Pub Date : 2025-11-22DOI: 10.1140/epjd/s10053-025-01077-9
Riccardo Fantoni
We propose a new quantum simulation method for a many-body quantum liquid of identical particles at finite (nonzero) temperature. The new scheme expands the high-temperature density matrix on the overcomplete set of single particles coherent states of John Rider Klauder instead of the usual plane waves as in conventional path integral methods. One is free to tune the elastic constant and/or the mass of the harmonic oscillator subtending the coherent states so as to maximize the computational efficiency of the algorithm. We prove that in the limit of an extremely stiff harmonic oscillator the results for the internal energy tend toward the correct expected values. Moreover, we suggest that a stiff harmonic oscillator could allow the use of larger (imaginary) timesteps. This additional degree of freedom is the characteristic feature of our new algorithm and is not available in more conventional path integral methods.
{"title":"Coherent state path integral Monte Carlo","authors":"Riccardo Fantoni","doi":"10.1140/epjd/s10053-025-01077-9","DOIUrl":"10.1140/epjd/s10053-025-01077-9","url":null,"abstract":"<p>We propose a new quantum simulation method for a many-body quantum liquid of identical particles at finite (nonzero) temperature. The new scheme expands the high-temperature density matrix on the overcomplete set of single particles coherent states of John Rider Klauder instead of the usual plane waves as in conventional path integral methods. One is free to tune the elastic constant and/or the mass of the harmonic oscillator subtending the coherent states so as to maximize the computational efficiency of the algorithm. We prove that in the limit of an extremely stiff harmonic oscillator the results for the internal energy tend toward the correct expected values. Moreover, we suggest that a stiff harmonic oscillator could allow the use of larger (imaginary) timesteps. This additional degree of freedom is the characteristic feature of our new algorithm and is not available in more conventional path integral methods.</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145612714","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 : 2025-11-22DOI: 10.1140/epjd/s10053-025-01093-9
T. V. Koshlan, K. G. Kulikov
In this work, we present a comprehensive quantum-mechanical analysis of the spectral properties of the titanium atom, with emphasis on semi-forbidden (intercombination) electronic transitions. The calculations are performed within density-functional theory (DFT) including spin–orbit coupling, and the Kohn–Sham equations are solved numerically by a conjugate-gradient method, yielding high accuracy at moderate computational cost. Oscillator strengths and transition characteristics are obtained within time-dependent DFT using the Casida formalism, which enables a consistent treatment of correlation effects and multiplet structure. Particular attention is paid to the mechanisms of population inversion and to comparisons between theory and experiment. The results validate the proposed approach and demonstrate its potential for applications to complex atomic systems in astrophysics, materials science, and quantum optics.
Four-level system: optical pumping, laser emission, collisions, and spontaneous decays
{"title":"Quantum-mechanical analysis of semi-forbidden transitions and lasing in the titanium atom","authors":"T. V. Koshlan, K. G. Kulikov","doi":"10.1140/epjd/s10053-025-01093-9","DOIUrl":"10.1140/epjd/s10053-025-01093-9","url":null,"abstract":"<p>In this work, we present a comprehensive quantum-mechanical analysis of the spectral properties of the titanium atom, with emphasis on semi-forbidden (intercombination) electronic transitions. The calculations are performed within density-functional theory (DFT) including spin–orbit coupling, and the Kohn–Sham equations are solved numerically by a conjugate-gradient method, yielding high accuracy at moderate computational cost. Oscillator strengths and transition characteristics are obtained within time-dependent DFT using the Casida formalism, which enables a consistent treatment of correlation effects and multiplet structure. Particular attention is paid to the mechanisms of population inversion and to comparisons between theory and experiment. The results validate the proposed approach and demonstrate its potential for applications to complex atomic systems in astrophysics, materials science, and quantum optics.</p><p>Four-level system: optical pumping, laser emission, collisions, and spontaneous decays</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145612681","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 : 2025-11-17DOI: 10.1140/epjd/s10053-025-01092-w
Vipul Badhan, Bindiya Arora
The choice of basis functions plays a vital role in performing accurate calculations of atomic properties. An alternative to the commonly used Gaussian-type orbitals (GTOs) is the use of B-spline functions, which offer a highly flexible and efficient basis for representing atomic wave functions. The accuracy of an atomic property depends on the quality of the chosen basis functions used to construct single-particle wave functions. This work aims at revisiting the behavior of GTOs and B-spline functions to use them optimally in different atomic calculations so that it can help reduce computational cost. In this context, we analyze the magnetic-dipole hyperfine constants ((A_{fs})) for a number of atomic states in (^{133})Cs. We first analyze results obtained using GTOs and B-splines, which are often used in the literature, followed by redefining them to improve efficiency in the calculation of atomic properties. Our comparative study reveals that an adaptive distribution of GTOs delivers the best results for low- and intermediate-lying states, whereas a kinetically balanced B-spline basis becomes more reliable for high-lying states, especially when a large number of basis functions are employed.
