{"title":"相对论Buneman不稳定性的一维细胞内粒子模拟","authors":"R. Rajawat, S. Sengupta","doi":"10.1109/PLASMA.2016.7534085","DOIUrl":null,"url":null,"abstract":"Summary form only given. Spatio-temporal evolution of relativistic Buneman instability has been investigated in one dimension using a particle-in-cell simulation code. Starting from the excitation of the instability, its evolution has been followed numerically till its quenching and beyond. It is found that the maximum growth rate(γ<sub>max</sub>) reduces due to relativistic effects and varies with γ<sub>e0</sub> and m/M as γ<sub>max</sub> ~ √(3/4γ<sub>e0</sub>) (m/2M)<sup>1/3</sup>, where γ<sub>e0</sub> is Lorentz factor associated with the initial electron beam velocity(v<sub>o</sub>) and (m/M) is the electron to ion mass ratio. Further it is observed that in contrast to the non-relativistic results<sup>1,2</sup> at the saturation point, ratio of electrostatic field energy density (E<sup>2</sup>/8π) to the initial drift kinetic energy density (W<sub>0</sub>) scales with γ<sub>e0</sub> as ~1/γ<sub>e0</sub><sup>2</sup>. These results are found to be in good agreement with that derived using fluid theory.","PeriodicalId":424336,"journal":{"name":"2016 IEEE International Conference on Plasma Science (ICOPS)","volume":"47 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-06-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"One dimensional particle-in-cell simulation of relativistic Buneman instability\",\"authors\":\"R. Rajawat, S. Sengupta\",\"doi\":\"10.1109/PLASMA.2016.7534085\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Summary form only given. Spatio-temporal evolution of relativistic Buneman instability has been investigated in one dimension using a particle-in-cell simulation code. Starting from the excitation of the instability, its evolution has been followed numerically till its quenching and beyond. It is found that the maximum growth rate(γ<sub>max</sub>) reduces due to relativistic effects and varies with γ<sub>e0</sub> and m/M as γ<sub>max</sub> ~ √(3/4γ<sub>e0</sub>) (m/2M)<sup>1/3</sup>, where γ<sub>e0</sub> is Lorentz factor associated with the initial electron beam velocity(v<sub>o</sub>) and (m/M) is the electron to ion mass ratio. Further it is observed that in contrast to the non-relativistic results<sup>1,2</sup> at the saturation point, ratio of electrostatic field energy density (E<sup>2</sup>/8π) to the initial drift kinetic energy density (W<sub>0</sub>) scales with γ<sub>e0</sub> as ~1/γ<sub>e0</sub><sup>2</sup>. These results are found to be in good agreement with that derived using fluid theory.\",\"PeriodicalId\":424336,\"journal\":{\"name\":\"2016 IEEE International Conference on Plasma Science (ICOPS)\",\"volume\":\"47 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-06-19\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2016 IEEE International Conference on Plasma Science (ICOPS)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/PLASMA.2016.7534085\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2016 IEEE International Conference on Plasma Science (ICOPS)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/PLASMA.2016.7534085","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
One dimensional particle-in-cell simulation of relativistic Buneman instability
Summary form only given. Spatio-temporal evolution of relativistic Buneman instability has been investigated in one dimension using a particle-in-cell simulation code. Starting from the excitation of the instability, its evolution has been followed numerically till its quenching and beyond. It is found that the maximum growth rate(γmax) reduces due to relativistic effects and varies with γe0 and m/M as γmax ~ √(3/4γe0) (m/2M)1/3, where γe0 is Lorentz factor associated with the initial electron beam velocity(vo) and (m/M) is the electron to ion mass ratio. Further it is observed that in contrast to the non-relativistic results1,2 at the saturation point, ratio of electrostatic field energy density (E2/8π) to the initial drift kinetic energy density (W0) scales with γe0 as ~1/γe02. These results are found to be in good agreement with that derived using fluid theory.