尚光网 本站首页 本所首页 联系我们
10.1063/1.4977459SCIAKHIEZER AI, 1956, SOV PHYS JETP-USSR, V3, P696; Beg FN, 2004, PHYS PLASMAS, V11, P2806, DOI 10.1063/1.1704643; BOURDIER A, 1983, PHYS FLUIDS, V26, P1804, DOI 10.1063/1.864355; BRUNEL F, 1987, PHYS REV LETT, V59, P52, DOI 10.1103/PhysRevLett.59.52; Buffechoux S, 2010, PHYS REV LETT, V105, DOI 10.1103/PhysRevLett.105.015005; GIBBON P, 1994, PHYS REV LETT, V73, P664, DOI 10.1103/PhysRevLett.73.664; Guerin S, 1996, PHYS PLASMAS, V3, P2693; Henig A, 2009, PHYS REV LETT, V103, DOI 10.1103/PhysRevLett.103.045002; KAW P, 1970, PHYS FLUIDS, V13, P472, DOI 10.1063/1.1692942; KRUER WL, 1985, PHYS FLUIDS, V28, P430, DOI 10.1063/1.865171; LEFEBVRE E, 1995, PHYS REV LETT, V74, P2002, DOI 10.1103/PhysRevLett.74.2002; Li XY, 2013, PHYS REV E, V88, DOI 10.1103/PhysRevE.88.023106; Lichters R, 1996, PHYS PLASMAS, V3, P3425, DOI 10.1063/1.871619; Lichters R., 1997, 225 MPQ; Mackinnon AJ, 2002, PHYS REV LETT, V88, DOI 10.1103/PhysRevLett.88.215006; MAX C, 1971, PHYS REV LETT, V27, P1342, DOI 10.1103/PhysRevLett.27.1342; Neumayer P, 2010, PHYS PLASMAS, V17, DOI 10.1063/1.3486520; Palaniyappan S, 2012, NAT PHYS, V8, P763, DOI [10.1038/nphys2390, 10.1038/NPHYS2390]; Roth M, 2013, PHYS REV LETT, V110, DOI 10.1103/PhysRevLett.110.044802; Sentoku Y, 2003, PHYS PLASMAS, V10, P2009, DOI 10.1063/1.1556298; TABAK M, 1994, PHYS PLASMAS, V1, P1626, DOI 10.1063/1.870664; Vshivkov VA, 1998, PHYS PLASMAS, V5, P2727, DOI 10.1063/1.872961; Wang HY, 2011, PHYS REV LETT, V107, DOI 10.1103/PhysRevLett.107.265002; WILKS SC, 1993, PHYS FLUIDS B-PLASMA, V5, P2603, DOI 10.1063/1.860697; WILKS SC, 1992, PHYS REV LETT, V69, P1383, DOI 10.1103/PhysRevLett.69.1383255889424243Phys. Plasmas2017INTENSE LASER-PULSES; PROPAGATION; ABSORPTION; TARGETS; COLD; WAVEREORTSOM21797A new phenomenon of an enhanced relativistic transparency of overdense plasmas by the influence of hot-electron refluxing has been discovered via particle-in-cell simulations. When a p-polarized laser pulse, with intensity below the self-induced-transparency (SIT) threshold, obliquely irradiates a thin overdense plasma, the initially opaque plasma becomes transparent after a time interval that is linearly dependent on the thickness of the plasma. This phenomenon can be interpreted as a consequence of hot-electron refluxing, which reduces the effective electron density by longitudinal heating. When the laser intensity is higher than the SIT threshold, the penetration velocity of the laser in the plasma is enhanced when the refluxing is present. Published by AIP Publishing.Hot-electron refluxing enhanced relativistic transparency of overdense plasmas期刊论文EnglishYu, Yong; Li, Xiao-Ya; Chen, Zi-Yu; Wang, Jia-Xiang; Shen, Bai-Fei; Zhu, Wen-Jun33117 WOS:000397872500071
外文题目: Hot-electron refluxing enhanced relativistic transparency of overdense plasmas
作者: Yu, Yong; Li, Xiao-Ya; Chen, Zi-Yu; Wang, Jia-Xiang; Shen, Bai-Fei; Zhu, Wen-Jun
刊名: Phys. Plasmas
年: 2017 卷: 24 期: 3 文章编号:33117
英文关键词:

INTENSE LASER-PULSES; PROPAGATION; ABSORPTION; TARGETS; COLD; WAVE
英文摘要:
文献类型: 期刊论文
正文语种: English
收录类别: SCI  
DOI: 10.1063/1.4977459
全文传递服务
clickdetails
页面点击量: 5
文章下载量: 2
visitlog
友情链接:
  中国光学期刊网
  光电汇
  上海大恒公司
  南京先进激光技术院
  光学产品库
  上海研发公共服务平台
版权所有 © 2009 中国科学院上海光学精密机械研究所 沪ICP备05015387号
主办:中国科学院上海光学精密机械研究所 上海市嘉定区清河路390号(201800)