Efficient basis choice improves accuracy and reduces computational cost in atomic property calculations
{"title":"Reassessing Gaussian-type orbital and B-spline basis functions for accurate calculations of atomic properties: application to (^{133})Cs","authors":"Vipul Badhan, Bindiya Arora","doi":"10.1140/epjd/s10053-025-01092-w","DOIUrl":"10.1140/epjd/s10053-025-01092-w","url":null,"abstract":"<p>The choice of basis functions plays a vital role in performing accurate calculations of atomic properties. An alternative to the commonly used Gaussian-type orbitals (GTOs) is the use of B-spline functions, which offer a highly flexible and efficient basis for representing atomic wave functions. The accuracy of an atomic property depends on the quality of the chosen basis functions used to construct single-particle wave functions. This work aims at revisiting the behavior of GTOs and B-spline functions to use them optimally in different atomic calculations so that it can help reduce computational cost. In this context, we analyze the magnetic-dipole hyperfine constants (<span>(A_{fs})</span>) for a number of atomic states in <span>(^{133})</span>Cs. We first analyze results obtained using GTOs and B-splines, which are often used in the literature, followed by redefining them to improve efficiency in the calculation of atomic properties. Our comparative study reveals that an adaptive distribution of GTOs delivers the best results for low- and intermediate-lying states, whereas a kinetically balanced B-spline basis becomes more reliable for high-lying states, especially when a large number of basis functions are employed.</p><p>Efficient basis choice improves accuracy and reduces computational cost in atomic property calculations</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145560916","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 : 2025-11-10DOI: 10.1140/epjd/s10053-025-01086-8
Michael E. N. Tschaffon, Matthias Freyberger
We investigate whether negative values of Wigner functions purely coming from correlations are sufficient for observing nonlocal correlations. We employ a simple model for superpositions of coherent states and examine how the corresponding Wigner negativity of correlations relates to the violation of a CHSH inequality based on pseudo-spins. We find that a critical amount of this negativity is necessary to violate the inequality, making a nonzero negativity not sufficient for observing nonlocal correlations.
{"title":"Wigner negativity and nonlocal correlations","authors":"Michael E. N. Tschaffon, Matthias Freyberger","doi":"10.1140/epjd/s10053-025-01086-8","DOIUrl":"10.1140/epjd/s10053-025-01086-8","url":null,"abstract":"<p>We investigate whether negative values of Wigner functions purely coming from correlations are sufficient for observing nonlocal correlations. We employ a simple model for superpositions of coherent states and examine how the corresponding Wigner negativity of correlations relates to the violation of a CHSH inequality based on pseudo-spins. We find that a critical amount of this negativity is necessary to violate the inequality, making a nonzero negativity not sufficient for observing nonlocal correlations.</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjd/s10053-025-01086-8.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145510616","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-11-09DOI: 10.1140/epjd/s10053-025-01084-w
Leila Rajaei, Effat Golpar-Raboky
The Rayleigh–Taylor instability appears at the boundary between fluids of different densities, especially when the denser fluid is subjected to acceleration by the less dense fluid. An important aspect of this phenomenon is the investigation of the stability conditions governing such systems. Several parameters, including the density difference between the two fluids, the length scale of the density inhomogeneity, the initial velocity difference between the two fluids, magnetic fields, viscosity, and collision rate, can significantly affect the stability or instability of the system. To date, several of these factors have been investigated in classical and quantum physics. This phenomenon has been analyzed in both its linear and nonlinear forms. This study considers a collisional magnetic inhomogeneous quantum plasma if the two fluids have inhomogeneous initial velocities. For the velocity inhomogeneity profile modeled in two cases, a linear profile, and a parabolic profile, we have obtained the second ordinary differential equation related to the turbulent velocity. Since the differential equation has no analytical solution, we have used numerical methods to calculate the growth rate curve and obtain the turbulent velocity characteristics in the discontinuity. Then, we investigate the effect of various parameters, such as collision interactions, magnetic fields, quantum effects, and density differences between the two fluids, on the stabilization of the system. In addition, we additionally try to investigate the effect of the two initial fluid velocity profiles on the stabilization of this discontinuity.
