Dust-Acoustic Solitary Waves in an Electron-Depleted Nonthermal Magnetized Plasma
A three-component electron-depleted magnetized plasma containing positive dust, negative dust, and kappa nonthermal ions is considered, and the linear and nonlinear properties of dust-acoustic waves (DAWs) are analyzed. A nonlinear Zakharov-Kuznetsov (ZK) equation is derived by applying the reductiv...
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description | A three-component electron-depleted magnetized plasma containing positive dust, negative dust, and kappa nonthermal ions is considered, and the linear and nonlinear properties of dust-acoustic waves (DAWs) are analyzed. A nonlinear Zakharov-Kuznetsov (ZK) equation is derived by applying the reductive perturbation method, and the solitary wave solution of the ZK equation is obtained to investigate the characteristics of dust-acoustic solitary waves (DASWs). The significant impacts of the plasma parameters [such as ion-to-negative dust density ratio ( \mu ), nonthermal parameter ( \kappa ), external magnetic field (expressed via \Omega ), adiabatic index ( \gamma ), and obliqueness angle ( \delta )] on DASWs are observed, and the polarity of DASWs is predicted to change due to the variation of ion-to-negative dust density ratio, that is, both the positive and negative polarity solitary structures may form due to the variation of the ion-to-negative dust density ratio. The existence of periodic and solitary wave solutions is also analyzed via the bifurcation analysis. The results that are investigated in the present study could be beneficial in explaining the propagation nature of low-frequency nonlinear structures in astrophysical plasma environments (viz., Saturn's F-ring, the magnetosphere of Jupiter, upper mesosphere, cometary tail, etc.) and laboratory experiments where electron-depleted magnetized dusty plasma exists. |
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R. ; Sultana, S. ; Mannan, A. ; Mamun, A. A.</creator><creatorcontrib>Habib, K. ; Hassan, M. R. ; Sultana, S. ; Mannan, A. ; Mamun, A. A.</creatorcontrib><description><![CDATA[A three-component electron-depleted magnetized plasma containing positive dust, negative dust, and kappa nonthermal ions is considered, and the linear and nonlinear properties of dust-acoustic waves (DAWs) are analyzed. A nonlinear Zakharov-Kuznetsov (ZK) equation is derived by applying the reductive perturbation method, and the solitary wave solution of the ZK equation is obtained to investigate the characteristics of dust-acoustic solitary waves (DASWs). The significant impacts of the plasma parameters [such as ion-to-negative dust density ratio (<inline-formula> <tex-math notation="LaTeX">\mu </tex-math></inline-formula>), nonthermal parameter (<inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>), external magnetic field (expressed via <inline-formula> <tex-math notation="LaTeX">\Omega </tex-math></inline-formula>), adiabatic index (<inline-formula> <tex-math notation="LaTeX">\gamma </tex-math></inline-formula>), and obliqueness angle (<inline-formula> <tex-math notation="LaTeX">\delta </tex-math></inline-formula>)] on DASWs are observed, and the polarity of DASWs is predicted to change due to the variation of ion-to-negative dust density ratio, that is, both the positive and negative polarity solitary structures may form due to the variation of the ion-to-negative dust density ratio. The existence of periodic and solitary wave solutions is also analyzed via the bifurcation analysis. The results that are investigated in the present study could be beneficial in explaining the propagation nature of low-frequency nonlinear structures in astrophysical plasma environments (viz., Saturn's F-ring, the magnetosphere of Jupiter, upper mesosphere, cometary tail, etc.) and laboratory experiments where electron-depleted magnetized dusty plasma exists.]]></description><identifier>ISSN: 0093-3813</identifier><identifier>EISSN: 1939-9375</identifier><identifier>DOI: 10.1109/TPS.2023.3308119</identifier><identifier>CODEN: ITPSBD</identifier><language>eng</language><publisher>New York: IEEE</publisher><subject>Acoustic properties ; Acoustic waves ; Acoustics ; Bifurcation analysis ; Comet tails ; Density ratio ; Depletion ; Dust ; dust-acoustic solitary waves (DASWs) ; Dusty plasmas ; electron-depleted plasma ; Fluids ; Formulas (mathematics) ; Ions ; kappa nonthermal ions ; Magnetic fields ; Magnetosphere ; Mesosphere ; Obliqueness ; opposite polarity dust ; Parameters ; Perturbation methods ; Planetary magnetospheres ; Plasma ; Plasma temperature ; Plasmas ; Polarity ; Solitary waves ; Zakharov–Kuznetsov (ZK) equation</subject><ispartof>IEEE transactions on plasma science, 2023-10, Vol.51 (10), p.3221-3233</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) 2023</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c334t-7cd45f8f0d4b622320e4f5d8560cd364898e86808d580e758678134f834850b73</citedby><cites>FETCH-LOGICAL-c334t-7cd45f8f0d4b622320e4f5d8560cd364898e86808d580e758678134f834850b73</cites><orcidid>0000-0003-3449-7716 ; 0000-0002-8879-8891 ; 0000-0002-5585-0358 ; 0000-0002-2536-3954</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/10251789$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>314,780,784,796,27924,27925,54758</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/10251789$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc></links><search><creatorcontrib>Habib, K.