Fundamental Plasma Physics最新文献

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Model expressions for refractive indices of electron waves in cold magnetoactive plasma of arbitrary density 任意密度冷磁动等离子体中电子波折射率的模型表达式
Fundamental Plasma Physics Pub Date : 2024-05-06 DOI: 10.1016/j.fpp.2024.100053
D.R. Shklyar , N.S. Artekha
{"title":"Model expressions for refractive indices of electron waves in cold magnetoactive plasma of arbitrary density","authors":"D.R. Shklyar ,&nbsp;N.S. Artekha","doi":"10.1016/j.fpp.2024.100053","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100053","url":null,"abstract":"<div><p>Despite the undoubted importance of having fairly simple analytical expressions for the refractive indices of wave modes in a magnetoactive plasma, such expressions are known only in some particular cases. For electron waves with frequencies much higher than the lower hybrid resonance frequency, such an expression is known only for whistler waves in a dense plasma when the electron plasma frequency significantly exceeds the electron cyclotron frequency. In this Letter, we propose simple operational expressions for the refractive indices of all four electron modes in a magnetoactive plasma, namely, the fast magnetosonic, also called whistler mode, the slow extraordinary mode, the ordinary mode, and the fast extraordinary mode. The form of these expressions does not depend on the value of the ratio of plasma frequency to cyclotron frequency.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100053"},"PeriodicalIF":0.0,"publicationDate":"2024-05-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000189/pdfft?md5=cfce0ca354cae85e7af3b6727d940f9a&pid=1-s2.0-S2772828524000189-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140901363","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Plasma wave propagation conditions analysis using the warm multi-fluid model 利用暖多流体模型分析等离子体波的传播条件
Fundamental Plasma Physics Pub Date : 2024-04-26 DOI: 10.1016/j.fpp.2024.100050
Huasheng Xie , Haojie Ma , Yukun Bai
{"title":"Plasma wave propagation conditions analysis using the warm multi-fluid model","authors":"Huasheng Xie ,&nbsp;Haojie Ma ,&nbsp;Yukun Bai","doi":"10.1016/j.fpp.2024.100050","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100050","url":null,"abstract":"<div><p>Although an accurate description of wave propagation and absorption in plasmas requires complicated full-wave solutions or kinetic simulations, local dispersion analysis can still be helpful to capture the main physics of wave properties. Plasma wave propagation conditions or accessibility informs whether a wave can propagate to a region, which usually depends on the wave frequency, wave vector, the local plasma density, and magnetic field. We demonstrate a warm multi-fluid eigenvalue model and a matrix approach to rapidly calculate plasma wave accessibility diagrams, where thermal effects are also included via an isotropic pressure term. All cold plasma waves, from high-frequency electron cyclotron waves, intermediate-frequency lower hybrid waves, to low-frequency ion cyclotron waves, are presented. By comparing with the kinetic model, it is interesting to find that the warm multi-fluid model, though incapable of reproducing the Bernstein modes, can provide a quick way to determine whether thermal effects are important.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100050"},"PeriodicalIF":0.0,"publicationDate":"2024-04-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000153/pdfft?md5=e7df8ca765e52eb87ab1b02c3084e6b4&pid=1-s2.0-S2772828524000153-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140807850","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Prospects of negative triangularity tokamak for advanced steady-state confinement of fusion plasmas in MHD stability consideration 在考虑 MHD 稳定性的情况下,负三角形托卡马克用于聚变等离子体先进稳态约束的前景
Fundamental Plasma Physics Pub Date : 2024-04-26 DOI: 10.1016/j.fpp.2024.100051
Linjin Zheng, M.T. Kotschenreuther, F.L. Waelbroeck, M.E. Austin, W.L. Rowan, P. Valanju, X. Liu
{"title":"Prospects of negative triangularity tokamak for advanced steady-state confinement of fusion plasmas in MHD stability consideration","authors":"Linjin Zheng,&nbsp;M.T. Kotschenreuther,&nbsp;F.L. Waelbroeck,&nbsp;M.E. Austin,&nbsp;W.L. Rowan,&nbsp;P. Valanju,&nbsp;X. Liu","doi":"10.1016/j.fpp.2024.100051","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100051","url":null,"abstract":"<div><p>The steady-state confinement, beta limit, and divertor heat load are among the most concerned issues for toroidal confinement of fusion plasmas. In this work, we show that the negative triangularity tokamak has promising prospects to address these issues. We first demonstrate that the negative triangularity tokamak generates the filed line rotation transform more effectively. This brings