Pub Date : 2024-10-24DOI: 10.1007/s12043-024-02842-y
Amin A Nizami
Periodically kicked Floquet systems, such as the kicked rotor, are a paradigmatic and illustrative simple model of chaos. For non-integrable quantum dynamics, there are several diagnostic measures, such as Loschmidt echo, autocorrelation function and out of time order correlator (OTOC) to study the presence of (or the transition to) chaotic behaviour. We analytically compute these measures in terms of the eigensystem of the unitary Floquet operator of the driven quantum systems. We use these expressions to determine the time variation of the measures for the quantum-kicked rotor (QKR) on the torus, for the integrable as well as the chaotic case. For a simpler integrable variant of the kicked rotor, we also give a representation theoretic derivation of its dynamics.
{"title":"Quantum chaos measures for Floquet dynamics","authors":"Amin A Nizami","doi":"10.1007/s12043-024-02842-y","DOIUrl":"10.1007/s12043-024-02842-y","url":null,"abstract":"<div><p>Periodically kicked Floquet systems, such as the kicked rotor, are a paradigmatic and illustrative simple model of chaos. For non-integrable quantum dynamics, there are several diagnostic measures, such as Loschmidt echo, autocorrelation function and out of time order correlator (OTOC) to study the presence of (or the transition to) chaotic behaviour. We analytically compute these measures in terms of the eigensystem of the unitary Floquet operator of the driven quantum systems. We use these expressions to determine the time variation of the measures for the quantum-kicked rotor (QKR) on the torus, for the integrable as well as the chaotic case. For a simpler integrable variant of the kicked rotor, we also give a representation theoretic derivation of its dynamics.\u0000</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142518932","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 : 2024-10-24DOI: 10.1007/s12043-024-02819-x
Madhubrata Bhattacharya, Debabrata Datta
Positron emission tomography (PET) scans are vital in diagnosing cancer and neurological disorders but raise concerns due to exposure to ionising radiation. This research is focussed on the development of an intelligent regression model to investigate the effective radiation dose received by a patient during the whole-body PET scan. Our newly developed intelligent model refers to the application of artificial intelligence (AI) and machine learning (ML) techniques. Since underfitting and overfitting are basic issues of any ML model, data fitting methodology for developing intelligent regression is taken care of by implementing the least absolute shrinkage and selection operator (Lasso) and ridge regression. In order to have the comparative performance of our model, we have also applied support vector and decision tree-based ML techniques as regressors to predict radiation doses in whole-body PET scans, keeping patient safety in mind. By incorporating patient-specific data and imaging parameters, these models aim to accurately estimate radiation doses, thereby optimising imaging protocols and reducing unnecessary exposure risks. The study uses PET({/})CT data from 2009 to 2012. The linearly-independent covariates applied in this model are age, weight, height, residence time and injected activity and the dependence variable is taken as the effective dose. Model performance is evaluated using root mean square error (RMSE). A systematic exploratory data analysis has been carried out to investigate data cleaning, missing information, scaling and normalisation. The top five organs such as the brain, stomach, kidney, adrenal and spleen are focussed to produce the traditional descriptive statistics of data summary. Least absolute shrinkage and selection operator (lasso) regression exhibit stable RMSE values for organ equivalent doses across genders, while substantial RMSE variations exist among different models and organs, suggesting sensitivity to specific organs and patient gender. Accurate dose estimation is pivotal for risk assessment and protocol optimisation. This study evidenced the need to improve radiation dosimetry for specific organs aiming at patient care and radiology practices by considering individualised factors in dose estimation methodologies to refine PET scan dose estimation methods.
