期刊文献+

Elastic rescattering photoelectron distributions entering the relativistic regime

Elastic rescattering photoelectron distributions entering the relativistic regime
原文传递
导出
摘要 We report photoelectron energy spectra and angular distributions for ionization with elastic scattering in ultra- strong laser fields. Noble gas species with Hartree-Fock scattering potentials show a reduction in elastic rescat- tering with the increasing energy of ultrastrong fields and when the Lorentz deflection of the photoelectron exceeds its wave function spread. The relativistic extension of a three-step recollision model is well-suited to the ultrastrong intensity regime (〉10^17 W/cm2) that lies between traditional strong fields and extreme relativistic interactions. We report photoelectron energy spectra and angular distributions for ionization with elastic scattering in ultra- strong laser fields. Noble gas species with Hartree-Fock scattering potentials show a reduction in elastic rescat- tering with the increasing energy of ultrastrong fields and when the Lorentz deflection of the photoelectron exceeds its wave function spread. The relativistic extension of a three-step recollision model is well-suited to the ultrastrong intensity regime (〉10^17 W/cm2) that lies between traditional strong fields and extreme relativistic interactions.
出处 《Chinese Optics Letters》 SCIE EI CAS CSCD 2015年第7期9-13,共5页 中国光学快报(英文版)
基金 supported by the National Science Foundation under Award PHY-1307042 the Delaware Space Grant College and Fellowship Program NNX10AN63H
  • 相关文献

参考文献26

  • 1L.F.DiMauro and P.Agostini, Adv.At.Mol.Opt.Phys.D 35, 79(1995).
  • 2Y.Huismans, A.Rouzee, A.Gijsbertsen, J.H.Jungmann, A.S.Smolkowska, P.S.W.M.Logman, F.Lepine, C.Cauchy, S.Zamith, T.Marchenko, J.M.Bakker, G.Berden, B.Redlich, A.F.G.van der Meer, H.G.Muller, W.Vermin, K.J.Schafer, M.Spanner, M.Y.Ivanov, O.Smirnova, D.Bauer, S.V.Popruzhenko, and M.J.J.Vrakking, Science 331, 61 (2011).
  • 3T.Weber, H.Giessen, M.Weckenbrock, G.Urbasch, A.Staudte, L.Spielberger, O.Jagutzki, V.Mergel, M.Vollmer, and R.Dorner, Nature 405, 658 (2000).
  • 4M.-C.Chen, C.Mancuso, C.Hernandez-Garcia, F.Dollar, B.Galloway, D.Popmintchev, P.-C.Huang, B.Walker, L.Plaja, A.A.Jaron-Becker, A.Becker, M.M.Murnane, H.C.Kapteyn, andT.Popmintchev, in Proc.Natl.Acad.Sci.USA111, E2361(2014).
  • 5J.Itatani, J.Levesque, D.Zeidler, H.Niikura, H.Pepin, J.Kieer, P.Corkum, and D.Villeneuve, Nature 432, 867 (2004).
  • 6B.Walker, B.Sheehy, K.C.Kulander, and L.F.DiMauro, Phys.Rev.Lett.77, 5031 (1996).
  • 7P.B.Corkum, Phys.Rev.Lett.71, 1994 (1993).
  • 8D.B.Milosevic, G.G.Paulus, D.Bauer, and W.Becker, J.Phys.B 39, R203 (2006).
  • 9C.J.Joachain, N.J.Kylstra, and R.M.Potvliege, J.Mod.Opt.50, 313 (2003).
  • 10D.B.Milosevic, S.Hu, and W.Becker, Phys.Rev.A 63, 011403(R) (2000).

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部