{"title":"The effect of velocity inhomogeneity on the Rayleigh–Taylor instability in quantum plasma","authors":"Leila Rajaei, Effat Golpar-Raboky","doi":"10.1140/epjd/s10053-025-01084-w","DOIUrl":"10.1140/epjd/s10053-025-01084-w","url":null,"abstract":"<div><p>The Rayleigh–Taylor instability appears at the boundary between fluids of different densities, especially when the denser fluid is subjected to acceleration by the less dense fluid. An important aspect of this phenomenon is the investigation of the stability conditions governing such systems. Several parameters, including the density difference between the two fluids, the length scale of the density inhomogeneity, the initial velocity difference between the two fluids, magnetic fields, viscosity, and collision rate, can significantly affect the stability or instability of the system. To date, several of these factors have been investigated in classical and quantum physics. This phenomenon has been analyzed in both its linear and nonlinear forms. This study considers a collisional magnetic inhomogeneous quantum plasma if the two fluids have inhomogeneous initial velocities. For the velocity inhomogeneity profile modeled in two cases, a linear profile, and a parabolic profile, we have obtained the second ordinary differential equation related to the turbulent velocity. Since the differential equation has no analytical solution, we have used numerical methods to calculate the growth rate curve and obtain the turbulent velocity characteristics in the discontinuity. Then, we investigate the effect of various parameters, such as collision interactions, magnetic fields, quantum effects, and density differences between the two fluids, on the stabilization of the system. In addition, we additionally try to investigate the effect of the two initial fluid velocity profiles on the stabilization of this discontinuity.</p><h3>Graphical abstract</h3><div><figure><div><div><picture><source><img></source></picture></div></div></figure></div></div>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145510805","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}
Considering a combined Kappa–Cairns electron distribution, we have analytically explored the nonlinear dynamics of ion-acoustic solitary waves in a magnetized electron–ion–dusty plasma, encompassing both suprathermal and nonthermal aspects to provide a more realistic characterization. The Korteweg–de Vries–Zakharov–Kuznetsov (KdV–ZK) equation is developed by employing the reductive perturbation approach. The nonlinear coefficient of KdV–ZK equation disappears for certain parametric curves, resulting in modified KdV–ZK equation. The soliton solutions are derived for each case and the consequences of key physical parameters on soliton characteristics are numerically investigated. The small-k perturbation expansion approach is used to investigate the stability of solitary solutions. The numerical research on the impacts of the parameters associated with this system on the growth rate of instability predicts that the enhancements of the propagation angle and the ion gyro-frequency lead to the shrinkage of the maximum growth rate of instability. On the other hand, the enhancements of the suprathermal and nonthermal parameters associated with electron’s distribution lead to the shrinkage of the maximum growth rate of instability. Understanding wave propagation and stability in space and astrophysical dusty plasmas, such as the solar wind, magnetosheath, and wider heliospheric regions, may be improved by the present research.
