional CBS-BK equations by utilizing the Kudryashov and modified Kudryashov techniques. The solutions, thus, acquired are demonstrated in figures by choosing appropriate values for the parameters. The solutions derived take the form of various wave patterns, including the kink type, the anti-kink type and the singular kink wave solutions. The obtained solutions are indeed beneficial to analyze the dynamic behavior of fractional CBS and CBS-BK equations in describing the interesting physical phenomena and mechanisms. The obtained solutions are entirely new and can be considered as a generalization of the existing results in the ordinary derivative case. The techniques presented here are very simple, efficacious and plausible and hence can be employed to attain new exact solutions for fractional PDEs.

本文首次采用库德亚绍夫方法和修正库德亚绍夫方法计算了时空分数 (3+1)-dimensional Calogero-Bogoyavlenskii-Schiff (CBS) 方程和 Calogero-Bogoyavlenskii-Schiff and Bogoyavlensky Konopelchenko (CBS-BK) 方程的新精确行波解。借助波变换,上述分数微分方程被转换为非线性常微分方程。本文旨在利用库德里亚绍夫技术和修正库德里亚绍夫技术,为时空分式 (3+1)-dimensional CBS 和时空分式 CBS-BK 方程设计新的精确解。通过选择适当的参数值,可以用图表展示由此获得的解。求得的解具有各种波形,包括扭结波、反扭结波和奇异扭结波。所得到的解确实有利于分析分数 CBS 和 CBS-BK 方程在描述有趣的物理现象和机制时的动态行为。所获得的解是全新的,可视为普通导数情况下现有结果的推广。这里介绍的技术非常简单、有效且可行,因此可用于获得分数 PDE 的新精确解。
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引用次数: 0
Electro-fluid-dynamics (EFD) of soft-bodied organisms swimming through mucus having dilatant, viscous, and pseudo-plastic properties 软体生物在具有扩张、粘性和假塑性特性的粘液中游泳的电流体动力学(EFD)
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-30 DOI: 10.1142/s0217979225500110
Zeeshan Asghar, Rehman Ali Shah, Muhammad Waqas, Muhammad Asif Gondal

The sperm propelling mechanism has been proposed as a possible resource for soft micro-robots in confined spaces, with potential applications in biomedical engineering. Human sperm cells essentially swim through the non-Newtonian liquid (cervical mucus) to reach their target. Thus, sperm cells swimming through non-Newtonian fluids is not vital only for physiology, but also for the fabrication of swimming micro-robots. Inspired by these remarkable applications, we examine the basic mechanics of spermatozoa motility using an undulating sheet model. This undulating sheet is bounded between two rigid walls which is self-propeling in the negative axial direction. The liquid around the spermatozoa is taken as Carreau fluid with electro-osmotic properties. The application of the lubrication approximation results in the reduction of momentum equations. The resulting ODE is solved numerically via the finite difference method and MATLAB’s built-in routine bvp5c. The unknowns that are present in the boundary conditions are refined by the root-finding algorithm. Power losses, cell speed, flow rate, velocity of the fluid, and streamline pattern are visualized by graphs. The findings of this study have important implications for the designing and optimization of electrically controlled microswimmers.

精子推进机制被认为是密闭空间中软体微型机器人的一种可能资源,在生物医学工程中具有潜在的应用价值。人类精子细胞基本上是游过非牛顿液体(宫颈粘液)到达目标的。因此,精子细胞在非牛顿流体中游动不仅对生理学至关重要,而且对制造游动微型机器人也至关重要。受这些杰出应用的启发,我们利用起伏片模型研究了精子运动的基本力学原理。这个起伏的薄片被束缚在两面刚性壁之间,沿负轴向自我推进。精子周围的液体是具有电渗特性的卡勒流体。润滑近似的应用导致动量方程的简化。通过有限差分法和 MATLAB 的内置例程 bvp5c 对所得到的 ODE 进行数值求解。边界条件中的未知数通过寻根算法进行细化。功率损耗、电池速度、流速、流体速度和流线模式通过图表可视化显示。这项研究的结果对电控微泳器的设计和优化具有重要意义。
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引用次数: 0
Application of micropolar fluid model to blood flow through catheterized artery with stenosis and thrombosis 将微极性流体模型应用于狭窄和血栓形成的导管动脉血流
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-30 DOI: 10.1142/s0217979225500481
Muhammad Ashfaq, Zeeshan Asghar, Yufeng Nie, Wasfi Shatanawi

