Abstract
A theoretical investigation has been carried out to examine the evolution of heavy- and light-nuclei acoustic (HLNA) dressed solitons (DSs) due to higher-order contributions of nonlinearity and dispersion effects in a degenerate ultra-relativistic degenerate quantum plasma composed of inertial heavy as well as light nuclei with inertia-less degenerate electrons. The nonlinear Korteweg–de Vries (KdV) equation is derived by using reductive perturbation method. Furthermore, higher-order corrections of nonlinearity and dispersion effects are considered and a linear inhomogeneous KdV-type equation is derived. With the contribution of higher-order effects, a new type of structures with two tails or DSs are formed. The influence of different plasma parameters on the dynamical evolution of the HLNA-DSs is examined. It is observed that insertion of higher-order corrections of nonlinearity and dispersion effects significantly alter the first-order soliton structures into DSs. The findings of present investigation may be applicable to provide a new insight to understand the evolution of HLNA-DSs in different dense astrophysical region.
| Original language | English |
|---|---|
| Pages (from-to) | 3331-3339 |
| Number of pages | 9 |
| Journal | Indian Journal of Physics |
| Volume | 96 |
| Issue number | 11 |
| DOIs | |
| State | Published - Sep 2022 |
| Externally published | Yes |
Funding
RK acknowledges DST, Govt. of India under DST-Purse scheme for financial support. Authors gratefully acknowledge the support for this research work from Department of Science and Technology, Govt. of India, New Delhi, under DST-SERB project No. CRG/2019/003988. RK acknowledges DST, Govt. of India under DST-Purse scheme for financial support. Authors gratefully acknowledge the support for this research work from Department of Science and Technology, Govt. of India, New Delhi, under DST-SERB project No. CRG/2019/003988.
Keywords
- Degenerate electrons
- Heavy and light nuclei
- KdV equation
- Reductive perturbation method
- Solitons
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