正电子发射断层扫描(PET)是诊断癌症和神经系统疾病的重要手段,但由于会受到电离辐射的影响,因此引起了人们的关注。这项研究的重点是开发一种智能回归模型,以调查病人在全身 PET 扫描过程中接受的有效辐射剂量。我们新开发的智能模型指的是人工智能(AI)和机器学习(ML)技术的应用。由于欠拟合和过拟合是任何 ML 模型的基本问题,因此开发智能回归的数据拟合方法采用了最小绝对收缩和选择算子(Lasso)以及脊回归。为了比较我们模型的性能,我们还应用了基于支持向量和决策树的 ML 技术作为回归因子,以预测全身 PET 扫描的辐射剂量,同时考虑到患者的安全。通过纳入患者的特定数据和成像参数,这些模型旨在准确估计辐射剂量,从而优化成像方案,减少不必要的照射风险。该研究使用了2009年至2012年的PET/({/}/)CT数据。该模型中应用的线性独立协变量包括年龄、体重、身高、停留时间和注射活动,因变量为有效剂量。模型性能采用均方根误差(RMSE)进行评估。我们进行了系统的探索性数据分析,以研究数据清理、缺失信息、缩放和归一化等问题。重点对脑、胃、肾、肾上腺和脾脏等前五大器官进行了数据汇总的传统描述性统计。最小绝对收缩和选择算子(lasso)回归对不同性别的器官等效剂量显示出稳定的 RMSE 值,而不同模型和器官之间存在巨大的 RMSE 差异,这表明对特定器官和患者性别的敏感性。准确的剂量估算对于风险评估和方案优化至关重要。这项研究证明,有必要通过考虑剂量估算方法中的个体化因素来改进 PET 扫描剂量估算方法,从而改善特定器官的辐射剂量估算,以达到患者护理和放射学实践的目的。
{"title":"Development of an intelligent linear regression model for dose estimation to patients during whole-body PET scan","authors":"Madhubrata Bhattacharya, Debabrata Datta","doi":"10.1007/s12043-024-02819-x","DOIUrl":"10.1007/s12043-024-02819-x","url":null,"abstract":"<div><p>Positron emission tomography (PET) scans are vital in diagnosing cancer and neurological disorders but raise concerns due to exposure to ionising radiation. This research is focussed on the development of an intelligent regression model to investigate the effective radiation dose received by a patient during the whole-body PET scan. Our newly developed intelligent model refers to the application of artificial intelligence (AI) and machine learning (ML) techniques. Since underfitting and overfitting are basic issues of any ML model, data fitting methodology for developing intelligent regression is taken care of by implementing the least absolute shrinkage and selection operator (Lasso) and ridge regression. In order to have the comparative performance of our model, we have also applied support vector and decision tree-based ML techniques as regressors to predict radiation doses in whole-body PET scans, keeping patient safety in mind. By incorporating patient-specific data and imaging parameters, these models aim to accurately estimate radiation doses, thereby optimising imaging protocols and reducing unnecessary exposure risks. The study uses PET<span>({/})</span>CT data from 2009 to 2012. The linearly-independent covariates applied in this model are age, weight, height, residence time and injected activity and the dependence variable is taken as the effective dose. Model performance is evaluated using root mean square error (RMSE). A systematic exploratory data analysis has been carried out to investigate data cleaning, missing information, scaling and normalisation. The top five organs such as the brain, stomach, kidney, adrenal and spleen are focussed to produce the traditional descriptive statistics of data summary. Least absolute shrinkage and selection operator (lasso) regression exhibit stable RMSE values for organ equivalent doses across genders, while substantial RMSE variations exist among different models and organs, suggesting sensitivity to specific organs and patient gender. Accurate dose estimation is pivotal for risk assessment and protocol optimisation. This study evidenced the need to improve radiation dosimetry for specific organs aiming at patient care and radiology practices by considering individualised factors in dose estimation methodologies to refine PET scan dose estimation methods.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142518928","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 : 2024-10-15DOI: 10.1007/s12043-024-02804-4
Shahid Rafiq, Muhammad Asim, Muhammad Mustahsan, M Ijaz Khan
This article uses a finite-element approximation approach for solving a three-dimensional flow problem of a nanofluid influenced by heat transfer due to nanoparticles over a non-linearly stretching sheet within an unbounded domain. Utilising similarity transformations, a well-posed coupled system of nonlinear ordinary differential equations is derived from the governing partial differential equations describing the flow and heat transfer processes. The resulting system is then solved by using quadratic Lagrange polynomials as basic functions over a mesh of different finite elements through the Galerkin finite element (GFE) technique. This implementation is based on a regular grid utilising Lagrange polynomials for solving the converted equations. The effects of various parameters of interest are efficiently discussed with the help of graphs and numeric tables. Both numerical and exact solutions are compared favourably, demonstrating a high level of accuracy. It is noteworthy that the GFE method emerges as a much more stable numerical technique than the other existing analytic and semi-analytical methods. Furthermore, the adopted finite-element method reduces the dimensionality of Sobolev's space's finite-dimensional subspace and also improves the solution's convergence rate. Moreover, the velocity is negative, and its magnitude increases as the stretching rates ratio increases due to the downward flow in the vertical direction. The temperature and heat transmission from the sheet are barely impacted by Brownian motion due to the dominance of other forces and length scales involved in the heat transfer process.
