Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T05:37:09.006Z Has data issue: false hasContentIssue false
  • English
  • Français

Density effects in harmonic emission from intense laser interactions with overdense plasmas

Published online by Cambridge University Press:  01 June 2007

T. J. M. BOYD  and
R. ONDARZA-ROVIRA
T. J. M. BOYD
Affiliation:
Centre for Physics, University of Essex, Wivenhoe Park, Colchester CO4 3SQ, Essex, UK ([email protected])
R. ONDARZA-ROVIRA
Affiliation:
Instituto Nacional de Investigaciones Nucleares, A.P. 18-1027, México 11801, D.F., Mexico ([email protected])
Get access Rights & Permissions [Opens in a new window]

Abstract

Although the harmonics generated when intense laser light interacts with solid targets are broadly understood in terms of their dependence on the incident intensity, less attention has been paid to the ways in which their behaviour depends on plasma density. In this paper the conversion efficiencies of the odd harmonics generated when light is incident normally on the target surface are shown to be strongly resonant in character. The number of resonances is governed by harmonic order and their behaviour with density is further complicated by Langmuir wave emission at the corresponding plasma resonant densities for successive harmonic orders. Only at densities well above these resonances does the emission decay monotonically with density. The density dependence predicted by theory is confirmed by particle-in-cell simulations.

Type
Papers
Information
Journal of Plasma Physics , Volume 73 , Issue 3 , June 2007 , pp. 307 - 313
Copyright
Copyright © Cambridge University Press 2006

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

[1]Norreys, P. A. et al. 1996 Phys. Rev. Lett. 76 11, 1832–1835.CrossRefGoogle Scholar
[2]Gibbon, P. 1996 Phys. Rev. Lett. 76 1, 50–53.CrossRefGoogle Scholar
[3]Kohlweyer, S. et al. 1995 Opt. Commun. 117, 431–438.CrossRefGoogle Scholar
[4]von der Linde, D. et al. 1995 Phys. Rev. A 52 (1), R25–27.CrossRefGoogle Scholar
[5]Zepf, M. et al. 1998 Phys. Rev. E 58, R5253.Google Scholar
[6]Teubner, U. et al. 2003 Phys. Rev. A 67, 013816.CrossRefGoogle Scholar
[7]Gibbon, P. 1997 J. Quantum. Electron. 33 11, 1915–1924.CrossRefGoogle Scholar
[8]Gordienko, S. et al. 2004 Phys. Rev. Lett. 93 11, 115002.CrossRefGoogle Scholar
[9]Ondarza, R. 2003 Phys. Rev. E 67, 066401.Google Scholar
[10]Boyd, T. J. M. and Ondarza-Rovira, R. 2000 Phys. Rev. Lett. 85 7, 1440–1443.CrossRefGoogle Scholar
[11]Wilks, S. C., Kruer, W. L. and Mori, W. B. 1993 IEEE Trans. Plasma Sci. 21 1, 120–124.CrossRefGoogle Scholar
[12]Rozmus, W. and Tikhonchuk, V. T. 1990 Phys. Rev. A 42 12, 7401–7412.CrossRefGoogle Scholar
[13]Gamaliy, E. G. and Dragila, R. 1990 Phys. Rev. A 42 2, 929–935.CrossRefGoogle Scholar