High Energy Density Physics最新文献

{"title":"On the study of unidirectional wave propagation: Exploring the fractional wave structures","authors":"Jan Muhammad ,&nbsp;Usman Younas ,&nbsp;Ahmed Zubair Jan","doi":"10.1016/j.hedp.2025.101252","DOIUrl":"10.1016/j.hedp.2025.101252","url":null,"abstract":"<div><div>In this study, we explore the solitary wave structure of the fractional (3+1) unidirectional wave model. This model is regarded as a significant high-order nonlinear partial differential equation that incorporates additional spatial and dispersive effects to generalize the concepts to more complex wave dynamics, applicable in engineering and science to comprehend complex phenomena and systems. These models aid in predicting the kinematics and wave development of irregular wave trains. The properties of unidirectional wave spectra are considered as well in order to understand wave behavior and its effects in coastal areas. To investigate the solitary wave solutions in unidirectional wave model, we use advanced analytical methods such as the generalized projective Riccati equation method, the new improved generalized exponential–rational function method and Riccati modified extended simple equation method, as well as using mathematical simulations to get a better understanding of wave propagation. The use of nonlinear optical phenomena in fluid dynamics and a number of other research areas is greatly influenced by soliton theory research. This has led to a notable increase in the focus of scholars on the study of such solitons in the last several decades. To investigate the desired soliton solutions, the nonlinear fractional partial differential equation is transformed into their corresponding ordinary differential equations using wave transforms with <span><math><mi>β</mi></math></span> and truncated <span><math><mi>M</mi></math></span>-fractional derivatives. The recommended approaches result in a number of soliton solutions including dark, bright, bright dark, singular, periodic and combined solitons. The results demonstrate the effectiveness and adaptability of the approaches used in solving complex nonlinear systems. Different physical parametric values are utilized to examine the dynamics of the obtained solutions. Examining the efficacy of current methods and clarifying the particular behaviors of the nonlinear dynamics of the system, this work contributes novel information to the area of high-dimensional nonlinear and nonlinear scientific wave phenomena. This not only expands the known solution space but also offers new insights into wave behavior in complex physical systems. The results have practical implications in nonlinear optics, fluid dynamics, and high-energy density physics, and open new avenues for modeling solitary wave propagation in real-world applications.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"58 ","pages":"Article 101252"},"PeriodicalIF":0.9,"publicationDate":"2026-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145694361","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Investigating casimir wormhole solutions supported by Yukawa potentials in modified symmetric teleparallel gravity","authors":"Chaitra Chooda Chalavadi ,&nbsp;V. Venkatesha ,&nbsp;H. Aruna Kumara ,&nbsp;S.V. Divya Rashmi","doi":"10.1016/j.hedp.2025.101222","DOIUrl":"10.1016/j.hedp.2025.101222","url":null,"abstract":"<div><div>This study delves into the phenomenon of Yukawa–Casimir wormholes within the context of modified symmetric teleparallel gravity. By employing an original approach that combines Casimir energy density with Yukawa potentials, we investigate two distinct scenarios. The manuscript examines the impact of model parameters on the existence of these wormhole structures and explores their characteristics by incorporating a traceless fluid equation of state. Notably, the derived shape functions satisfy all fundamental criteria, and the presence of exotic matter is confirmed in all cases. Furthermore, we analyze the stability of Yukawa–Casimir wormholes using the TOV equation, which supports the viability and stability of our constructed model.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101222"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144902507","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Dynamical analysis of fraction soliton solutions, and analysis of multistability, bifurcation, and chaotic nature of m-fractional nonlinear evolution equation through two analytical methods: a comprehensive study","authors":"Mohamed Abdalla ,&nbsp;Md. Mamunur Roshid ,&nbsp;Mahtab Uddin ,&nbsp;Mohammad Safi Ullah","doi":"10.1016/j.hedp.2025.101242","DOIUrl":"10.1016/j.hedp.2025.101242","url":null,"abstract":"<div><div>In this manuscript, we study a fractional new variant (2+1)-dimensional Boussinesq equation (M-fNVBE), focusing on the parametric bifurcation, chaotic nature, multistability, soliton solutions, and the influence of fractional parameters on it. This equation is used to describe how waves move in shallow water. It can also be utilized in fluid dynamics, atmospheric science, and acoustics. First, we investigate the chaotic nature, parametric bifurcation, Lyapunov exponent, and multistability with 2D, 3D, and Poincaré diagrams to analyze the unpredictable situation. Secondly, the modified extended tanh (METH) and extended hyperbolic functions (EHF) methods apply to a reliable treatment of the M-fNVBE, conducting exact soliton solutions. The obtained results are stated as a function of trigonometric, rational, and hyperbolic