{"title":"Finite-element approximation for three-dimensional nanofluid flow with heat transfer over a non-linearly stretching sheet","authors":"Shahid Rafiq, Muhammad Asim, Muhammad Mustahsan, M Ijaz Khan","doi":"10.1007/s12043-024-02804-4","DOIUrl":"10.1007/s12043-024-02804-4","url":null,"abstract":"<div><p>This article uses a finite-element approximation approach for solving a three-dimensional flow problem of a nanofluid influenced by heat transfer due to nanoparticles over a non-linearly stretching sheet within an unbounded domain. Utilising similarity transformations, a well-posed coupled system of nonlinear ordinary differential equations is derived from the governing partial differential equations describing the flow and heat transfer processes. The resulting system is then solved by using quadratic Lagrange polynomials as basic functions over a mesh of different finite elements through the Galerkin finite element (GFE) technique. This implementation is based on a regular grid utilising Lagrange polynomials for solving the converted equations. The effects of various parameters of interest are efficiently discussed with the help of graphs and numeric tables. Both numerical and exact solutions are compared favourably, demonstrating a high level of accuracy. It is noteworthy that the GFE method emerges as a much more stable numerical technique than the other existing analytic and semi-analytical methods. Furthermore, the adopted finite-element method reduces the dimensionality of Sobolev's space's finite-dimensional subspace and also improves the solution's convergence rate. Moreover, the velocity is negative, and its magnitude increases as the stretching rates ratio increases due to the downward flow in the vertical direction. The temperature and heat transmission from the sheet are barely impacted by Brownian motion due to the dominance of other forces and length scales involved in the heat transfer process.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142438783","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 : 2024-10-15DOI: 10.1007/s12043-024-02827-x
Nirmoy Kumar Das, Dhanashri Barman, Ashoke Das, Towhid E Aman
A new generalised non-local nonlinear Schrödinger (NLS) equation is introduced which possesses a Lax pair and is parity–time (PT)-symmetric. Thus, it is confirmed that the generalised non-local NLS equation is integrable. The inverse scattering transform for the generalised non-local NLS equation is developed using a Riemann–Hilbert problem for rapidly decaying initial data and an approach for finding pure soliton solutions is described. The analytical characteristics of the eigenfunctions, scattering data and their symmetries are discussed. Finally, using Mathematica some important two-dimensional plots of the wave solutions are shown to illustrate the dynamics of the model.
{"title":"PT-invariant generalised non-local nonlinear Schrödinger equation: soliton solutions","authors":"Nirmoy Kumar Das, Dhanashri Barman, Ashoke Das, Towhid E Aman","doi":"10.1007/s12043-024-02827-x","DOIUrl":"10.1007/s12043-024-02827-x","url":null,"abstract":"<div><p>A new generalised non-local nonlinear Schrödinger (NLS) equation is introduced which possesses a Lax pair and is parity–time (<i>PT</i>)-symmetric. Thus, it is confirmed that the generalised non-local NLS equation is integrable. The inverse scattering transform for the generalised non-local NLS equation is developed using a Riemann–Hilbert problem for rapidly decaying initial data and an approach for finding pure soliton solutions is described. The analytical characteristics of the eigenfunctions, scattering data and their symmetries are discussed. Finally, using <i>Mathematica</i> some important two-dimensional plots of the wave solutions are shown to illustrate the dynamics of the model.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142438784","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 : 2024-10-10DOI: 10.1007/s12043-024-02839-7
Van Hong Nguyen, Hoang Anh Nguyen
In this study, we employ molecular dynamics simulations to develop a large model (19,998 atoms) of liquid SiO2 at 3500 K. We construct models at different pressures in the 0–100 GPa range using the Beest–Kramer–Santen (BKS) potential and periodic boundary conditions. The goal is to detail the structural transition from the polyamorphic liquid state of SiO2 to the crystalline stishovite form, which occurs between 45 and 60 GPa. We analyse the polyamorphic state of liquid SiO2 by examining the formation of SiOx clusters from 2 to 60 GPa. Beyond 60 GPa, the pair radial distribution functions (PRDFs) for Si–O, O–O and Si–Si display multiple peaks, indicating the crystalline phase. This observation is further supported by examining the bond angle distribution, the fraction of SiOx units and OSix linkages, Si–O bond lengths within SiOx units, structural visualisations and the analysis of ring statistics in the liquid SiO2 system, all of which underscore the comprehensive changes in the structure of the system.