bright prospects for the advanced steady-state tokamak scenario. Given this, the MHD stability and equilibrium confinement of negative triangularity tokamak are investigated. We point out that the negative triangularity configuration with a broad pressure profile is indeed more unstable for low-<span><math><mi>n</mi></math></span> magnetohydrodynamic modes than the positive triangularity case so that the H-mode confinement can hardly be achieved in this configuration, where <span><math><mi>n</mi></math></span> is the toroidal mode number. Nevertheless, we found that the negative triangularity configuration with high bootstrap current fraction, high poloidal beta, and peaked pressure profiles can achieve higher normalized beta for low-<span><math><mi>n</mi></math></span> modes than the positive triangularity case. In a certain parameter domain, the normalized beta can reach about twice the extended Troyon limit, while the same computation indicates that the positive triangularity configuration is indeed constrained by the Troyon limit. This shows that the negative triangularity tokamaks are not only favorable for divertor design to avoid the edge localized modes but also can have promising prospects for advanced steady-state confinement of fusion plasmas in high beta.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100051"},"PeriodicalIF":0.0,"publicationDate":"2024-04-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000165/pdfft?md5=7226485704d08552a46a853c6c20fd6c&pid=1-s2.0-S2772828524000165-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140821979","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Possibility of inverse sheath in the lunar nightside due to secondary electron emission 二次电子发射导致月球夜面出现反向鞘的可能性
Fundamental Plasma Physics Pub Date : 2024-04-26 DOI: 10.1016/j.fpp.2024.100052
Trinesh Sana , S.K. Mishra
{"title":"Possibility of inverse sheath in the lunar nightside due to secondary electron emission","authors":"Trinesh Sana ,&nbsp;S.K. Mishra","doi":"10.1016/j.fpp.2024.100052","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100052","url":null,"abstract":"<div><p>This study assesses the plasma sheath formation on the night side of the Moon when exposed to highly energetic ambient plasma. The calculations indicate that the secondary electron emission (SEE) due to highly energetic plasma electrons leads to the formation of the inverse sheath around the positively charged lunar surface on the night side, where a traditional Debye sheath with a high negative surface potential is anticipated. Analytical formulation of Debye sheath and inverse sheath formation is given considering Maxwellian plasma and secondary electrons and cold ions. For a given SEE yield, a temperature regime is predicted where the inverse sheath is possible.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100052"},"PeriodicalIF":0.0,"publicationDate":"2024-04-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000177/pdfft?md5=cf67cb1e7da06258ca9aabfa9742a47a&pid=1-s2.0-S2772828524000177-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140813170","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
From kink instability to magnetic reconnection to oscillations in solar flares 从太阳耀斑的扭结不稳定性到磁重联再到振荡
Fundamental Plasma Physics Pub Date : 2024-04-20 DOI: 10.1016/j.fpp.2024.100049
Philippa K. Browning, Mykola Gordovskyy, Luiz A.C.A. Schiavo, James Stewart
{"title":"From kink instability to magnetic reconnection to oscillations in solar flares","authors":"Philippa K. Browning,&nbsp;Mykola Gordovskyy,&nbsp;Luiz A.C.A. Schiavo,&nbsp;James Stewart","doi":"10.1016/j.fpp.2024.100049","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100049","url":null,"abstract":"<div><p>We show how some different fundamental plasma processes - the ideal kink instability, magnetic reconnection and magnetohydrodynamic oscillations - can be causally linked. This is shown through reviewing a series of models of energy release in twisted magnetic flux ropes in the solar corona, representing confined solar flares. 3D magnetohydrodynamic simulations demonstrate that fragmented current sheets develop during the nonlinear phase of the ideal kink instability, leading to multiple magnetic reconnections and the release of stored magnetic energy. By coupling these simulations with a test particle code, we can predict the development of populations of non-thermal electrons and ions, as observed in solar flares, and produce synthetic observables for comparison with observations. We also show that magnetic oscillations arise in the reconnecting loop, although there is no oscillatory external driver, and these lead to pulsations in the microwave emission similar to observed flare quasi-periodic pulsations. Oscillations and propagating waves also arise from reconnection when two twisted flux ropes merge, which is modelled utilising 2D magnetohydrodynamic simulations.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100049"},"PeriodicalIF":0.0,"publicationDate":"2024-04-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000141/pdfft?md5=617285bdd749202a8b7b0881cb9438df&pid=1-s2.0-S2772828524000141-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140649779","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Electrostatic supersolitary waves: A challenging paradigm in nonlinear plasma science and beyond – State of the art and overview of recent results 静电超孤立波:非线性等离子体科学及其他领域的挑战性范例 - 技术现状和最新成果概览