This paper presents a model of nonisothermal blood flow through a diseased arterial segment due to the presence of stenosis and thrombosis. The rheological properties of the blood in the annulus are captured by utilizing micropolar fluid model. The equation describing the blood flow and heat transfer is developed under the assumption that stenosis growth into the lumen of the artery is small as compared to the average radius of the artery. Biological processes like intimal proliferation of cells or changes in artery caliber may be activated by small growths that cause moderate stenotic blockages. Closed-form solutions for temperature, velocity, resistance impedance and wall shear stress are obtained and then utilized to estimate the impact of various physical parameters on micropolar blood flow. Graphs are plotted to illustrate variations in temperature, velocity, shear stress at the wall and resistance impedance against different controlling parameters. The results are also validated via the bvp4c approach.

本文介绍了一个由于动脉狭窄和血栓形成而流经病变动脉段的非等温血流模型。利用微极性流体模型捕捉到了动脉环中血液的流变特性。描述血液流动和热量传递的方程是在假定与动脉平均半径相比,狭窄处向动脉腔内的生长很小的情况下建立的。生物过程,如内膜细胞增殖或动脉口径的变化,可能会被导致中度狭窄堵塞的微小增生激活。我们获得了温度、速度、阻抗和壁剪应力的闭式解,然后利用这些解来估算各种物理参数对微极血流的影响。图表说明了温度、速度、管壁剪应力和阻抗随不同控制参数的变化。这些结果还通过 bvp4c 方法进行了验证。
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引用次数: 0
Investigating the effect of oxygen vacancy on electronic, optical, thermoelectric and thermodynamic properties of CeO2 (ceria) for energy and ReRAM applications: A first-principles quantum analysis 研究氧空位对用于能源和 ReRAM 应用的 CeO2(铈)的电子、光学、热电和热力学特性的影响:第一原理量子分析
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-17 DOI: 10.1142/s0217979225500389
Shafaat Hussain Mirza, Sikander Azam, Zeesham Abbas, Shoyebmohamad F. Shaikh
<p>CeO<sub>2</sub> thin film-based devices have become hot favorite candidates for researchers due to the outstanding characteristics of ceria such as memory storage materials, high oxygen storage capacity, excellent chemical and thermal stability, high transparency in visible region and highly tunable energy band structures. Developing suitable materials for industrial uses like optoelectronic and thermoelectric devices is the primary goal of researchers in the field of renewable energy. Herein, we have investigated the optical, thermoelectric and thermodynamic properties of CeO<sub>2</sub> and <span><math altimg="eq-00001.gif" display="inline" overflow="scroll"><msub><mrow><mstyle><mtext mathvariant="normal">CeO</mtext></mstyle></mrow><mrow><mn>2</mn></mrow></msub><mo>+</mo><msub><mrow><mstyle><mtext mathvariant="normal">V</mtext></mstyle></mrow><mrow><mstyle><mtext mathvariant="normal">O</mtext></mstyle></mrow></msub></math></span><span></span> as promising candidates for energy applications using first-principles calculations. We can observe significant absorption of incident photons by CeO<sub>2</sub> and <span><math altimg="eq-00002.gif" display="inline" overflow="scroll"><msub><mrow><mstyle><mtext mathvariant="normal">CeO</mtext></mstyle></mrow><mrow><mn>2</mn></mrow></msub><mo>+</mo><msub><mrow><mstyle><mtext mathvariant="normal">V</mtext></mstyle></mrow><mrow><mstyle><mtext mathvariant="normal">O</mtext></mstyle></mrow></msub></math></span><span></span> near UV region. The highest peaks of the <span><math altimg="eq-00003.gif" display="inline" overflow="scroll"><msub><mrow><mi>ε</mi></mrow><mrow><mn>2</mn></mrow></msub><mo stretchy="false">(</mo><mi>ω</mi><mo stretchy="false">)</mo></math></span><span></span> are present around 3.7<span><math altimg="eq-00004.gif" display="inline" overflow="scroll"><mspace width=".17em"></mspace></math></span><span></span>eV in spin <span><math altimg="eq-00005.gif" display="inline" overflow="scroll"><mi>↑</mi></math></span><span></span> channel, however, in spin <span><math altimg="eq-00006.gif" display="inline" overflow="scroll"><mi>↓</mi></math></span><span></span> channel, the highest peaks of the <span><math altimg="eq-00007.gif" display="inline" overflow="scroll"><msub><mrow><mi>ε</mi></mrow><mrow><mn>2</mn></mrow></msub><mo stretchy="false">(</mo><mi>ω</mi><mo stretchy="false">)</mo></math></span><span></span> are present around 3.5<span><math altimg="eq-00008.gif" display="inline" overflow="scroll"><mspace width=".17em"></mspace></math></span><span></span>eV. The most intense peaks that emerge are due to the transitions of O[<span><math altimg="eq-00009.gif" display="inline" overflow="scroll"><msup><mrow><mn>2</mn><mi>p</mi></mrow><mrow><mn>4</mn></mrow></msup></math></span><span></span>] to Ce [<span><math altimg="eq-00010.gif" display="inline" overflow="scroll"><msup><mrow><mn>4</mn><mi>f</mi></mrow><mrow><mn>1</mn></mrow></msup></math></span><span></span>]. The investigated values of <span><ma