{"title":"Crystallisation of liquid silica under compression: a molecular dynamics simulation","authors":"Van Hong Nguyen, Hoang Anh Nguyen","doi":"10.1007/s12043-024-02839-7","DOIUrl":"10.1007/s12043-024-02839-7","url":null,"abstract":"<div><p>In this study, we employ molecular dynamics simulations to develop a large model (19,998 atoms) of liquid SiO<sub>2</sub> at 3500 K. We construct models at different pressures in the 0–100 GPa range using the Beest–Kramer–Santen (BKS) potential and periodic boundary conditions. The goal is to detail the structural transition from the polyamorphic liquid state of SiO<sub>2</sub> to the crystalline stishovite form, which occurs between 45 and 60 GPa. We analyse the polyamorphic state of liquid SiO<sub>2</sub> by examining the formation of SiO<sub><i>x</i></sub> clusters from 2 to 60 GPa. Beyond 60 GPa, the pair radial distribution functions (PRDFs) for Si–O, O–O and Si–Si display multiple peaks, indicating the crystalline phase. This observation is further supported by examining the bond angle distribution, the fraction of SiO<sub><i>x</i></sub> units and OSi<sub><i>x</i></sub> linkages, Si–O bond lengths within SiO<sub><i>x</i></sub> units, structural visualisations and the analysis of ring statistics in the liquid SiO<sub>2</sub> system, all of which underscore the comprehensive changes in the structure of the system.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142411205","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 : 2024-10-10DOI: 10.1007/s12043-024-02835-x
S Diana Emerald Aasha, Shanthi Prince
The performance of multilayer organic light emitting diode (OLED) is studied by stacking poly(3,4-ethylenedioxythiophene) polystyrene sulphonate (PEDOT:PSS) as the hole transport layer (HTL), tris(4-carbazoyl-9-ylphenyl) amine (TCTA) as the hole injection layer (HIL) and bathophenanthroline (BPhen) as the electron transport layer (ETL). Modification is done in the emissive layer (EML) by the introduction of host–guest material which is bis[2-(4,6-difluorophenyl) pyridinato-C2,N](picolinato)iridium(III) (FlrPic) and bis[2-(diphenylphosphino) phenyl] ether oxide (DPEPO). Multiple devices are fabricated and the performance is compared in terms of turn-on voltage, current density, brightness and luminous efficiency. The device with co-deposition of guest and host materials has improved the luminous efficiency by 6.17% when compared to the other fabricated devices.