Fundamental Plasma Physics Pub Date : 2024-04-18 DOI: 10.1016/j.fpp.2024.100048
Steffy Sara Varghese , Kuldeep Singh , Ioannis Kourakis
{"title":"Electrostatic supersolitary waves: A challenging paradigm in nonlinear plasma science and beyond – State of the art and overview of recent results","authors":"Steffy Sara Varghese ,&nbsp;Kuldeep Singh ,&nbsp;Ioannis Kourakis","doi":"10.1016/j.fpp.2024.100048","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100048","url":null,"abstract":"<div><p>A comprehensive overview is presented of recent theoretical advancements and observational manifestations of a relatively new type of electrostatic solitary wave (ESW), known as <em>supersoliton</em> or <em>supersolitary wave</em> (SSW). These nonlinear structures are characterized by a distorted pulse-shaped electrostatic potential excitations, deviating from the standard (“sech<sup>2</sup>”-like) form generally expected from solitonic pulses. In Space plasmas, in particular, e.g. in magnetospheric observations, SSWs may be associated with a characteristic wiggly bipolar electric field waveform. It has been shown that a three-component configuration is essential, as a minimum requirement for SSWs to occur in a plasma.</p><p>Various spacecraft missions have recorded evidence of “non-conventional” electrostatic solitary waves (pulses) such as wiggly bipolar pulses, offset bipolar pulses, and monopolar pairs. This review article aims to present the current state of the art in this fascinating new theme, first outlining the basic framework for the modeling of such “exotic” ESWs and then putting forward a correlation between SSW structures with certain non-standard bipolar electric field forms observed in planetary magnetospheres.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100048"},"PeriodicalIF":0.0,"publicationDate":"2024-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S277282852400013X/pdfft?md5=49cbcd2a0e610c5b3f1408887a7e700c&pid=1-s2.0-S277282852400013X-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140641202","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
High stability plasma illumination from micro discharges with nanodiamond decorated laser induced graphene electrodes 使用纳米金刚石装饰的激光诱导石墨烯电极进行微放电的高稳定性等离子体照明
Fundamental Plasma Physics Pub Date : 2024-03-30 DOI: 10.1016/j.fpp.2024.100047
S. Suman , S.K. Sethy , K.J. Sankaran
{"title":"High stability plasma illumination from micro discharges with nanodiamond decorated laser induced graphene electrodes","authors":"S. Suman ,&nbsp;S.K. Sethy ,&nbsp;K.J. Sankaran","doi":"10.1016/j.fpp.2024.100047","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100047","url":null,"abstract":"<div><p>Superior lifetime stability for the microplasma device developed by decorating nanodiamonds (nDs) on laser induced graphene (LIG) is reported. Upon overwhelming the difficulty of poor stability in graphene, the nD-LIG displays exceptional lifetime stability of 1770s verified at an applied voltage of 340 V. But, the lifetime stability of LIG is only 718 s at the same applied voltage. Therefore, the nD-LIG with enhanced lifetime stability have pronounced prospective as cathodes in microplasma device applications.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100047"},"PeriodicalIF":0.0,"publicationDate":"2024-03-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000128/pdfft?md5=e82ca17af359f13027806f02cb9aebaf&pid=1-s2.0-S2772828524000128-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140343983","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
KrF laser-driven shock tube: Realization and first experiments KrF 激光驱动冲击管:实现和首次实验
Fundamental Plasma Physics Pub Date : 2024-03-28 DOI: 10.1016/j.fpp.2024.100046
V.D. Zvorykin, P.V. Veliev, I.A. Kozin, N.V. Morozov, E.V. Parkevich, K.T. Smaznova, N.N. Ustinovskii, A.V. Shutov
{"title":"KrF laser-driven shock tube: Realization and first experiments","authors":"V.D. Zvorykin,&nbsp;P.V. Veliev,&nbsp;I.A. Kozin,&nbsp;N.V. Morozov,&nbsp;E.V. Parkevich,&nbsp;K.T. Smaznova,&nbsp;N.N. Ustinovskii,&nbsp;A.V. Shutov","doi":"10.1016/j.fpp.2024.100046","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100046","url":null,"abstract":"<div><p>We report on the first implementation of a miniature laser-driven shock tube (LDST) of 5 × 5 mm cross section and 50-mm length for generating and studying strong shock waves (SW) and hypersonic gas flows with <em>M</em> &gt; 10. Operation of the LDST is based on the acceleration of a thin CH-film by ablative plasma pressure produced when the film is irradiated by high-energy UV pulse of the GARPUN KrF laser (100 J &amp; 100-ns). The film serves as a piston that pushes a SW in the gas filling the LDST. An optical system based on a multi-element prism raster provides focusing of KrF laser beam into 7 × 7 mm square spot with 100 J/cm<sup>2</sup> energy fluence (1 GW/cm<sup>2</sup> intensity) with inhomogeneity ∼3 % across the LDST aperture. It is expected that the LDST with KrF laser driver can be an effective tool for studying hydrodynamic phenomena, such as hydrodynamic instabilities and transition to a turbulence, hypersonic gas flow around bodies, reflection and cumulation of strong SW.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100046"},"PeriodicalIF":0.0,"publicationDate":"2024-03-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000116/pdfft?md5=221386dde950270064ca1f0d9d3b44e3&pid=1-s2.0-S2772828524000116-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140328564","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Ionisation in nanowire by ultra-short relativistic laser pulse 超短相对论激光脉冲在纳米线中的电离作用
Fundamental Plasma Physics Pub Date : 2024-03-27 DOI: 10.1016/j.fpp.2024.100045
F.T.T. Houng , S.Y. Hoh , J.F. Ong
{"title":"Ionisation in nanowire by ultra-short relativistic laser pulse","authors":"F.T.T. Houng ,&nbsp;S.Y. Hoh ,&nbsp;J.F. Ong","doi":"10.1016/j.fpp.2024.100045","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100045","url":null,"abstract":"<div><p>We show that the wakefield driven by fast electrons inside the nanowire when irradiated with an ultra-short relativistic laser pulse strips atoms to a higher charge state. Using particle-in-cell simulations, we demonstrate that the charge state agrees with the barrier suppression threshold of the wakefield and reaches a higher value via collision. The ionisation of gold nanowires occurs only via collisional-damped wakefield. We found that the collisional ionisation of high-Z nanowires depends on the onset of the z pinch. These results suggest a different ionisation mechanism of the structured target in the subfemtosecond regime.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100045"},"PeriodicalIF":0.0,"publicationDate":"2024-03-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000104/pdfft?md5=e871395d63b33dd6eba2ce039a6643f7&pid=1-s2.0-S2772828524000104-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140328565","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Scaling laws of the plasma velocity in visco-resistive magnetohydrodynamic systems 粘阻磁流体动力系统中等离子体速度的缩放规律
Fundamental Plasma Physics Pub Date : 2024-03-19 DOI: 10.1016/j.fpp.2024.100044
A. Krupka, M.-C. Firpo
{"title":"Scaling laws of the plasma velocity in visco-resistive magnetohydrodynamic systems","authors":"A. Krupka,&nbsp;M.-C. Firpo","doi":"10.1016/j.fpp.2024.100044","DOIUrl":"https://doi.org/10.1016/j.fpp.2024.100044","url":null,"abstract":"<div><p>We consider a visco-resistive magnetohydrodynamic modelling of a steady-state incompressible tokamak plasma with a prescribed toroidal current drive, featuring constant resistivity <em>η</em> and viscosity <em>ν</em>. It is shown that the plasma velocity root-mean-square behaves as <span><math><mi>η</mi><mi>f</mi><mo>(</mo><mi>H</mi><mo>)</mo></math></span> as long as the inertial term remains negligible, where <em>H</em> stands for the Hartmann number <span><math><mi>H</mi><mo>≡</mo><msup><mrow><mo>(</mo><mi>η</mi><mi>ν</mi><mo>)</mo></mrow><mrow><mo>−</mo><mn>1</mn><mo>/</mo><mn>2</mn></mrow></msup></math></span>, and that <span><math><mi>f</mi><mo>(</mo><mi>H</mi><mo>)</mo></math></span> exhibits power-law behaviours in the limits <span><math><mi>H</mi><mo>≪</mo><mn>1</mn></math></span> and <span><math><mi>H</mi><mo>≫</mo><mn>1</mn></math></span>. In the latter limit, we establish that <span><math><mi>f</mi><mo>(</mo><mi>H</mi><mo>)</mo></math></span> scales as <span><math><msup><mrow><mi>H</mi></mrow><mrow><mn>1</mn><mo>/</mo><mn>4</mn></mrow></msup></math></span>, which is consistent with numerical results.</p></div>","PeriodicalId":100558,"journal":{"name":"Fundamental Plasma Physics","volume":"10 ","pages":"Article 100044"},"PeriodicalIF":0.0,"publicationDate":"2024-03-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S2772828524000098/pdfft?md5=a466eeef37a256e3c75b644a84b157fa&pid=1-s2.0-S2772828524000098-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140187615","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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