由于铈具有存储记忆材料、高储氧能力、优异的化学和热稳定性、可见光区域的高透明度以及高度可调的能带结构等突出特性,基于 CeO2 薄膜的设备已成为研究人员的热门候选对象。为光电和热电设备等工业用途开发合适的材料是可再生能源领域研究人员的首要目标。在此,我们利用第一性原理计算研究了 CeO2 和 CeO2+VO 的光学、热电和热力学性质,并将其作为能源应用的理想候选材料。我们可以观察到 CeO2 和 CeO2+VO 在紫外区附近对入射光子的显著吸收。在自旋 ↑ 通道中,ε2(ω)的最高峰出现在 3.7eV 附近;而在自旋 ↓ 通道中,ε2(ω)的最高峰出现在 3.5eV 附近。出现的最高峰是由于 O[2p4] 到 Ce [4f1] 的跃迁。n(ω) 的研究值表明 CeO2 和 CeO2+VO 是活性光学材料。在整个能量范围内,CeO2 和 CeO2+VO 反射的入射光子数量微乎其微(∼20%)。S 值为正表示所研究的 CeO2 是 p 型半导体,而 CeO2+VO 是 n 型半导体,因为其 S 值为负。CeO2 的 S 值接近既定标准。因此,CeO2 是一种可用于设备的热电材料。功值(ZT)光谱显示,与 CeO2+VO (ZT=0.14)相比,CeO2(ZT=1.01)更适合用作热电材料。所研究的热力学参数表明,CeO2 和 CeO2+VO 是动态稳定的化合物。
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Herein, we have investigated the optical, thermoelectric and thermodynamic properties of CeO&lt;sub&gt;2&lt;/sub&gt; and &lt;span&gt;&lt;math altimg=\"eq-00001.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;CeO&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;V&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;O&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; as promising candidates for energy applications using first-principles calculations. We can observe significant absorption of incident photons by CeO&lt;sub&gt;2&lt;/sub&gt; and &lt;span&gt;&lt;math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;CeO&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;V&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mstyle&gt;&lt;mtext mathvariant=\"normal\"&gt;O&lt;/mtext&gt;&lt;/mstyle&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; near UV region. The highest peaks of the &lt;span&gt;&lt;math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;ε&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;mi&gt;ω&lt;/mi&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; are present around 3.7&lt;span&gt;&lt;math altimg=\"eq-00004.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mspace width=\".17em\"&gt;&lt;/mspace&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;eV in spin &lt;span&gt;&lt;math altimg=\"eq-00005.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;↑&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; channel, however, in spin &lt;span&gt;&lt;math altimg=\"eq-00006.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mi&gt;↓&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; channel, the highest peaks of the &lt;span&gt;&lt;math altimg=\"eq-00007.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mi&gt;ε&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;mo stretchy=\"false\"&gt;(&lt;/mo&gt;&lt;mi&gt;ω&lt;/mi&gt;&lt;mo stretchy=\"false\"&gt;)&lt;/mo&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt; are present around 3.5&lt;span&gt;&lt;math altimg=\"eq-00008.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;mspace width=\".17em\"&gt;&lt;/mspace&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;eV. The most intense peaks that emerge are due to the transitions of O[&lt;span&gt;&lt;math altimg=\"eq-00009.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;mi&gt;p&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;4&lt;/mn&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;] to Ce [&lt;span&gt;&lt;math altimg=\"eq-00010.gif\" display=\"inline\" overflow=\"scroll\"&gt;&lt;msup&gt;&lt;mrow&gt;&lt;mn&gt;4&lt;/mn&gt;&lt;mi&gt;f&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;/mrow&gt;&lt;/msup&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;/span&gt;]. The investigated values of &lt;span&gt;&lt;ma","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"12 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140610324","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
Novel optical solitons patterns via Biswas–Arshed equation with gain or loss. Modulated wave gain 通过具有增益或损耗的 Biswas-Arshed 方程实现新颖的光学孤子模式调制波增益
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-03 DOI: 10.1142/s0217979225500171
H. I. Abdel-Gawad