</creatorcontrib><creatorcontrib>Hassan, M. R.</creatorcontrib><creatorcontrib>Sultana, S.</creatorcontrib><creatorcontrib>Mannan, A.</creatorcontrib><creatorcontrib>Mamun, A. A.</creatorcontrib><title>Dust-Acoustic Solitary Waves in an Electron-Depleted Nonthermal Magnetized Plasma</title><title>IEEE transactions on plasma science</title><addtitle>TPS</addtitle><description><![CDATA[A three-component electron-depleted magnetized plasma containing positive dust, negative dust, and kappa nonthermal ions is considered, and the linear and nonlinear properties of dust-acoustic waves (DAWs) are analyzed. A nonlinear Zakharov-Kuznetsov (ZK) equation is derived by applying the reductive perturbation method, and the solitary wave solution of the ZK equation is obtained to investigate the characteristics of dust-acoustic solitary waves (DASWs). The significant impacts of the plasma parameters [such as ion-to-negative dust density ratio (<inline-formula> <tex-math notation="LaTeX">\mu </tex-math></inline-formula>), nonthermal parameter (<inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>), external magnetic field (expressed via <inline-formula> <tex-math notation="LaTeX">\Omega </tex-math></inline-formula>), adiabatic index (<inline-formula> <tex-math notation="LaTeX">\gamma </tex-math></inline-formula>), and obliqueness angle (<inline-formula> <tex-math notation="LaTeX">\delta </tex-math></inline-formula>)] on DASWs are observed, and the polarity of DASWs is predicted to change due to the variation of ion-to-negative dust density ratio, that is, both the positive and negative polarity solitary structures may form due to the variation of the ion-to-negative dust density ratio. The existence of periodic and solitary wave solutions is also analyzed via the bifurcation analysis. The results that are investigated in the present study could be beneficial in explaining the propagation nature of low-frequency nonlinear structures in astrophysical plasma environments (viz., Saturn's F-ring, the magnetosphere of Jupiter, upper mesosphere, cometary tail, etc.) and laboratory experiments where electron-depleted magnetized dusty plasma exists.]]></description><subject>Acoustic properties</subject><subject>Acoustic waves</subject><subject>Acoustics</subject><subject>Bifurcation analysis</subject><subject>Comet tails</subject><subject>Density ratio</subject><subject>Depletion</subject><subject>Dust</subject><subject>dust-acoustic solitary waves (DASWs)</subject><subject>Dusty plasmas</subject><subject>electron-depleted plasma</subject><subject>Fluids</subject><subject>Formulas (mathematics)</subject><subject>Ions</subject><subject>kappa nonthermal ions</subject><subject>Magnetic fields</subject><subject>Magnetosphere</subject><subject>Mesosphere</subject><subject>Obliqueness</subject><subject>opposite polarity dust</subject><subject>Parameters</subject><subject>Perturbation methods</subject><subject>Planetary magnetospheres</subject><subject>Plasma</subject><subject>Plasma temperature</subject><subject>Plasmas</subject><subject>Polarity</subject><subject>Solitary waves</subject><subject>Zakharov–Kuznetsov (ZK) equation</subject><issn>0093-3813</issn><issn>1939-9375</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>RIE</sourceid><recordid>eNpNkM1Lw0AQxRdRsFbvHjwEPKfOfiW7x9IPFapWWvG4bJOJpqRJ3d0K-te7pT14ejC8NzPvR8g1hQGloO-W88WAAeMDzkFRqk9Ij2quU81zeUp6AJqnXFF-Ti68XwNQIYH1yOt450M6LLoodZEsuqYO1v0k7_YbfVK3iW2TSYNFcF2bjnHbYMAyee7a8IluY5vkyX60GOrfOJ031m_sJTmrbOPx6qh98jadLEcP6ezl_nE0nKUF5yKkeVEKWakKSrHKGOMMUFSyVDKDouSZUFqhyhSoUirAXKosj9-LSnGhJKxy3ie3h71b133t0Aez7naujScNU5oCQA4QXXBwFa7z3mFltq7exIaGgtmDMxGc2YMzR3AxcnOI1Ij4z84kzZXmf2CqZ_Y</recordid><startdate>20231001</startdate><enddate>20231001</enddate><creator>Habib, K.</creator><creator>Hassan, M. R.</creator><creator>Sultana, S.</creator><creator>Mannan, A.</creator><creator>Mamun, A. A.</creator><general>IEEE</general><general>The Institute of Electrical and Electronics Engineers, Inc. (IEEE)</general><scope>97E</scope><scope>RIA</scope><scope>RIE</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-3449-7716</orcidid><orcidid>https://orcid.org/0000-0002-8879-8891</orcidid><orcidid>https://orcid.org/0000-0002-5585-0358</orcidid><orcidid>https://orcid.org/0000-0002-2536-3954</orcidid></search><sort><creationdate>20231001</creationdate><title>Dust-Acoustic Solitary Waves in an Electron-Depleted Nonthermal Magnetized Plasma</title><author>Habib, K. ; Hassan, M. R. ; Sultana, S. ; Mannan, A. ; Mamun, A. