{"title":"Nonresonant Effects in CO2 Amplifier of Ultrashort Laser Pulses","authors":"S. Chelkowski, A. Bandrauk","doi":"10.1364/nlopm.1988.mf22","DOIUrl":null,"url":null,"abstract":"Recently the amplification of subpicosecond pulses in CO2 resonant with 10.6 μm lasing transition 001→100 has been achieved for intensities up to 1012 W/cm2 [1]. This corresponds to Rabi frequency ≃ 10 cm-1 which becomes comparable to the detuning of various CO2 transitions usually neglected in standard calculations [2]. For instance, this Rabi frequency becomes close to the spacing between laser P(20) transition and R(18) transition equal to 32 cm-1 [1,3]. For higher intensities, the 9.6 μm, 001→020 transition should be taken into account, as well as the transitions 001→000, 001-002, etc. - see fig. 1.","PeriodicalId":208307,"journal":{"name":"Nonlinear Optical Properties of Materials","volume":"135 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":"Nonlinear Optical Properties of Materials","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/nlopm.1988.mf22","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
Recently the amplification of subpicosecond pulses in CO2 resonant with 10.6 μm lasing transition 001→100 has been achieved for intensities up to 1012 W/cm2 [1]. This corresponds to Rabi frequency ≃ 10 cm-1 which becomes comparable to the detuning of various CO2 transitions usually neglected in standard calculations [2]. For instance, this Rabi frequency becomes close to the spacing between laser P(20) transition and R(18) transition equal to 32 cm-1 [1,3]. For higher intensities, the 9.6 μm, 001→020 transition should be taken into account, as well as the transitions 001→000, 001-002, etc. - see fig. 1.