{"title":"Maximising OLED performance: Unleashing the power of stacking transport, injection and blocking layers along with different emissive materials","authors":"S Diana Emerald Aasha, Shanthi Prince","doi":"10.1007/s12043-024-02835-x","DOIUrl":"10.1007/s12043-024-02835-x","url":null,"abstract":"<div><p>The performance of multilayer organic light emitting diode (OLED) is studied by stacking poly(3,4-ethylenedioxythiophene) polystyrene sulphonate (PEDOT:PSS) as the hole transport layer (HTL), tris(4-carbazoyl-9-ylphenyl) amine (TCTA) as the hole injection layer (HIL) and bathophenanthroline (BPhen) as the electron transport layer (ETL). Modification is done in the emissive layer (EML) by the introduction of host–guest material which is bis[2-(4,6-difluorophenyl) pyridinato-C2,N](picolinato)iridium(III) (FlrPic) and bis[2-(diphenylphosphino) phenyl] ether oxide (DPEPO). Multiple devices are fabricated and the performance is compared in terms of turn-on voltage, current density, brightness and luminous efficiency. The device with co-deposition of guest and host materials has improved the luminous efficiency by 6.17% when compared to the other fabricated devices.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142411166","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 : 2024-10-10DOI: 10.1007/s12043-024-02829-9
Abir Baidya, Swati Mukhopadhyay, G C Layek
It is obvious that due to its higher viscosity, non-Newtonian fluid show better heat transport than the Newtonian fluid. Moreover, shear flow helps us to make our surrounding environment friendly. With this view point, an attempt has been taken in this paper to explore the two-dimensional flow of low electrically conducting Eyring–Prandtl fluid and heat transfer over a moving porous plate subject to suction/blowing with externally applied magnetic field. The flow is maintained due to the incoming shear away from the plate so that boundary layer type of flow is formed over the plate. This makes the problem new, not yet been addressed by any researcher. Similarity transformations are applied to obtain self-similar structure of the leading equations. However, similar solutions of the problem are attained for a specific power-law velocity (index, (n=1/3)) of the moving plate. The equations are solved numerically and compared with different flow quantities having different grid sizes. The data are plotted graphically to represent velocity, velocity gradient and temperature for different parametric values. The influences of suction/blowing parameter, fluid material parameters, Prandtl number and magnetic parameter on velocity, temperature and velocity gradient are shown and explained at length with physical explanations as far as practicable. The velocity decreases with increasing values of magnetic parameter due to the appearance of Lorenz force. However, temperature increases. So, the boundary layer flow can be controlled using a suitable magnetic field. It is found that fluid velocity rises with the growing suction/blowing parameter and fluid material parameter (alpha ) but the temperature is found to diminish resulting in the reduction of heat transfer in fluid. The analysis reveals that blowing destabilises the flow, while the suction stabilises the boundary layer flow. This study explores the boundary layer flow structure of a fluid with low electrical conductivity along with heat transfer in the presence of suction/blowing, externally applied magnetic field and shear flow.
{"title":"Heat transfer of MHD Eyring–Prandtl fluid flow past a moving permeable plate with shear flow","authors":"Abir Baidya, Swati Mukhopadhyay, G C Layek","doi":"10.1007/s12043-024-02829-9","DOIUrl":"10.1007/s12043-024-02829-9","url":null,"abstract":"<div><p>It is obvious that due to its higher viscosity, non-Newtonian fluid show better heat transport than the Newtonian fluid. Moreover, shear flow helps us to make our surrounding environment friendly. With this view point, an attempt has been taken in this paper to explore the two-dimensional flow of low electrically conducting Eyring–Prandtl fluid and heat transfer over a moving porous plate subject to suction/blowing with externally applied magnetic field. The flow is maintained due to the incoming shear away from the plate so that boundary layer type of flow is formed over the plate. This makes the problem new, not yet been addressed by any researcher. Similarity transformations are applied to obtain self-similar structure of the leading equations. However, similar solutions of the problem are attained for a specific power-law velocity (index, <span>(n=1/3)</span>) of the moving plate. The equations are solved numerically and compared with different flow quantities having different grid sizes. The data are plotted graphically to represent velocity, velocity gradient and temperature for different parametric values. The influences of suction/blowing parameter, fluid material parameters, Prandtl number and magnetic parameter on velocity, temperature and velocity gradient are shown and explained at length with physical explanations as far as practicable. The velocity decreases with increasing values of magnetic parameter due to the appearance of Lorenz force. However, temperature increases. So, the boundary layer flow can be controlled using a suitable magnetic field. It is found that fluid velocity rises with the growing suction/blowing parameter and fluid material parameter <span>(alpha )</span> but the temperature is found to diminish resulting in the reduction of heat transfer in fluid. The analysis reveals that blowing destabilises the flow, while the suction stabilises the boundary layer flow. This study explores the boundary layer flow structure of a fluid with low electrical conductivity along with heat transfer in the presence of suction/blowing, externally applied magnetic field and shear flow.\u0000</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142411167","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 : 2024-10-05DOI: 10.1007/s12043-024-02824-0