forms. We identified a variety of soliton wave patterns, like W-shape soliton, bright and dark periodic singular soliton solutions, bright bell soliton, dark bell soliton solutions, periodic rogue wave soliton solutions by using METH method and periodic soliton solutions, bright bell soliton, dark bell soliton solutions, rogue wave soliton solutions by EHF method, each delineated by graphical simulations to emphasize their distinct characteristics and existence criteria. By using chaos theory, bifurcation analysis, and soliton dynamics together, this work makes a big step forward in our knowledge of fractional Boussinesq-type equations. Researchers in wave mechanics, fluid dynamics, and nonlinear sciences can use the resulting solutions and stability assessments to help them with disaster prediction, energy transport, and signal processing. This text connects mathematical theory with real-world wave phenomena, which makes it useful for both theoretical and applied disciplines.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101242"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145617723","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Dynamics of a singularity-free universe in f(R,T2) Gravity","authors":"I. Hashim ,&nbsp;M. Sharif ,&nbsp;M. Zeeshan Gul","doi":"10.1016/j.hedp.2025.101223","DOIUrl":"10.1016/j.hedp.2025.101223","url":null,"abstract":"<div><div>This study investigates bouncing cosmological solutions to understand cosmic evolution in the background of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>R</mi><mo>,</mo><msup><mrow><mi>T</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>)</mo></mrow></mrow></math></span> theory, where <span><math><mi>R</mi></math></span> denotes the Ricci scalar and <span><math><mrow><msup><mrow><mi>T</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>=</mo><msup><mrow><mi>T</mi></mrow><mrow><mi>ξ</mi><mi>η</mi></mrow></msup><msub><mrow><mi>T</mi></mrow><mrow><mi>ξ</mi><mi>η</mi></mrow></msub></mrow></math></span> is the self-contraction of the stress energy tensor. For this purpose, we analyze a flat Friedmann–Robertson–Walker spacetime with perfect matter distribution and assume a specific functional form of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>R</mi><mo>,</mo><msup><mrow><mi>T</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>)</mo></mrow></mrow></math></span> theory to explore the effects of modified gravity on cosmic dynamics. Further, we evaluate super bounce and exponential bounce models to investigate the non-singular universe in this framework. The positive behavior of energy density and the negative behavior of pressure, as well as null energy condition ensure the existence of a viable cosmological bounce solutions. The equation of state parameter indicates the phantom region corresponding to the super bounce model and the quintessence era for exponential bounce model, indicating that the universe experiences cosmic acceleration. The stability of the obtained solutions is analyzed through linear perturbation, demonstrating the model’s robustness against small fluctuations and confirming its validity as a framework for understanding cosmic evolution. Our findings suggest that this modified gravitational theory provides an alternative framework to standard cosmology, offering insights into gravitational interactions and the early cosmic evolution.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101223"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144902509","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Dark energy influenced compact spheres under Karmarkar condition","authors":"Mariyah Aslam ,&nbsp;Adnan Malik ,&nbsp;Gulfam Shahzadi ,&nbsp;Alina Asim ,&nbsp;Fatemah Mofarreh","doi":"10.1016/j.hedp.2025.101233","DOIUrl":"10.1016/j.hedp.2025.101233","url":null,"abstract":"<div><div>This paper investigates the viability and stability of anisotropic dark energy stars using the embedding class-1 technique within Einstein’s general relativity. The widely used Krori–Barua ansatz is adopted for the temporal metric component, while the radial counterpart is derived by enforcing the Karmarkar condition. To close the system, we introduce an equation of state in which the dark energy density is directly proportional to the isotropic baryonic fluid density, with the proportionality parameter <span><math><mi>ϖ</mi></math></span>. The model’s unknown parameters are determined by applying junction conditions between the interior solution and the Schwarzschild exterior manifold. A comprehensive physical analysis ensures the regularity and consistency of metric potentials and state determinants. The compactness factor and gravitational redshift provide insights into stellar objects such as PSR J1903+327, SMC X-4, LMC X-4 and Her X-1. Furthermore, energy bounds validate the model’s physical plausibility, while stability is examined through the Tolman–Oppenheimer–Volkoff equation, causality condition, Zeldovich criterion and adiabatic index. The results indicate that, for the observed masses and radii of the selected stellar objects, the proposed embedded model remains physically consistent, offering a viable and stable description of anisotropic dark energy stars.