{"title":"Coherent X-Ray Generation Via Laser Pumping of a Relativistic Ion Beam - Feasibility Assessment","authors":"S. Bogacz","doi":"10.1364/sxray.1991.wa3","DOIUrl":null,"url":null,"abstract":"The efficiency of most popular approach to generating short wavelength radiation involving particle beams, FEL1, is limited by the Thomson scattering cross section. If one were to use a beam of particles having a resonant scattering cross section for some frequency, a greatly enhanced gain might be expected. A natural candidate is a hydrogenic positive ion, having Z > 2, with a single bound electron. The fact that the ion is charged allows the beam to be accelerated to relativistic energies (γ≫ 1), therefore one can exploit the properties of relativistic kinematics which dictate that the back scattered radiation will have its wavelength shortened by a factor (2γ)2.","PeriodicalId":409291,"journal":{"name":"Soft-X-Ray Projection Lithography","volume":"175 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Soft-X-Ray Projection Lithography","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/sxray.1991.wa3","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The efficiency of most popular approach to generating short wavelength radiation involving particle beams, FEL1, is limited by the Thomson scattering cross section. If one were to use a beam of particles having a resonant scattering cross section for some frequency, a greatly enhanced gain might be expected. A natural candidate is a hydrogenic positive ion, having Z > 2, with a single bound electron. The fact that the ion is charged allows the beam to be accelerated to relativistic energies (γ≫ 1), therefore one can exploit the properties of relativistic kinematics which dictate that the back scattered radiation will have its wavelength shortened by a factor (2γ)2.