Pub Date : 2024-05-16DOI: 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.
{"title":"Möbius group actions in the solvable chimera model","authors":"Vladimir Jaćimović, Aladin Crnkić","doi":"10.1142/s0217979225400053","DOIUrl":"https://doi.org/10.1142/s0217979225400053","url":null,"abstract":"<p>We study actions of Möbius group on two sub-populations in the solvable chimera model proposed by Abrams <i>et al.</i> 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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"18 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-05-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141169606","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}
Pub Date : 2024-05-08DOI: 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 -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 -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。
{"title":"On the solutions of space-time fractional CBS and CBS-BK equations describing the dynamics of Riemann wave interaction","authors":"A. K. Sahoo, A. K. Gupta, Aly R. Seadawy","doi":"10.1142/s0217979225400016","DOIUrl":"https://doi.org/10.1142/s0217979225400016","url":null,"abstract":"<p>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 <span><math altimg=\"eq-00001.gif\" display=\"inline\" overflow=\"scroll\"><mo stretchy=\"false\">(</mo><mn>3</mn><mo>+</mo><mn>1</mn><mo stretchy=\"false\">)</mo></math></span><span></span>-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 <span><math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"><mo stretchy=\"false\">(</mo><mn>3</mn><mo>+</mo><mn>1</mn><mo stretchy=\"false\">)</mo></math></span><span></span>-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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"34 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-05-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140926104","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}
Pub Date : 2024-04-30DOI: 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.
{"title":"Electro-fluid-dynamics (EFD) of soft-bodied organisms swimming through mucus having dilatant, viscous, and pseudo-plastic properties","authors":"Zeeshan Asghar, Rehman Ali Shah, Muhammad Waqas, Muhammad Asif Gondal","doi":"10.1142/s0217979225500110","DOIUrl":"https://doi.org/10.1142/s0217979225500110","url":null,"abstract":"<p>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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"17 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140830408","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}
Pub Date : 2024-04-30DOI: 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.
{"title":"Application of micropolar fluid model to blood flow through catheterized artery with stenosis and thrombosis","authors":"Muhammad Ashfaq, Zeeshan Asghar, Yufeng Nie, Wasfi Shatanawi","doi":"10.1142/s0217979225500481","DOIUrl":"https://doi.org/10.1142/s0217979225500481","url":null,"abstract":"<p>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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"43 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140830290","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}
Pub Date : 2024-04-17DOI: 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
{"title":"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","authors":"Shafaat Hussain Mirza, Sikander Azam, Zeesham Abbas, Shoyebmohamad F. Shaikh","doi":"10.1142/s0217979225500389","DOIUrl":"https://doi.org/10.1142/s0217979225500389","url":null,"abstract":"<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","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}
Pub Date : 2024-04-03DOI: 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.
{"title":"Novel optical solitons patterns via Biswas–Arshed equation with gain or loss. Modulated wave gain","authors":"H. I. Abdel-Gawad","doi":"10.1142/s0217979225500171","DOIUrl":"https://doi.org/10.1142/s0217979225500171","url":null,"abstract":"<p>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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"205 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140570028","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}
Pub Date : 2024-04-03DOI: 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.
{"title":"Influence of temperature on Rashba effect of bound polaron in a parabolic quantum well","authors":"Ya-Li Li, Shu-Ping Shan","doi":"10.1142/s0217979225500286","DOIUrl":"https://doi.org/10.1142/s0217979225500286","url":null,"abstract":"<p>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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"55 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140602943","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}
Pub Date : 2024-04-03DOI: 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 ( promotes it. By promoting the heating source, Eckert and , the heat transfer process is observed rapidly while the mixed convective number controls it. Further, the particular used ternary nanoliquid is examined and found to be good for cooling purposes.
{"title":"Numerical heat featuring in radiative convective ternary nanofluid under induced magnetic field and heat generating source","authors":"Adnan, Waseem Abbas, Aisha M. Alqahtani, Zafar Mahmood, Sid Ahmed Ould Beinane, Muhammad Bilal","doi":"10.1142/s0217979225500444","DOIUrl":"https://doi.org/10.1142/s0217979225500444","url":null,"abstract":"<p>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 (<span><math altimg=\"eq-00001.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>λ</mi></mrow><mrow><mn>1</mn></mrow></msub><mo stretchy=\"false\">)</mo></math></span><span></span> promotes it. By promoting the heating source, Eckert and <span><math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>R</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span><span></span>, the heat transfer process is observed rapidly while the mixed convective number <span><math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"><mi>α</mi></math></span><span></span> controls it. Further, the particular used ternary nanoliquid is examined and found to be good for cooling purposes.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"47 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140570035","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}
Pub Date : 2024-04-03DOI: 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.
{"title":"Thermal and mass stratification effects on MHD nanofluid past an exponentially accelerated vertical plate through a porous medium with thermal radiation and heat source","authors":"Rupam Shankar Nath, Rudra Kanta Deka","doi":"10.1142/s0217979225500456","DOIUrl":"https://doi.org/10.1142/s0217979225500456","url":null,"abstract":"<p>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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"92 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140569973","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}
Pub Date : 2024-04-03DOI: 10.1142/s0217979225500250
Shruti Goel, Vandana Gupta, Manoj Kumar
In this paper, we discuss the reflection and refraction of an incident P wave or wave at the interface of a plane. The plane, which is divided into two halves, is an elastic medium having an incident wave and a thermoelastic diffusion medium 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 a quasi-mass diffusion wave , a quasi-thermal wave and one is a transverse wave . 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.
{"title":"Effect of three-phase-lag thermal and three-phase-lag diffusion models on waves at the boundary of elastic and thermoelastic diffusion medium","authors":"Shruti Goel, Vandana Gupta, Manoj Kumar","doi":"10.1142/s0217979225500250","DOIUrl":"https://doi.org/10.1142/s0217979225500250","url":null,"abstract":"<p>In this paper, we discuss the reflection and refraction of an incident <i>P</i> wave or <span><math altimg=\"eq-00001.gif\" display=\"inline\" overflow=\"scroll\"><mi>S</mi><mi>V</mi></math></span><span></span> wave at the interface of a plane. The plane, which is divided into two halves, is an elastic medium <span><math altimg=\"eq-00002.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>M</mi></mrow><mrow><mn>1</mn></mrow></msub></math></span><span></span> having an incident wave and a thermoelastic diffusion medium <span><math altimg=\"eq-00003.gif\" display=\"inline\" overflow=\"scroll\"><msub><mrow><mi>M</mi></mrow><mrow><mn>2</mn></mrow></msub></math></span><span></span> 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 <span><math altimg=\"eq-00004.gif\" display=\"inline\" overflow=\"scroll\"><mi>q</mi><mi>P</mi><mo>,</mo></math></span><span></span> a quasi-mass diffusion wave <span><math altimg=\"eq-00005.gif\" display=\"inline\" overflow=\"scroll\"><mi>q</mi><mi>V</mi></math></span><span></span>, a quasi-thermal wave <span><math altimg=\"eq-00006.gif\" display=\"inline\" overflow=\"scroll\"><mi>q</mi><mi>T</mi></math></span><span></span> and one is a transverse wave <span><math altimg=\"eq-00007.gif\" display=\"inline\" overflow=\"scroll\"><mi>S</mi><mi>V</mi></math></span><span></span>. 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.</p>","PeriodicalId":14108,"journal":{"name":"International Journal of Modern Physics B","volume":"109 1","pages":""},"PeriodicalIF":1.7,"publicationDate":"2024-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140570036","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}