Ion-acoustic solitons in a relativistic Fermi plasma at finite temperature

TL;DR

This paper investigates ion-acoustic solitons in a relativistic, finite-temperature, multi-component degenerate plasma, revealing different soliton behaviors depending on the thermal energy regime relevant to astrophysical plasmas.

Contribution

It extends the theory of ion-acoustic solitons to relativistic, finite-temperature plasmas, analyzing regimes where previous nonrelativistic models do not apply.

Findings

Both positive and negative potential solitons coexist for 1<1

Only compressive solitons exist for 1>1

Energy of compressive solitons reaches a steady state

Abstract

The theory of ion-acoustic solitons in nonrelativistic fully degenerate plasmas and nonrelativistic and ultra-relativistic degenerate plasmas at low temperatures is known. We consider a multi-component relativistic degenerate electron-positron-ion plasma at finite temperatures. Specifically, we focus on the intermediate region where the particle's thermal energy $(k_BT)$ and the rest-mass energy $(mc^2)$ do not differ significantly, i.e., $k_BT\sim mc^2$. However, the Fermi energy $(k_BT_F)$ is larger than the thermal energy and the normalized chemical energy ($\xi=\mu/k_BT$) is positive and finite. Two different parameter regimes with $\beta\equiv k_BT/mc^2<1$ and $\beta>1$, relevant for astrophysical plasmas, are defined, and the existence of small amplitude ion-acoustic solitons in these regimes are studied, including the critical cases where the known KdV (Korteweg-de Vries) theory fails. We show that while the solitons with both the positive (compressive) and negative (rarefactive) potentials coexist in the case of $\beta<1$, only compressive solitons can exist in the other regime $(\beta>1)$. Furthermore, while the rarefactive solitons within the parameter domains of $\beta$ and $\xi$ can evolve with increasing amplitude and hence increasing energy, the energy of compressive solitons reaches a steady state.