Skip to main content
Log in

Ion-acoustic solitons in pair-ion plasma with non-thermal electrons

  • Original Article
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

Properties of fully nonlinear ion-acoustic solitary waves in an unmagnetized and collisionless pair-ion (PI) plasma containing superthermal electrons obeying Cairns distribution have been analyzed. A linear biquadratic dispersion relation has been derived, which yields the fast (supersonic) and slow (subsonic) modes in a pair-ion-electron plasma with nonthermal electrons. For nonlinear analysis, Korteweg-de Vries equation is obtained using the reductive perturbation technique. It is found that in case of slow mode, both electrostatic hump and dip type structures are formed depending on the temperature difference between positively and negatively charged ions, whereas, only dip type solitary structures have been observed for fast mode. The present work may be employed to explore and to understand the formation of solitary structures in the space (especially, the Earth’s ionosphere where two distinct pair ion species (H ±) are present) and laboratory produced pair-ion plasmas with nonthermal electrons.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2a
Fig. 2b
Fig. 3a
Fig. 3b
Fig. 4a
Fig. 4b
Fig. 5a
Fig. 5b
Fig. 6a
Fig. 6b
Fig. 6c
Fig. 7a
Fig. 7b

Similar content being viewed by others

References

Download references

Acknowledgements

This research work was partially supported by the Quaid-i-Azam University Research Fund (URF) Project (2011–2012). One of us (T.A. Khan) thanks HEC, Islamabad, Pakistan for the financial support under Indigenous Ph.D. 5000 Fellowship Program, Phase-V.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Arshad M. Mirza.

Appendix

Appendix

The linear dispersion relation (Eq. (11)) can also be derived by Fourier analysis by using the normalized perturbed quantities up to first order (\(n_{s}=1+n_{s}^{(1)}\), \(v_{s}=v_{s}^{(1)}\), φ=φ (1)) in Eq. (7). After substitution, the linearized system of equations is

$$ \partial_{x}^{2}\varphi^{(1)}=p\varGamma\varphi ^{(1)}+(1-p)n_{-}^{(1)}-n_{+}^{(1)}, $$

where \(n_{s}^{(1)},v_{s}^{(1)}\), φ (1) are the first order perturbations. Assuming \(n_{s}^{(1)},\varphi^{(1)}\sim e^{i(kx-\omega t)}\) where k (wave number) and ω (wave frequency) are normalized by \(\lambda_{D+}^{-1}\) and ω p+ and x, t by λ D+, \(\omega_{p+}^{-1}\), respectively, after eliminating \(v_{s}^{(1)}\) and solving the above system of equations gives the following dispersion relation

$$ \bigl( p\varGamma+k^{2} \bigr) -\frac{1-p}{\lambda^{2}-\sigma\delta }-\frac{1}{\lambda^{2}-\sigma}=0 $$

with λ 2=ω 2/k 2. In the long wavelength limit, the dispersion relation reduces to

$$ p\varGamma-\frac{1-p}{\lambda^{2}-\sigma\delta}-\frac{1}{\lambda ^{2}-\sigma}=0 $$

or it can be rearranged to Eq. (11),

Rights and permissions

Reprints and permissions

About this article

Cite this article

Jilani, K., Mirza, A.M. & Khan, T.A. Ion-acoustic solitons in pair-ion plasma with non-thermal electrons. Astrophys Space Sci 344, 135–143 (2013). https://doi.org/10.1007/s10509-012-1309-x

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s10509-012-1309-x

Keywords

Navigation