<p>This study investigates the nonlinear dynamics and stability of dust-acoustic waves (DAWs) in a magnetized three-component dusty plasma comprising cold negative dust impurities and superthermally distributed cold/hot positive ions. By employing a reductive perturbation technique, a (3+1)-dimensional Zakharov-Kuznetsov (ZK) equation is derived, governing the evolution of compressive solitons. Numerical analyses reveal that the phase velocity of DAWs increases with the spectral indices (<InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq1.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="18" /> </InlineMediaObject> <EquationSource Format="TEX">\( \kappa _{c} \)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>κ</mi> <mi>c</mi> </msub> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq2.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="20" /> </InlineMediaObject> <EquationSource Format="TEX">\( \kappa _{h} \)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>κ</mi> <mi>h</mi> </msub> </math></EquationSource> </InlineEquation>) of cold and hot ions, attributed to reduced Landau damping, but decreases with higher cold-to-hot ion temperature ratios (<InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq3.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\( \theta \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>θ</mi> </math></EquationSource> </InlineEquation>) and density ratios (<InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq4.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="15" /> </InlineMediaObject> <EquationSource Format="TEX">\( \mu \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>μ</mi> </math></EquationSource> </InlineEquation>), due to enhanced ion drag and thermal damping. Solitary wave amplitudes grow with lower <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq4.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="15" /> </InlineMediaObject> <EquationSource Format="TEX">\( \mu \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>μ</mi> </math></EquationSource> </InlineEquation>, <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq3.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\( \theta \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>θ</mi> </math></EquationSource> </InlineEquation>, and <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq1.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="18" /> </InlineMediaObject> <EquationSource Format="TEX">\( \kappa _{c} \)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>κ</mi> <mi>c</mi> </msub> </math></EquationSource> </InlineEquation> while widths broaden with increasing <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq1.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="18" /> </InlineMediaObject> <EquationSource Format="TEX">\( \kappa _{c} \)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>κ</mi> <mi>c</mi> </msub> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq9"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq2.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="20" /> </InlineMediaObject> <EquationSource Format="TEX">\( \kappa _{h} \)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>κ</mi> <mi>h</mi> </msub> </math></EquationSource> </InlineEquation>. The nonlinear term’s negativity confirms compressive solitons, with modulating their energy by the magnetic field strength (<InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq10.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\( \Omega \)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">Ω</mi> </math></EquationSource> </InlineEquation>) and propagation angle (<InlineEquation ID="IEq11"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13538_2025_1799_Article_IEq11.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="12" /> </InlineMediaObject> <EquationSource Format="TEX">\( \delta \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>δ</mi> </math></EquationSource> </InlineEquation>). Instability growth rates escalate with higher electron densities and magnetic gradients, linked to current-driven turbulence. These findings elucidate wave behavior in astrophysical environments (e.g., cometary tails, planetary rings) and laboratory setups, particularly in fusion devices where superthermal particles and magnetic confinement govern plasma stability.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

Nonlinear Dust-Acoustic Solitons and Multidimensional Instabilities in Magnetized Plasmas with Superthermal Ions: A Zakharov-Kuznetsov Framework

  • S. A. Gwaily,
  • Reem Altuijri,
  • Kottakkaran Sooppy Nisar,
  • Abdel-Haleem Abdel-Aty,
  • A. Atteya,
  • Eman Mohammed El-Bayoumi

摘要

This study investigates the nonlinear dynamics and stability of dust-acoustic waves (DAWs) in a magnetized three-component dusty plasma comprising cold negative dust impurities and superthermally distributed cold/hot positive ions. By employing a reductive perturbation technique, a (3+1)-dimensional Zakharov-Kuznetsov (ZK) equation is derived, governing the evolution of compressive solitons. Numerical analyses reveal that the phase velocity of DAWs increases with the spectral indices ( \( \kappa _{c} \) κ c and \( \kappa _{h} \) κ h ) of cold and hot ions, attributed to reduced Landau damping, but decreases with higher cold-to-hot ion temperature ratios ( \( \theta \) θ ) and density ratios ( \( \mu \) μ ), due to enhanced ion drag and thermal damping. Solitary wave amplitudes grow with lower \( \mu \) μ , \( \theta \) θ , and \( \kappa _{c} \) κ c while widths broaden with increasing \( \kappa _{c} \) κ c and \( \kappa _{h} \) κ h . The nonlinear term’s negativity confirms compressive solitons, with modulating their energy by the magnetic field strength ( \( \Omega \) Ω ) and propagation angle ( \( \delta \) δ ). Instability growth rates escalate with higher electron densities and magnetic gradients, linked to current-driven turbulence. These findings elucidate wave behavior in astrophysical environments (e.g., cometary tails, planetary rings) and laboratory setups, particularly in fusion devices where superthermal particles and magnetic confinement govern plasma stability.