The Biswas–Arshed equation (BAE) with space–time dispersion was currently considered in the literature. Optical phenomena embedded in this equation are self-steepening, self-phase modulation and Raman scattering. Here, we consider BAE with gain or loss. It is worth mentioning that the gain or loss has an impact on blowup or decaying solitons propagation in optical fibers, which is novel. Our objective is to find optical soliton solutions of BAE and the aforementioned physical phenomena are investigated in some details. The conditions for the dominance of a phenomenon are predicted. This is physically important to inspect the behavior of solitons prpagation. To this issue, exact solutions of the model equation are derived by using the unified method. The solutions obtained are displayed graphically. Dark soliton, bright soliton, M-shaped soliton, rhombus soliton (which is novel) and chirped soliton with tunneling are observed. The modulation instability is studied and it is found that it triggers when the coefficients of the space–time dispersions are positive.

目前的文献考虑了具有时空色散的 Biswas-Arshed 方程 (BAE)。该方程中包含的光学现象有自膨胀、自相位调制和拉曼散射。在这里,我们考虑的是具有增益或损耗的 BAE。值得一提的是,增益或损耗会影响孤子在光纤中的传播,这一点很新颖。我们的目标是找到 BAE 的光学孤子解,并对上述物理现象进行了详细研究。我们预测了一种现象占主导地位的条件。这对于检验孤子的传播行为具有重要的物理意义。为此,利用统一方法推导出了模型方程的精确解。得到的解以图形显示。观察到了暗孤子、亮孤子、M 形孤子、菱形孤子(新颖)和带有隧道的啁啾孤子。对调制不稳定性进行了研究,发现当时空色散系数为正时,调制不稳定性就会触发。
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引用次数: 0
Influence of temperature on Rashba effect of bound polaron in a parabolic quantum well 温度对抛物面量子阱中束缚极子的拉什巴效应的影响
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-03 DOI: 10.1142/s0217979225500286
Ya-Li Li, Shu-Ping Shan

In this paper, using an improved linear combination operator method and variational technique, the expression of the bound polaron effective mass ratio in a parabolic quantum well is derived. Due to the spin–orbit interaction, the effective mass ratio of bound polaron splits into two branches. The relations among effective mass ratio with temperature, electron–phonon coupling strength and Coulomb bound potential strength are discussed by numerical calculation. The effective mass ratio of polaron is an increasing function of temperature, electron–phonon coupling strength and Coulomb bound potential strength. The absolute value of spin splitting effective mass ratio increases with the increase of temperature, spin–orbit coupling parameter, electron–phonon coupling strength and Coulomb bound potential strength, respectively, and decreases with the increase of velocity. Due to the heavy hole characteristic, the spin splitting effective mass ratio is negative.

本文利用改进的线性组合算子方法和变分技术,推导了抛物面量子阱中束缚极子有效质量比的表达式。由于自旋轨道相互作用,束缚极子的有效质量比分成两个分支。通过数值计算讨论了有效质量比与温度、电子-声子耦合强度和库仑束缚势强度之间的关系。极子的有效质量比是温度、电子-声子耦合强度和库仑束缚势强度的递增函数。自旋分裂有效质量比的绝对值分别随温度、自旋轨道耦合参数、电子-声子耦合强度和库仑束缚势强度的增大而增大,随速度的增大而减小。由于重空穴特性,自旋分裂有效质量比为负值。
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引用次数: 0
Numerical heat featuring in radiative convective ternary nanofluid under induced magnetic field and heat generating source 诱导磁场和发热源作用下辐射对流三元纳米流体的热特征数值计算
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-03 DOI: 10.1142/s0217979225500444
Adnan, Waseem Abbas, Aisha M. Alqahtani, Zafar Mahmood, Sid Ahmed Ould Beinane, Muhammad Bilal

The study of nanoliquid characteristics and their heat performance have attracted the interest of engineers. These engineered fluids have high thermal conductivity due to which such liquids are reliable for different engineering applications including heating/cooling of buildings, thermal and mechanical engineering, etc. Therefore, the current research design provides a new ternary nanoliquid model for the heat transport process under induced magnetic field effects, mixed convection, heating source and thermal radiations. The modeling has been done by implementing the ternary fluid characteristics and supportive transformations and then for results simulation; bvp4c is coded successfully. It is scrutinized that a higher inductive magnetic field (0.1–0.4) and nanoparticles amount (0.01–0.07) are better to resist the movement while the wedge parameter (λ1) promotes it. By promoting the heating source, Eckert and Rd, the heat transfer process is observed rapidly while the mixed convective number α controls it. Further, the particular used ternary nanoliquid is examined and found to be good for cooling purposes.

对纳米液体特性及其热性能的研究引起了工程师们的兴趣。这些工程液体具有很高的热导率,因此在不同的工程应用中,包括建筑物的加热/冷却、热能和机械工程等,这些液体都是可靠的。因此,当前的研究设计为诱导磁场效应、混合对流、加热源和热辐射下的热传输过程提供了一个新的三元纳米液体模型。该模型通过实现三元流体特性和支持性变换来进行建模,然后对结果进行仿真;bvp4c 已成功编码。研究发现,较高的感应磁场(0.1-0.4)和纳米粒子数量(0.01-0.07)能更好地阻止运动,而楔形参数(λ1)则能促进运动。通过提高加热源、Eckert 和 Rd,可以观察到传热过程的快速发展,而混合对流数 α 则控制了这一过程。此外,我们还研究了特定使用的三元纳米液体,发现其具有良好的冷却效果。
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引用次数: 0
Thermal and mass stratification effects on MHD nanofluid past an exponentially accelerated vertical plate through a porous medium with thermal radiation and heat source 热辐射和热源对以指数加速度穿过多孔介质的垂直板的 MHD 纳米流体的热效应和质量分层效应
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-03 DOI: 10.1142/s0217979225500456
Rupam Shankar Nath, Rudra Kanta Deka

