Nonlinear electrostatic kelvin-helmholtz shock waves in a viscous electron-positron-ion plasma with non-maxwellian distribution Article Swipe
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· 2023
· Open Access
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· DOI: https://doi.org/10.1088/1402-4896/ad1454
A theoretical investigation is carried out for nonlinear electrostatic Kelvin-Helmholtz (K-H) shock waves in a magnetized electron-positron-ion viscous plasma in the presence of transport equations and non-Maxwellian particles by following the generalized ( r , q ) distribution function. The propagation of electrostatic K-H modes are studied both in the presence of trapped and free electrons. The nonlinear analysis with inclusion of plasma transport properties (magnetic viscosity and heat conduction) lead to nonlinear electrostatic K-H mode in the form of shock like waves by solving the modified Burgers’ equation. The electrostatic K-H shocks are investigated numerically with effect of different plasma parameters such as shear velocity and non-Maxwellian distributed particles. It is observed that the striking features (viz., amplitude and width of dissipative shock through the solution of Burgers’ equation) of the K-H mode are significantly modified by the effects of non-thermality of electrons and positrons both at shoulder and tails along with shear velocity due to viscosity. The relevancy of our work to the observations in space (viz., cometary comae and earth’s ionosphere), astrophysical (viz., pulsars) and laboratory (viz., solid-high intense laser plasma interaction experiments) plasmas is highlighted.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1088/1402-4896/ad1454
- OA Status
- hybrid
- Cited By
- 2
- References
- 59
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- OpenAlex ID
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Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4389540674Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1088/1402-4896/ad1454Digital Object Identifier
- Title
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Nonlinear electrostatic kelvin-helmholtz shock waves in a viscous electron-positron-ion plasma with non-maxwellian distributionWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-12-11Full publication date if available
- Authors
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A. Mushtaq, Zulfiqar Ahmad, M. Farooq, S. UsmanList of authors in order
- Landing page
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https://doi.org/10.1088/1402-4896/ad1454Publisher landing page
- Open access
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YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
- OA URL
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https://doi.org/10.1088/1402-4896/ad1454Direct OA link when available
- Concepts
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Physics, Plasma, Distribution function, Electron, Atomic physics, Shock wave, Dissipative system, Classical mechanics, Mechanics, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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2Total citation count in OpenAlex
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2025: 1, 2024: 1Per-year citation counts (last 5 years)
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59Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.with | 60, 97, 153 |
| abstract_inverted_index.work | 163 |
| abstract_inverted_index.(K-H) | 11 |
| abstract_inverted_index.along | 152 |
| abstract_inverted_index.comae | 171 |
| abstract_inverted_index.laser | 183 |
| abstract_inverted_index.modes | 45 |
| abstract_inverted_index.shear | 105, 154 |
| abstract_inverted_index.shock | 12, 81, 124 |
| abstract_inverted_index.space | 168 |
| abstract_inverted_index.tails | 151 |
| abstract_inverted_index.waves | 13, 83 |
| abstract_inverted_index.width | 121 |
| abstract_inverted_index.(viz., | 118, 169, 176, 180 |
| abstract_inverted_index.effect | 98 |
| abstract_inverted_index.plasma | 19, 63, 101, 184 |
| abstract_inverted_index.shocks | 93 |
| abstract_inverted_index.carried | 5 |
| abstract_inverted_index.effects | 140 |
| abstract_inverted_index.intense | 182 |
| abstract_inverted_index.plasmas | 187 |
| abstract_inverted_index.solving | 85 |
| abstract_inverted_index.studied | 47 |
| abstract_inverted_index.through | 125 |
| abstract_inverted_index.trapped | 53 |
| abstract_inverted_index.viscous | 18 |
| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.analysis | 59 |
| abstract_inverted_index.cometary | 170 |
| abstract_inverted_index.features | 117 |
| abstract_inverted_index.modified | 87, 137 |
| abstract_inverted_index.observed | 113 |
| abstract_inverted_index.presence | 22, 51 |
| abstract_inverted_index.pulsars) | 177 |
| abstract_inverted_index.shoulder | 149 |
| abstract_inverted_index.solution | 127 |
| abstract_inverted_index.striking | 116 |
| abstract_inverted_index.velocity | 106, 155 |
| abstract_inverted_index.(magnetic | 66 |
| abstract_inverted_index.amplitude | 119 |
| abstract_inverted_index.different | 100 |
| abstract_inverted_index.earth’s | 173 |
| abstract_inverted_index.electrons | 144 |
| abstract_inverted_index.equation) | 130 |
| abstract_inverted_index.equation. | 89 |
| abstract_inverted_index.equations | 25 |
| abstract_inverted_index.following | 30 |
| abstract_inverted_index.function. | 39 |
| abstract_inverted_index.inclusion | 61 |
| abstract_inverted_index.nonlinear | 8, 58, 73 |
| abstract_inverted_index.particles | 28 |
| abstract_inverted_index.positrons | 146 |
| abstract_inverted_index.relevancy | 160 |
| abstract_inverted_index.transport | 24, 64 |
| abstract_inverted_index.viscosity | 67 |
| abstract_inverted_index.Burgers’ | 88, 129 |
| abstract_inverted_index.electrons. | 56 |
| abstract_inverted_index.laboratory | 179 |
| abstract_inverted_index.magnetized | 16 |
| abstract_inverted_index.parameters | 102 |
| abstract_inverted_index.particles. | 110 |
| abstract_inverted_index.properties | 65 |
| abstract_inverted_index.solid-high | 181 |
| abstract_inverted_index.viscosity. | 158 |
| abstract_inverted_index.conduction) | 70 |
| abstract_inverted_index.dissipative | 123 |
| abstract_inverted_index.distributed | 109 |
| abstract_inverted_index.generalized | 32 |
| abstract_inverted_index.interaction | 185 |
| abstract_inverted_index.numerically | 96 |
| abstract_inverted_index.propagation | 41 |
| abstract_inverted_index.theoretical | 2 |
| abstract_inverted_index.distribution | 38 |
| abstract_inverted_index.experiments) | 186 |
| abstract_inverted_index.highlighted. | 189 |
| abstract_inverted_index.investigated | 95 |
| abstract_inverted_index.ionosphere), | 174 |
| abstract_inverted_index.observations | 166 |
| abstract_inverted_index.astrophysical | 175 |
| abstract_inverted_index.electrostatic | 9, 43, 74, 91 |
| abstract_inverted_index.investigation | 3 |
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| abstract_inverted_index.non-Maxwellian | 27, 108 |
| abstract_inverted_index.non-thermality | 142 |
| abstract_inverted_index.Kelvin-Helmholtz | 10 |
| abstract_inverted_index.electron-positron-ion | 17 |
| cited_by_percentile_year.max | 95 |
| cited_by_percentile_year.min | 90 |
| corresponding_author_ids | https://openalex.org/A5101970602, https://openalex.org/A5101466143 |
| countries_distinct_count | 1 |
| institutions_distinct_count | 4 |
| corresponding_institution_ids | https://openalex.org/I121243025, https://openalex.org/I181063083 |
| citation_normalized_percentile.value | 0.67903128 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |