• Volume/Page
  • Keyword
  • DOI
  • Citation
  • Advanced
   
 
 
 

Flickr Twitter UniPHY Group iResearch App Facebook

Phys. Plasmas 15, 062107 (2008); doi:10.1063/1.2918673 (9 pages)

Streaming instabilities of intense charged particle beams propagating along a solenoidal magnetic field in a background plasma

Edward A. Startsev, Ronald C. Davidson, and Mikhail Dorf

Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543, USA

View MapView Map

(Received 22 January 2008; accepted 11 April 2008; published online 11 June 2008)

Streaming instabilities of intense charged particle beams propagating along a solenoidal magnetic field in a background plasma are studied analytically and numerically. It is shown that the growth rate of the electromagnetic Weibel instability is modified by a relatively weak solenoidal magnetic field such that ωce>βbωpe, where ωce is the electron gyrofrequency, ωpe is the electron plasma frequency, and βb is the ion-beam velocity relative to the speed of light. Moreover, the Weibel instability is limited to very small propagation angles and long longitudinal wavelengths satisfying k2k2 and c2k2ωpb2ωpi2/(ωpb2+ωpi2), where ωpb and ωpi are the plasma frequencies of the beam ions and the background plasma ions, respectively. For shorter longitudinal wavelengths, the electrostatic lower-hybrid instability becomes dominant. In this paper, the growth rates of various electrostatic beam-plasma instabilities and the electromagnetic Weibel instability are compared, and the space-time development of the modified two-stream instability is studied in detail and compared with numerical simulations.

© 2008 American Institute of Physics

Article Outline

  1. INTRODUCTION
  2. GENERAL DISPERSION RELATION AND THE ELECTROMAGNETIC FILAMENTATION (WEIBEL) INSTABILITY FOR B0 ≠ 0
  3. ELECTROSTATIC MODIFIED TWO-STREAM INSTABILITY
  4. NUMERICAL SOLUTIONS TO DISPERSION RELATIONS
  5. SPACE-TIME DEVELOPMENT OF ELECTROSTATIC MODIFIED TWO-STREAM INSTABILITY
  6. CONCLUSIONS

RELATED DATABASES

To view database links for this article, you need to log in.

KEYWORDS and PACS

PACS

  • 52.35.Qz

    Microinstabilities (ion-acoustic, two-stream, loss-cone, beam-plasma, drift, ion- or electron-cyclotron, etc.)

  • 52.40.Mj

    Particle beam interactions in plasmas

PUBLICATION DATA

ISSN:

1070-664X (print)  
1089-7674 (online)

For access to fully linked references, you need to log in.
    R. C. Davidson and H. Qin, Physics of Intense Charged Particle Beams in High Energy Accelerators (World Scientific, Singapore, 2001), and references therein.

    P. K. Roy, S. S. Yu, E. Henestroza, A. Anders, F. M. Bieniosek, J. Coleman, S. Eylon, W. G. Greenway, M. Leither, B. G. Logan, W. L. Waldron, D. R. Welch, C. Thoma, A. B. Sefkow, E. P. Gilson, P. C. Efthimion, and R. C. Davidson, Phys. Rev. Lett. 95, 234801 (2005).

    E. A. Startsev and R. C. Davidson, Phys. Plasmas 13, 062108 (2006)PHPAEN000013000006062108000001.

    H. Qin, E. A. Startsev, and R. C. Davidson, Phys. Rev. ST Accel. Beams 6, 014401 (2003).

    R. C. Davidson, I. D. Kaganovich, H. Qin, and E. A. Startsev, Phys. Rev. ST Accel. Beams 7, 114801 (2004).

    I. D. Kaganovich, E. A. Startsev, A. B. Sefkow, and R. C. Davidson, Phys. Rev. Lett. 99, 235002 (2007).

    E. S. Weibel, Phys. Rev. Lett. 2, 83 (1959).

    R. C. Davidson, D. A. Hammer, I. Haber, and C. E. Wagner, Phys. Fluids 15, 317 (1972)PFLDAS000015000002000317000001.

    R. Lee and M. Lampe, Phys. Rev. Lett. 31, 1390 (1973).

    C. A. Kapetanakos, Appl. Phys. Lett. 25, 484 (1974)APPLAB000025000009000484000001.

    T. P. Hughes, S. S. Yu, and R. E. Clark, Phys. Rev. ST Accel. Beams 2, 110401 (1999).

    E. A. Startsev and R. C. Davidson, Phys. Plasmas 13, 062108 (2006)PHPAEN000013000006062108000001.

    E. P. Lee, S. Yu, H. L. Buchanan, F. W. Chambers, and M. N. Rosenbluth, Phys. Fluids 23, 2095 (1980)PFLDAS000023000010002095000001.


For access to citing articles, you need to log in.


Figures (6)

Access to article objects (figures, tables, multimedia) requires a subscription; log in to view available files.
(Access to supplementary files, where available, is free for this journal.)



Close
Google Calendar
ADVERTISEMENT

close