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101233"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145096245","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Energy-driven soliton dynamics in the (2+1) KP-BBM model: Exact solutions and numerical insights","authors":"Dean Chou ,&nbsp;Abdul Rehman Tahseen ,&nbsp;Yasser Alrashedi ,&nbsp;Theyab Alrashdi ,&nbsp;Hamood Ur Rehman","doi":"10.1016/j.hedp.2025.101241","DOIUrl":"10.1016/j.hedp.2025.101241","url":null,"abstract":"<div><div>In this article, we explore the energy-guided evolution of the (2+1)-dimensional Kadomtsev–Petviashvili– Benjamin–Bona–Mahony (KP-BBM) equation — an important nonlinear evolution equation that describes bidirectional traveling water surface waves and simulates intricate fluid energy flows. To reveal the abundant energy structures underlying this system, we use the modified Sardar sub-equation technique, a powerful and effective analytical tool for producing multifamily solutions with ease. By following this method, we obtain a range of new and physically relevant exact energy solutions, such as dark solitons, bright solitons, singular solitons, exponential solitons, and singular periodic waveforms. To better expose wave energy propagation and interaction in the KP-BBM model, we offer extensive graphical visualizations: 2D profiles, 3D surface plots, and contour maps show in detail the complex energy landscapes and wave dynamics. To justify the accuracy and energetic stability of such solutions, we use the differential transform method (DTM) for numerical approximations. The good agreement between analytical and numerical solutions provides justification for the efficiency and reliability of the suggested method in modeling nonlinear wave energy dynamics. In general, this study not only shows the versatility of the upgraded Sardar sub-equation technique for the solution of energy-abundant nonlinear wave equations but also broadens the theoretical horizon on wave energy transport in fluid mechanics. To ensure the robustness of our results, we performed a stability analysis on the derived solutions, confirming their reliability and physical applicability.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101241"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145519936","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Implications of modified Gauss–Bonnet gravity on gravastar-like structures: High-energy stability and electromagnetic effects","authors":"M. Yousaf ,&nbsp;H. Asad ,&nbsp;Muhammad Aslam","doi":"10.1016/j.hedp.2025.101221","DOIUrl":"10.1016/j.hedp.2025.101221","url":null,"abstract":"<div><div>In this study, we explore the formation and stability of electrically charged, singularity-free, cylindrically symmetric gravastar-like structures as viable alternatives to black holes in the framework of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>G</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></mrow></math></span> gravity. Here, <span><math><mi>G</mi></math></span> represents the Gauss–Bonnet term, while <span><math><mi>T</mi></math></span> denotes the trace of the energy–momentum tensor. We construct solutions across three distinct regions, employing an appropriate equation of state (EoS) for each to describe their physical properties. By deriving the metric coefficients and analyzing the equations of motion with the non-conservation law in a cylindrically symmetric spacetime, we examine the impact of electromagnetic fields on entropy, energy, and structural length. Our analysis is relevant to the study of high-energy astrophysical environments, such as relativistic plasma structures, non-local thermodynamic equilibrium (LTE) kinetic conditions, and the interiors of ultra-dense objects. Through a graphical investigation, we demonstrate that cylindrical gravastar-like objects can exist in nature under specific parametric choices within Gauss–Bonnet corrected gravity, contributing to the broader understanding of matter and radiation interactions under extreme conditions. Furthermore, we assess the role of charge in modifying the stability conditions of these compact objects. Through the second derivative of the potential function and the derived constraint equation, we establish that charged gravastar models exhibit enhanced stability compared to their uncharged counterparts, provided appropriate parametric conditions are met. Our findings offer insights into the interplay between modified gravity, such as <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mi>G</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></mrow></math></span> gravity, and the behavior of energy density profiles influenced by electromagnetic effects in compact charged structures.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101221"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144902510","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Dynamical visualization and modulation instability of two nonlinear fractional models via generalized Kudryashov method","authors":"Jamshad Ahmad ,&nbsp;Khalid Masood ,&nbsp;Farah Pervaiz ,&nbsp;Nehad Ali Shah","doi":"10.1016/j.hedp.2025.101237","DOIUrl":"10.1016/j.hedp.2025.101237","url":null,"abstract":"<div><div>In this paper we applied the generalized Kudryashov method (GKM) to investigate the exact traveling wave solutions to nonlinear evolution equations (NLEEs) in the domain of applied physics and engineering. The current article explores two dynamical models named as the time-fractional Benney Luke (FBL) equation and the time-fractional Clannish Random Walker’s parabolic (FCRWP) equation. These equations can be utilized to explain the contact between the modes in nonlinear optics, fluid mechanics, acoustics, anomalous diffusion, biophysics, plasma physics, image processing, and ecology. Fractional nonlinear partial differential equations (FNLPDEs) have become prevalent due to their capability to describe intricate physical events. We demonstrate the dynamics of the assessed solutions for understanding the real phenomena of such nonlinear models by plotting their 3D, 2D, contour, and density profiles using proper parametric values. Consequently, we obtain distinct types of solutions, containing dark, bright, kink, singular, combo kink singular, and combo dark singular soliton solutions. These results are essential to the explanation of several mesmerizing and intricate physical phenomena. Also, the modulation instability (MI) of the proposed models is analyzed, and conditions are developed accordingly. The soliton solutions demonstrate the competency of the proposed technique in identifying traveling wave solutions, offering a useful tool for tackling a variety of nonlinear evolution equations (NLEEs). The proposed models have applications in various scientific domains, including condensed matter physics, hydrodynamics, plasma physics, optical fiber communications, ocean engineering, and nonlinear dynamics.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101237"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145415663","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Influences of shock imprinting on mix in a 3D-printed porous media","authors":"R.S. Lester,&nbsp;B.J. Albright,&nbsp;N.S. Christiansen,&nbsp;T.A. Coffman,&nbsp;L.M. Green,&nbsp;M.A. Gunderson,&nbsp;B.M. Haines,&nbsp;Y. Kim,&nbsp;P.M. Kozlowski,&nbsp;J.M. Levesque,&nbsp;R.E. Olson,&nbsp;D.W. Schmidt,&nbsp;R.W. VanDervort,&nbsp;C.H. Wong","doi":"10.1016/j.hedp.2025.101224","DOIUrl":"10.1016/j.hedp.2025.101224","url":null,"abstract":"<div><div>Mixing of materials in porous media can cause a significant impact on fusion yield as previously demonstrated by the National Ignition Facility (NIF) MARBLE Campaign. Initially, the reactants are separated, with deuterium in the lattice struts and a tritium gas fill in the voids. Lattice parameters such as the strut thickness and relative pitch, provide a control for the mix parameters in the experiment. Los Alamos National Laboratory’s (LANL) BOSQUE project looks to better understand how the mix of the reactants and shell materials impact the fusion burn and resultant yield on various laser platforms. xRAGE’s Eulerian hydrodynamics and adaptive mesh refinement (AMR) provide the unique ability to study the impacts of multiscale features of complex lattice structures. This modeling provides the ability to measure shock front variations as the wave progress’ through a given media. Initial conditions of the lattice are essential to accurately model mix and burn measured by experiment. By varying the initial orientation and densities of these lattice regions the early time dynamics of how the shock is launched into the system is changed and advocates for the study of resulting effects. In this work, we will study the sensitivities of shock effects in varying 3D printed geometric systems and how these shocks alter the structure and mix in the lattice. We will discuss both preliminary experimental results and simulations to help plan and constrain future experiments where we will study the impact of different lattice geometries and lattice bulk densities. This work concludes with the relative impacts of lattice geometries on shock speeds at different bulk densities and the resultant mix widths due to those shock interactions. We see agreement with theory at the higher end of our bulk density study, however, as we approach lower bulk density systems the dynamics of these interactions begin to change.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101224"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144912307","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}

{"title":"Analysis of charged spherical structures via minimal geometric deformation in f(Q,T) theory","authors":"M. Zeeshan Gul ,&nbsp;M. Sharif ,&nbsp;Sadia Zahid ,&nbsp;Adnan Malik ,&nbsp;Fei Ni","doi":"10.1016/j.hedp.2025.101239","DOIUrl":"10.1016/j.hedp.2025.101239","url":null,"abstract":"<div><div>In this manuscript, we investigate the charged spherical solutions with anisotropic matter configuration using gravitational decoupling via minimal geometric deformation technique in the framework of extended symmetric teleparallel theory. The presence of an additional source in this theory introduces anisotropy into the interior geometry. This method decouples the radial component and separates the field equations into two distinct sets that represent isotropic and anisotropic sources. The viable metric coefficients are applied to solve the first set of equations, while the second set containing unknown variables is solved by imposing specific constraints on the pressure and density. Anisotropic effects can be found by integrating solutions from both distributions. The influence of the decoupling factor on various cosmic parameters was investigated to determine the physical viability of charged spherical systems. The stability of each solution was assessed using causality approach and Herrera cracking method. The obtain results reveal that the considered modified theory provides the viable solutions with a stable structure.</div></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"57 ","pages":"Article 101239"},"PeriodicalIF":0.9,"publicationDate":"2025-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145568409","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"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}