Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T05:36:03.206Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetization of Rydberg plasmas by electromagnetic waves

Published online by Cambridge University Press:  30 November 2009

J. T. MENDONÇA ,
NITIN SHUKLA  and
P. K. SHUKLA
J. T. MENDONÇA
Affiliation:
IPFN and CFIF, Instituto Superior Técnico, 1049-001 Lisboa, Portugal ([email protected])
NITIN SHUKLA
Affiliation:
Department of Physics, Umeå University, SE-90187 Umeå, SE-90187Sweden ([email protected])
P. K. SHUKLA
Affiliation:
Institut für Theoretische Physik IV, Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany ([email protected])
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is shown that the ponderomotive force of a large-amplitude electromagnetic wave in Rydberg plasmas can generate quasi-stationary magnetic fields. The present result can account for the origin of seed magnetic fields in the ultracold Rydberg plasmas when they are irradiated by the high-frequency electromagnetic wave.

Type
Letter to the Editor
Information
Journal of Plasma Physics , Volume 76 , Issue 1 , February 2010 , pp. 19 - 23
Copyright
Copyright © Cambridge University Press 2009

References

[1]Killian, T. C., Kulin, S., Bergeson, S. D., Orozco, L. A., Orzel, C. and Rolston, S. L. 1999 Phys. Rev. Lett. 83, 4776.CrossRefGoogle Scholar
[2]Robinson, M. R., Tolra, B. L., Noel, N. W., Gallagher, T. F. and Pillet, P. 2000 Phys. Rev. Lett. 85, 4466.CrossRefGoogle Scholar
[3]Bergeson, S. D. and Spencer, R. L. 2003 Phys. Rev. E 67, 026414.CrossRefGoogle Scholar
[4]Fletcher, R. S., Zhang, X. L. and Rolston, S. L. 2006 Phys. Rev. Lett. 96, 105003.CrossRefGoogle Scholar
[5]Killian, T. C., Pattard, T., Pohl, T. and Rost, J. M. 2007 Phys. Rep. 44, 77.CrossRefGoogle Scholar
[6]Rolston, S. L. 2008 Physics 1, 2.CrossRefGoogle Scholar
[7]Morrison, J. P., Rennick, C. J., Keller, J. S. and Grant, E. R. 2008 Phys. Rev. Lett. 101, 205005.CrossRefGoogle Scholar
[8]Zhang, X. L., Fletcher, R. S., Rolston, S. L., Guzdar, P. N. and Swisdak, M. 2008 Phys. Rev. Lett. 100, 235002.CrossRefGoogle Scholar
[9]Zhang, X. L., Fletcher, R. S. and Rolston, S. L. 2008 Phys. Rev. Lett. 101, 195002.CrossRefGoogle Scholar
[10]Mendonça, J. T., Kaiser, R., Terças, H. and Loureiro, J. 2008 Phys. Rev. A 78, 013408.CrossRefGoogle Scholar
[11]Mendonça, J. T.Loureiro, J. and Terças, H. 2009 J. Plasma Phys. 75, 713.CrossRefGoogle Scholar
[12]Schlickeiser, R. and Shukla, P. K. 2003 Astrophys. J. 599, L57.CrossRefGoogle Scholar
[13]Karpman, V. I. and Washimi, H. 1976 Sov. Phys. JETP 44, 528.Google Scholar
[14]Gradov, O. M. and Stenflo, L. 1980 Zh. Naturforsch. 35a, 461; 1983 Phys. Lett. A 95A, 233.CrossRefGoogle Scholar
[15]Shukla, P. K. and Yu, M. Y. 1984 Plasma Phys. Control. Fusion 26, 841; Tsintsadze, L. N. and Shukla, P. K. 1994 Phys. Lett. A 187, 67.CrossRefGoogle Scholar
[16]Shukla, P. K., Rao, N. N., Yu, M. Y. and Tsintsadze, N. L. 1986 Phys. Rep. 138, 1; Berezhiani, V. I., Tskhakaya, D. D. and Shukla, P. K. 1992 Phys. Rev. A 46, 6608.CrossRefGoogle Scholar
[17]Marklund, M. and Shukla, P. K. 2006 Rev. Mod. Phys. 78, 591.CrossRefGoogle Scholar