{"title":"Ion-acoustic waves and stability analysis in magnetized dusty plasma with combined Kappa–Cairns-distributed electrons","authors":"Rittika Pain, Sandip Dalui, Sankirtan Sardar, Anup Bandyopadhyay","doi":"10.1140/epjd/s10053-025-01088-6","DOIUrl":"10.1140/epjd/s10053-025-01088-6","url":null,"abstract":"<p>Considering a combined Kappa–Cairns electron distribution, we have analytically explored the nonlinear dynamics of ion-acoustic solitary waves in a magnetized electron–ion–dusty plasma, encompassing both suprathermal and nonthermal aspects to provide a more realistic characterization. The Korteweg–de Vries–Zakharov–Kuznetsov (KdV–ZK) equation is developed by employing the reductive perturbation approach. The nonlinear coefficient of KdV–ZK equation disappears for certain parametric curves, resulting in modified KdV–ZK equation. The soliton solutions are derived for each case and the consequences of key physical parameters on soliton characteristics are numerically investigated. The small-<i>k</i> perturbation expansion approach is used to investigate the stability of solitary solutions. The numerical research on the impacts of the parameters associated with this system on the growth rate of instability predicts that the enhancements of the propagation angle and the ion gyro-frequency lead to the shrinkage of the maximum growth rate of instability. On the other hand, the enhancements of the suprathermal and nonthermal parameters associated with electron’s distribution lead to the shrinkage of the maximum growth rate of instability. Understanding wave propagation and stability in space and astrophysical dusty plasmas, such as the solar wind, magnetosheath, and wider heliospheric regions, may be improved by the present research.</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145456867","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}
Topological photonic crystals are innovative optical structures that leverage topological phases to achieve robust photonic bandgaps, exhibiting immunity to structural imperfections and disorder. However, a significant challenge in conventional topological photonic crystal designs has been the difficulty in precisely controlling the position of the transmission peak. To address this limitation, we present a modified topological photonic crystal composed of alternating (hbox {SiO}_2) and (hbox {TiO}_2) layers. This design incorporates a synergistic approach that integrates the transfer matrix method, quarter-wavelength thickness design principles, and iterative optimization of layer parameters to ensure precise wavelength alignment and enhanced spectral control. The proposed modified topological photonic crystal demonstrates superior performance, including wider photonic bandgaps, moderate transmission efficiency, and improved resistance to structural defects.
Top panel: Schematic diagrams of the proposed structure without modification (top) and with modification (bottom), together with the transmission spectra for the symmetric (red) and topological (blue) structures. Bottom panel: Transmission spectra (blue line), average transmission over perturbation (red line), and mean square error (gray shaded region) for the symmetric structure (left), topological structure (middle), and modified topological structure (right).
{"title":"Modified topological photonic crystal","authors":"Abhradeep Basu, Archita Nath, Suhani Das, Arya Pandey, Aksh Agrawal, Parth Hooda, Chittaranjan Nayak","doi":"10.1140/epjd/s10053-025-01079-7","DOIUrl":"10.1140/epjd/s10053-025-01079-7","url":null,"abstract":"<p>Topological photonic crystals are innovative optical structures that leverage topological phases to achieve robust photonic bandgaps, exhibiting immunity to structural imperfections and disorder. However, a significant challenge in conventional topological photonic crystal designs has been the difficulty in precisely controlling the position of the transmission peak. To address this limitation, we present a modified topological photonic crystal composed of alternating <span>(hbox {SiO}_2)</span> and <span>(hbox {TiO}_2)</span> layers. This design incorporates a synergistic approach that integrates the transfer matrix method, quarter-wavelength thickness design principles, and iterative optimization of layer parameters to ensure precise wavelength alignment and enhanced spectral control. The proposed modified topological photonic crystal demonstrates superior performance, including wider photonic bandgaps, moderate transmission efficiency, and improved resistance to structural defects.</p><p>Top panel: Schematic diagrams of the proposed structure without modification (top) and with modification (bottom), together with the transmission spectra for the symmetric (red) and topological (blue) structures. Bottom panel: Transmission spectra (blue line), average transmission over perturbation (red line), and mean square error (gray shaded region) for the symmetric structure (left), topological structure (middle), and modified topological structure (right).</p>","PeriodicalId":789,"journal":{"name":"The European Physical Journal D","volume":"79 11","pages":""},"PeriodicalIF":1.5,"publicationDate":"2025-11-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145456302","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 : 2025-11-05DOI: 10.1140/epjd/s10053-025-01090-y
Serhat F. Özeren
In this study, we investigate the classical and quantum dynamics of a harmonic oscillator with a mass that increases over time and asymptotically approaches a finite limit. The mass evolution is modeled by a logistic-type growth law, which leads to the disappearance of the effective damping in the longtime limit. Two scenarios are considered: (i) the case of a constant spring constant, corresponding to a parametric oscillator with decreasing frequency, and (ii) the case of a constant natural frequency, where the stiffness increases proportionally with the mass. In the classical regime, we derive the exact equations of motion, analyze phase-space trajectories, and examine the time evolution of the total energy. In both cases, as (t to infty), the oscillator approaches a stable periodic motion with constant energy. In the quantum regime, we employ the SU(1,1) coherent state formalism to obtain semiclassical equations of motion and compare them with the classical results. The analytical results obtained are supported by numerical simulations.