T Koohrokhi, A Izadpanah, M Gerayloo
Most physical systems, whether classical or quantum mechanical, exhibit spherical symmetry. Angular momentum, denoted as (ell ), is a conserved quantity that appears in the centrifugal potential when a particle moves under the influence of a central force. This study introduces a formalism in which (ell ) plays a unifying role, consolidating solvable central potentials into a superpotential. This framework illustrates that the Coulomb potential emerges as a direct consequence of a homogeneous (r-independent) isotropic superpotential. Conversely, an (ell )-independent central superpotential results in a 3-dimensional harmonic oscillator (3-DHO) potential. Moreover, a local (ell )-dependent central superpotential generates potentials applicable to finite-range interactions such as molecular or nucleonic systems. Additionally, we discuss generalisations to arbitrary D dimensions and investigate the properties of the superpotential to determine when supersymmetry is broken or unbroken. This scheme also shows that the free-particle wave function in three dimensions is obtained from the spontaneous breakdown of supersymmetry and clarifies how a positive 3-DHO potential, as an upside-down potential, can have a negative energy spectrum. We also present complex isospectral deformations of the central superpotential and superpartners, which can have interesting applications for open systems in dynamic equilibrium. Finally, as a practical application, we apply this formalism to specify a new effective potential for the deuteron.
{"title":"A unified scheme of central symmetric shape-invariant potentials","authors":"T Koohrokhi, A Izadpanah, M Gerayloo","doi":"10.1007/s12043-024-02824-0","DOIUrl":"10.1007/s12043-024-02824-0","url":null,"abstract":"<div><p>Most physical systems, whether classical or quantum mechanical, exhibit spherical symmetry. Angular momentum, denoted as <span>(ell )</span>, is a conserved quantity that appears in the centrifugal potential when a particle moves under the influence of a central force. This study introduces a formalism in which <span>(ell )</span> plays a unifying role, consolidating solvable central potentials into a superpotential. This framework illustrates that the Coulomb potential emerges as a direct consequence of a homogeneous (<i>r</i>-independent) isotropic superpotential. Conversely, an <span>(ell )</span>-independent central superpotential results in a 3-dimensional harmonic oscillator (3-DHO) potential. Moreover, a local <span>(ell )</span>-dependent central superpotential generates potentials applicable to finite-range interactions such as molecular or nucleonic systems. Additionally, we discuss generalisations to arbitrary <i>D</i> dimensions and investigate the properties of the superpotential to determine when supersymmetry is broken or unbroken. This scheme also shows that the free-particle wave function in three dimensions is obtained from the spontaneous breakdown of supersymmetry and clarifies how a positive 3-DHO potential, as an upside-down potential, can have a negative energy spectrum. We also present complex isospectral deformations of the central superpotential and superpartners, which can have interesting applications for open systems in dynamic equilibrium. Finally, as a practical application, we apply this formalism to specify a new effective potential for the deuteron.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142410084","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 : 2024-09-28DOI: 10.1007/s12043-024-02811-5
Sourav Chaudhary, S K Maurya, Jitendra Kumar, Sweeti Kiroriwal
In this work, we have obtained new phantom fluid-type traversable wormhole (WH) solutions in the context of (f(mathcal {R}, T)) modified gravity. We investigate the potential that some equations of state (EoS), specifically phantom energy, which describes the accelerated expansion of the universe, could support the existence of traversable wormholes. This cosmic fluid thus offers us a plausible explanation for the occurrence of WH geometries. We construct two WH models with matter Lagrangian density (mathcal {L}_{m}=-(-rho +mathcal {P}_{r}+2mathcal {P}_{t})) and inspect numerous characteristics of these models under the WH geometry. The first WH solution (WH-I) is discovered by utilising a linear barotropic equation of state (EoS) connected with phantom energy (omega <-1) indicating the presence of the phantom fluid and pointing to the Universe’s expansion, while in the second WH (WH-II) solution, we take into account an interesting EoS (rho =eta (mathcal {P}_{t}-mathcal {P}_{r})) to generate a WH model. Additionally, it showed that the phantom fluid WH-I solution violates the radial null energy condition (NEC) while tangential NEC is satisfied. On the other hand, for the WH-II solution, NEC is violated. Extensive detailed discussions of the matter components have been done via graphical analysis. The obtained WH geometries satisfy a stable WH’s physically acceptable criteria.
