2017
DOI: 10.1063/1.4994706
|View full text |Cite
|
Sign up to set email alerts
|

Effects of energetic electrons on ion acceleration in a quasi-static model

Abstract: Based on the Passoni-Lontano model [M. Lontano and M. Passoni, Phys. Plasmas 13(4), 042102 (2006)], the expansion of an intense laser produced plasma into vacuum is analyzed, assuming that hot and energetic electrons responsible for ion acceleration, in the framework of a TNSA mechanism, are nonthermal and modelled by the Cairns distribution function. Due to the presence of energetic nonthermal electron population, the electric potential, electrical field, ion maximum energy, and ion spectrum energy are enhanc… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

0
6
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 7 publications
(6 citation statements)
references
References 39 publications
0
6
0
Order By: Relevance
“…The non-relativistic Cairns distribution function [85] has been proposed to describe the non-thermal electrons in TNSA modelling [86] however its non-relativistic character is an intrinsic limitation as far as hot, relativistic electrons are concerned. Here we make use of a relativistically correct Cairns-like distribution function, namely: 2…”
Section: Role Of Non-thermal Electrons In Tnsamentioning
confidence: 99%
“…The non-relativistic Cairns distribution function [85] has been proposed to describe the non-thermal electrons in TNSA modelling [86] however its non-relativistic character is an intrinsic limitation as far as hot, relativistic electrons are concerned. Here we make use of a relativistically correct Cairns-like distribution function, namely: 2…”
Section: Role Of Non-thermal Electrons In Tnsamentioning
confidence: 99%
“…Here, we choose a Cairns-like distribution function. The Cairns distribution function was first introduced to explain soliton structures observed in cold space plasmas [35] and then employed in a non-relativistic TNSA model [31]. We extend the Cairns distribution function [35] to the relativistic regime, which, in a manifestly covariant form, reads:…”
Section: Non-equilibrium Relativistic Distribution Functionmentioning
confidence: 99%
“…This allows us to interpret α as a knob that moves the distribution function from equilibrium (α = 0) to a higher degree of non-equilibrium (α → ∞). Second, when plugging f α into the sheath model, computations in the non-relativistic [31] and ultra-relativistic limits can be partially carried out analytically. In addition, as we will detail in section 4, f α is consistent with 3D PIC simulations of TNSA.…”
Section: Non-equilibrium Relativistic Distribution Functionmentioning
confidence: 99%
See 2 more Smart Citations