Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-26T00:21:14.977Z Has data issue: false hasContentIssue false

Generation of magnetic fields by the ponderomotive force of electromagnetic waves in dense plasmas

Published online by Cambridge University Press:  17 April 2009

P. K. SHUKLA
Affiliation:
Institut für Theoretische Physik IV, Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany ([email protected])
NITIN SHUKLA
Affiliation:
Department of Physics, Umeå University, SE-90187 Umeå, SE-90187Sweden
L. STENFLO
Affiliation:
Department of Physics, Linköping University, SE-58183 Linköping, SwedenDepartment of Physics, Umeå University, SE-90187 Umeå, Sweden

Abstract

We show that the non-stationary ponderomotive force of a large-amplitude electromagnetic wave in a very dense quantum plasma with streaming degenerate electrons can spontaneously create d.c. magnetic fields. The present result can account for the seed magnetic fields in compact astrophysical objects and in the next-generation intense laser–solid density plasma interaction experiments.

Type
Papers
Copyright
Copyright © Cambridge University Press 2009

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]Biermann, L. 1950 Z. Naturforsch 5a, 65.Google Scholar
[2]Weibel, E. S. 1959 Phys. Rev. Lett. 2, 83.CrossRefGoogle Scholar
[3]Gruzinov, A. 2001 Astrophys. J. 563, L15.CrossRefGoogle Scholar
[4]Schlickeiser, R. and Shukla, P. K. 2003 Astrophys. J. 599, L57.Google Scholar
[5]Karpman, V. I. and Washimi, H. 1976 Sov. Phys. JETP 44, 528.Google Scholar
[6]Karpman, V. I. and Washimi, H. 1977 J. Plasma Phys. 18, 173.Google Scholar
[7]Washimi, H. and Watanabe, M. 1977 J. Phys. Soc. Jpn 42, 1081.Google Scholar
[8]Washimi, H. 1989 J. Phys. Soc. Jpn 58, 3960.CrossRefGoogle Scholar
[9]Gradov, O. M. and Stenflo, L. 1980 Z. Naturforsch. 35a, 461.CrossRefGoogle Scholar
[10]Gradov, O. M. and Stenflo, L. 1983 Phys. Lett. A 95A, 233.CrossRefGoogle Scholar
[11]Shukla, P. K. and Yu, M. Y. 1984 Plasma Phys. Control. Fusion 26, 841.CrossRefGoogle Scholar
[12]Tsintsadze, L. N. and Shukla, P. K. 1994 Phys. Lett. A 187, 67.Google Scholar
[13]Shukla, P. K., et al. 1986 Phys. Rep. 138, 1.CrossRefGoogle Scholar
[14]Berezhiani, V. I., Tskhakaya, D. D. and Shukla, P. K. 1992 Phys. Rev. A 46, 6608.CrossRefGoogle Scholar
[15]Marklund, M. and Shukla, P. K. 2006 Rev. Mod. Phys. 78, 591.CrossRefGoogle Scholar
[16]Stamper, J. A., et al. 1971 Phys. Rev. Lett. 26, 1012.CrossRefGoogle Scholar
[17]Stamper, J. A. and Ripin, B. H. 1975 Phys. Rev. Lett. 34, 138.CrossRefGoogle Scholar
[18]Stamper, J. A. and Tidman, D. A. 1973 Phys. Fluids 16, 2004.CrossRefGoogle Scholar
[19]Hasegawa, A., Yu, M. Y., Shukla, P. K., and Spatschek, K. H. 1978 Phys. Rev. Lett. 41, 1656.Google Scholar
[20]Hasegawa, A., Yu, M. Y., Shukla, P. K., and Spatschek, K. H. 1979 Phys. Rev. Lett. 42, 412.CrossRefGoogle Scholar
[21]Key, M. H. 1978 Nature (London) 276, 210.CrossRefGoogle Scholar
[22]Borghesi, M., et al. 1998 Phys. Rev. Lett. 81, 112.CrossRefGoogle Scholar
[23]Tatarakis, M., et al. 2002 Nature (London) 415, 280.Google Scholar
[24]Wagner, U., et al. 2004 Phys. Rev. E 70, 026401.CrossRefGoogle Scholar
[25]Kolb, E. W. and Turner, M. S. 1994 The Early Universe. Reading, MA: Addison-Wesley.Google Scholar
[26]Rye, D., Kang, H., Cho, J. and Das, S. 2008 Science 320, 909.CrossRefGoogle Scholar
[27]Rees, M. 2006 Astron. Nachr. 327, 395.CrossRefGoogle Scholar
[28]Grasso, D. and Rubinstein, H. R. 2001 Phys. Rep. 348, 163.Google Scholar
[29]Widrow, L. M. 2002 Rev. Mod. Phys. 74, 775.CrossRefGoogle Scholar
[30]Kronberg, P. P. 2002 Phys. Today 55, 40.CrossRefGoogle Scholar
[31]Kulsrud, R. M. and Zweibel, E. G. 2008 Rep. Prog. Phys. 71, 046901.Google Scholar
[32]Bernet, M.-L., et al. 2008 Nature (London) 454, 302.CrossRefGoogle Scholar
[33]Glenzer, S. H., et al. 2007 Phys. Rev. Lett. 98, 065002.CrossRefGoogle Scholar
[34]Shukla, P. K. and Eliasson, B. 2007 Phys. Rev. Lett. 99, 096401.Google Scholar
[35]Shaikh, D. and Shukla, P. K. 2007 Phys. Rev. Lett. 99, 125002.CrossRefGoogle Scholar
[36]Marklund, M., et al. 2008 Europhys. Lett. 84, 1706.CrossRefGoogle Scholar
[37]Harding, A. K. and Lai, D. 2006 Rep. Prog. Phys. 69, 2631.CrossRefGoogle Scholar
[38]Chabier, G., et al. 2006 J. Phys. A: Math. Gen. 39, 4411.Google Scholar
[39]Gardner, C. L. and Ringhofer, C. 1996 Phys. Rev. E 53, 157.Google Scholar
[40]Manfredi, G. 2005 Fields Inst. Commun. 46, 263.Google Scholar
[41]Shukla, P. K. and Eliasson, B. 2006 Phys. Rev. Lett. 96, 245001.CrossRefGoogle Scholar
[42]Shukla, P. K. 2006 Phys. Lett. A 352, 242.CrossRefGoogle Scholar
[43]Marklund, M. and Brodin, G. 2007 Phys. Rev. Lett. 98, 025001.CrossRefGoogle Scholar
[44]Brodin, G. and Marklund, M. 2007 Phys. Rev. E 76, 055402.Google Scholar
[45]Brodin, G., et al. 2008 Phys. Rev. Lett. 101, 245002.CrossRefGoogle Scholar
[46]Shukla, P. K. 2009 Nature Phys. 5 92 (2009).CrossRefGoogle Scholar
[47]Stenflo, L. 1971 J. Plasma Phys. 5, 413.CrossRefGoogle Scholar
[48]Piovella, N., et al. 2008 Phys. Rev. Lett. 100, 044801.CrossRefGoogle Scholar
[49]Serbeto, A., Mendonça, J. T., Tsui, K. H. and Bonifacio, R. 2008 Phys. Rev. Lett. 100, 044801.Google Scholar
[50]Shukla, P. K. and Eliasson, B. 2008 Phys. Rev. Lett. 100, 036801.CrossRefGoogle Scholar