{"title":"Traversable wormhole solutions with phantom fluid in modified f(R, T) gravity","authors":"Sourav Chaudhary, S K Maurya, Jitendra Kumar, Sweeti Kiroriwal","doi":"10.1007/s12043-024-02811-5","DOIUrl":"10.1007/s12043-024-02811-5","url":null,"abstract":"<div><p>In this work, we have obtained new phantom fluid-type traversable wormhole (WH) solutions in the context of <span>(f(mathcal {R}, T))</span> modified gravity. We investigate the potential that some equations of state (EoS), specifically phantom energy, which describes the accelerated expansion of the universe, could support the existence of traversable wormholes. This cosmic fluid thus offers us a plausible explanation for the occurrence of WH geometries. We construct two WH models with matter Lagrangian density <span>(mathcal {L}_{m}=-(-rho +mathcal {P}_{r}+2mathcal {P}_{t}))</span> and inspect numerous characteristics of these models under the WH geometry. The first WH solution (WH-I) is discovered by utilising a linear barotropic equation of state (EoS) connected with phantom energy <span>(omega <-1)</span> indicating the presence of the phantom fluid and pointing to the Universe’s expansion, while in the second WH (WH-II) solution, we take into account an interesting EoS <span>(rho =eta (mathcal {P}_{t}-mathcal {P}_{r}))</span> to generate a WH model. Additionally, it showed that the phantom fluid WH-I solution violates the radial null energy condition (NEC) while tangential NEC is satisfied. On the other hand, for the WH-II solution, NEC is violated. Extensive detailed discussions of the matter components have been done via graphical analysis. The obtained WH geometries satisfy a stable WH’s physically acceptable criteria.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142414739","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}
The dynamical probing and linear offset boosting of constants in Josephson junction (JJ) instigated by the Wien bridge oscillator (JJIWBO) are investigated in this paper. Via numerical simulations, the JJIWBO unveiled bistable periodic oscillations, bistable periodic doubling with an evolving path to bistable chaotic characteristics, monostable chaotic behaviours and monostable periodic characteristics. The numerical dynamics are realised by the microcontroller validation (MCV) scheme. Two constant parameters are introduced in the rate equations of JJIWBO to implement the linear offset boosting of constants based on the two voltage variables. It is demonstrated that the polarity of the chaotic voltage and phase difference signals can be flexibly changed by varying one of the two constant parameters which is different from zero and the other constant parameter is zero. When two constant parameters have the same value, the chaotic voltages and phase difference signals can switch between bipolar and unipolar signals flexibly by changing the unique constant parameter.
{"title":"Dynamical probing and multiple actions of linear offset boosting of constants in Josephson junction instigated by Wien bridge oscillator embedded in the microcontroller","authors":"Balakrishnan Sriram, Daniel Maoussi Godonou, Cyrille Ainamon, Isidore Komofor Ngongiah, Karthikeyan Rajagopal","doi":"10.1007/s12043-024-02816-0","DOIUrl":"10.1007/s12043-024-02816-0","url":null,"abstract":"<div><p>The dynamical probing and linear offset boosting of constants in Josephson junction (JJ) instigated by the Wien bridge oscillator (JJIWBO) are investigated in this paper. Via numerical simulations, the JJIWBO unveiled bistable periodic oscillations, bistable periodic doubling with an evolving path to bistable chaotic characteristics, monostable chaotic behaviours and monostable periodic characteristics. The numerical dynamics are realised by the microcontroller validation (MCV) scheme. Two constant parameters are introduced in the rate equations of JJIWBO to implement the linear offset boosting of constants based on the two voltage variables. It is demonstrated that the polarity of the chaotic voltage and phase difference signals can be flexibly changed by varying one of the two constant parameters which is different from zero and the other constant parameter is zero. When two constant parameters have the same value, the chaotic voltages and phase difference signals can switch between bipolar and unipolar signals flexibly by changing the unique constant parameter.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"98 4","pages":""},"PeriodicalIF":1.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142414802","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}