The aim of this research is to investigate the combined effects of thermal and mass stratification on unsteady magnetohydrodynamic nanofluid moving through an exponentially accelerated vertical plate in a porous medium. The governing equations of the problem are solved numerically by using the implicit Crank–Nicolson method. The results of the nanofluid with two different stratification are compared to those obtained without any stratification. The velocity of the nanofluid decreases with both types of stratification, whereas temperature and concentration decrease with thermal stratification and mass stratification, respectively. A variety of parameters, including the volume fraction of nanoparticles, thermal radiation, heat source/sink, and chemical reaction, can be studied using graphs. The important results demonstrate that nanofluids are more thermally conductive than normal fluids. This research holds significant implications in various fields, including power generation, electronic component cooling, and vehicle construction.

本研究旨在探讨热分层和质量分层对在多孔介质中以指数加速度通过垂直板的非稳态磁流体的综合影响。采用隐式 Crank-Nicolson 方法对问题的支配方程进行了数值求解。将两种不同分层的纳米流体与无分层纳米流体的结果进行了比较。纳米流体的速度在两种分层情况下都会降低,而温度和浓度则分别在热分层和质量分层情况下降低。利用图表可以研究各种参数,包括纳米粒子的体积分数、热辐射、热源/散热和化学反应。重要结果表明,纳米流体的导热性能比普通流体更强。这项研究在发电、电子元件冷却和汽车制造等多个领域都具有重要意义。
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引用次数: 0
Effect of three-phase-lag thermal and three-phase-lag diffusion models on waves at the boundary of elastic and thermoelastic diffusion medium 三相滞后热扩散模型和三相滞后扩散模型对弹性和热弹性扩散介质边界波的影响
IF 1.7 4区 物理与天体物理 Q2 PHYSICS, APPLIED Pub Date : 2024-04-03 DOI: 10.1142/s0217979225500250
Shruti Goel, Vandana Gupta, Manoj Kumar

In this paper, we discuss the reflection and refraction of an incident P wave or SV wave at the interface of a plane. The plane, which is divided into two halves, is an elastic medium M1 having an incident wave and a thermoelastic diffusion medium M2 with TPLT (i.e., three-phase-lag thermal) and TPLD (i.e., three-phase-lag diffusion) models. It has been noticed that two waves are reflected and four are refracted in an isotropic thermoelastic diffusion medium. Out of the four refracted waves, three are longitudinal waves: a quasi-longitudinal wave qP, a quasi-mass diffusion wave qV, a quasi-thermal wave qT and one is a transverse wave SV. If we consider the above waves first, the amplitude and energy ratio are calculated by using the surface boundary conditions and then graphically represented to compare the change in energy and amplitude ratio with the change in incident angle for three particular cases. The conservation of energy is depicted by verifying that all the energy sums up to unity. The considered problem has its application in earthquake engineering, astronautics, rocket engineering, seismology and many more engineering areas.

本文讨论入射 P 波或 SV 波在平面界面上的反射和折射。该平面分为两半,一部分是有入射波的弹性介质 M1,另一部分是热弹性扩散介质 M2,分别采用 TPLT(即三相滞后热)和 TPLD(即三相滞后扩散)模型。我们注意到,在各向同性的热弹性扩散介质中,有两个波被反射,四个波被折射。在四个折射波中,有三个是纵波:准纵波 qP、准质量扩散波 qV、准热波 qT 和一个横波 SV。如果我们首先考虑上述波,则可利用表面边界条件计算出振幅和能量比,然后用图表表示,比较三种特定情况下能量和振幅比随入射角变化而变化的情况。通过验证所有能量总和为 1,说明了能量守恒。所考虑的问题可应用于地震工程、宇航、火箭工程、地震学和其他许多工程领域。
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International Journal of Modern Physics B
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