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A magnetically tapered plasma density for overcoming electron dephasing

Published online by Cambridge University Press:  30 September 2011

C. M. WANG*
Affiliation:
School of Mechanical and Automotive Engineering, Hefei University of Technology, Postcode 230009, Hefei, China ([email protected])

Abstract

One of the main limitations of energy gain in laser wakefield accelerators is the electron dephasing, In order to resolve the dephasing problem, a tapered plasma channel is proposed and tested numerically. The tapered density is created by means of a laser heating, combining an axially increased external magnetic field. The locally strong magnetic field prevents the thermal energy transport crossing the field lines, and leads to a pressure buildup. The pressure gradient expels the plasma radially and tapers the density axially. A tapered plasma with a density contrast of 2.2 within a 6-cm channel is established. Propagating in the tapered plasma channel, the energy of an accelerated electron is expected to be enhanced greatly.

Type
Papers
Copyright
Copyright © Cambridge University Press 2011

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References

[1]Taijma, T. and Dawson, J. 1979 Phys. Rev. Lett. 43, 267.CrossRefGoogle Scholar
[2]Modena, A. et al. . 1995 Nature 377, 606.CrossRefGoogle Scholar
[3]Umstadter, D., Chen, S. Y., Maksimchuk, A., Mourou, G. and Wagner, R. 1996 Science 273, 472.CrossRefGoogle Scholar
[4]Moore, C. I., Ting, A., Krushelnick, K., Esarey, E., Hubbard, R. F., Hafizi, B., Burris, H. R., Manka, C. and Sprangle, P. 1997 Phys. Rev. Lett. 79, 3909.CrossRefGoogle Scholar
[5]Malka, V., Fritzler, S., Lefebvre, E., Aleonard, M. M., Burgy, F., Cambaret, J. P., Chemin, J. F., Krushelnick, K., Malka, G., Mangles, S. P. D. 2002 Science 298, 1596.CrossRefGoogle Scholar
[6]Katsouleas, T., 1986 Phys. Rev. A 33, 2056.CrossRefGoogle Scholar
[7]Sprangle, P., Penano, J. R., Hafizi, B., Hubbard, R. F., Ting, A., Zigler, A. and Antonsen, T. M. 2002 Phys. Plasma 9, 2364.CrossRefGoogle Scholar
[8]Spence, D. J. and Hooker, S. M. 2000 Phys. Rev. E 63, 015401.Google Scholar
[9]Junck, K. L. and Getty, W. D. 1994 J. Vac. Sci. Technol. A 12, 2767.CrossRefGoogle Scholar
[10]Froula, D. H. et al. . 2007 Phys. Rev. Lett. 98, 135001.CrossRefGoogle Scholar
[11]Goedbloed, H. and Poedts, S. 2004 Principles of Magnetohydrodynamics. Cambridge, UK: Cambridge University Press.CrossRefGoogle Scholar
[12]Duston, D. and Duderstadt, J. J. 1978 Phys. Rev. A 18, 1707.CrossRefGoogle Scholar
[13]Toth, G. and Odstrcil, D. 1996 J. Comput. Phys. 128, 82.CrossRefGoogle Scholar