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c334t-7cd45f8f0d4b622320e4f5d8560cd364898e86808d580e758678134f834850b73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Acoustic properties</topic><topic>Acoustic waves</topic><topic>Acoustics</topic><topic>Bifurcation analysis</topic><topic>Comet tails</topic><topic>Density ratio</topic><topic>Depletion</topic><topic>Dust</topic><topic>dust-acoustic solitary waves (DASWs)</topic><topic>Dusty plasmas</topic><topic>electron-depleted plasma</topic><topic>Fluids</topic><topic>Formulas (mathematics)</topic><topic>Ions</topic><topic>kappa nonthermal ions</topic><topic>Magnetic fields</topic><topic>Magnetosphere</topic><topic>Mesosphere</topic><topic>Obliqueness</topic><topic>opposite polarity dust</topic><topic>Parameters</topic><topic>Perturbation methods</topic><topic>Planetary magnetospheres</topic><topic>Plasma</topic><topic>Plasma temperature</topic><topic>Plasmas</topic><topic>Polarity</topic><topic>Solitary waves</topic><topic>Zakharov–Kuznetsov (ZK) equation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Habib, K.</creatorcontrib><creatorcontrib>Hassan, M. R.</creatorcontrib><creatorcontrib>Sultana, S.</creatorcontrib><creatorcontrib>Mannan, A.</creatorcontrib><creatorcontrib>Mamun, A. A.</creatorcontrib><collection>IEEE All-Society Periodicals Package (ASPP) 2005-present</collection><collection>IEEE All-Society Periodicals Package (ASPP) 1998-Present</collection><collection>IEEE Electronic Library (IEL)</collection><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>IEEE transactions on plasma science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Habib, K.</au><au>Hassan, M. R.</au><au>Sultana, S.</au><au>Mannan, A.</au><au>Mamun, A. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dust-Acoustic Solitary Waves in an Electron-Depleted Nonthermal Magnetized Plasma</atitle><jtitle>IEEE transactions on plasma science</jtitle><stitle>TPS</stitle><date>2023-10-01</date><risdate>2023</risdate><volume>51</volume><issue>10</issue><spage>3221</spage><epage>3233</epage><pages>3221-3233</pages><issn>0093-3813</issn><eissn>1939-9375</eissn><coden>ITPSBD</coden><abstract><![CDATA[A three-component electron-depleted magnetized plasma containing positive dust, negative dust, and kappa nonthermal ions is considered, and the linear and nonlinear properties of dust-acoustic waves (DAWs) are analyzed. A nonlinear Zakharov-Kuznetsov (ZK) equation is derived by applying the reductive perturbation method, and the solitary wave solution of the ZK equation is obtained to investigate the characteristics of dust-acoustic solitary waves (DASWs). The significant impacts of the plasma parameters [such as ion-to-negative dust density ratio (<inline-formula> <tex-math notation="LaTeX">\mu </tex-math></inline-formula>), nonthermal parameter (<inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>), external magnetic field (expressed via <inline-formula> <tex-math notation="LaTeX">\Omega </tex-math></inline-formula>), adiabatic index (<inline-formula> <tex-math notation="LaTeX">\gamma </tex-math></inline-formula>), and obliqueness angle (<inline-formula> <tex-math notation="LaTeX">\delta </tex-math></inline-formula>)] on DASWs are observed, and the polarity of DASWs is predicted to change due to the variation of ion-to-negative dust density ratio, that is, both the positive and negative polarity solitary structures may form due to the variation of the ion-to-negative dust density ratio. The existence of periodic and solitary wave solutions is also analyzed via the bifurcation analysis. The results that are investigated in the present study could be beneficial in explaining the propagation nature of low-frequency nonlinear structures in astrophysical plasma environments (viz., Saturn's F-ring, the magnetosphere of Jupiter, upper mesosphere, cometary tail, etc.) and laboratory experiments where electron-depleted magnetized dusty plasma exists.]]></abstract><cop>New York</cop><pub>IEEE</pub><doi>10.1109/TPS.2023.3308119</doi><tpages>13</tpages><orcidid>https://orcid.org/0000-0003-3449-7716</orcidid><orcidid>https://orcid.org/0000-0002-8879-8891</orcidid><orcidid>https://orcid.org/0000-0002-5585-0358</orcidid><orcidid>https://orcid.org/0000-0002-2536-3954</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Acoustic properties Acoustic waves Acoustics Bifurcation analysis Comet tails Density ratio Depletion Dust dust-acoustic solitary waves (DASWs) Dusty plasmas electron-depleted plasma Fluids Formulas (mathematics) Ions kappa nonthermal ions Magnetic fields Magnetosphere Mesosphere Obliqueness opposite polarity dust Parameters Perturbation methods Planetary magnetospheres Plasma Plasma temperature Plasmas Polarity Solitary waves Zakharov–Kuznetsov (ZK) equation |
title | Dust-Acoustic Solitary Waves in an Electron-Depleted Nonthermal Magnetized Plasma |
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