{"title":"Effects of ion source term on the sheath in electronegative dusty plasmas","authors":"S.A. Galyanseyedi , G. Foroutan , T. Mohsenpour","doi":"10.1016/j.newast.2025.102476","DOIUrl":null,"url":null,"abstract":"<div><div>This study examines a stationary model of the magneto-electronegative dusty plasma sheath, treating dust particles as a cold fluid. In the present model, the electron and negative ion are in Maxwellian thermodynamic equilibrium, while positive ions are considered as a hot fluid with an ion source term. The effects of ion sources and ionization frequencies (IFs) on the sheath are examined to compare their contributions. A modified sheath criterion and floating potential are established theoretically using the Sagdeev potential method. The governing equations of the model are then solved numerically. The effects of the ion source on sheath electric potential, particle density, positive ion velocity, and space charge density are also investigated. It was found that the modified Bohm criterion decreases with an increase of the IF. It can be seen that the different ion source term is effective in the dusty plasma sheath structure.</div></div>","PeriodicalId":54727,"journal":{"name":"New Astronomy","volume":"122 ","pages":"Article 102476"},"PeriodicalIF":2.1000,"publicationDate":"2025-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"New Astronomy","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1384107625001265","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This study examines a stationary model of the magneto-electronegative dusty plasma sheath, treating dust particles as a cold fluid. In the present model, the electron and negative ion are in Maxwellian thermodynamic equilibrium, while positive ions are considered as a hot fluid with an ion source term. The effects of ion sources and ionization frequencies (IFs) on the sheath are examined to compare their contributions. A modified sheath criterion and floating potential are established theoretically using the Sagdeev potential method. The governing equations of the model are then solved numerically. The effects of the ion source on sheath electric potential, particle density, positive ion velocity, and space charge density are also investigated. It was found that the modified Bohm criterion decreases with an increase of the IF. It can be seen that the different ion source term is effective in the dusty plasma sheath structure.
期刊介绍:
New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation.
New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.