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Electrostatic interactions and stability of dusty plasmas and the multicomponent Ornstein-Zernike equation

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Electrostatic interactions and stability of dusty plasmas and the multicomponent Ornstein-Zernike equation

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dc.contributor.author Tkachenko Gorski, Igor Mijail es_ES
dc.contributor.author Filippov, A.V. es_ES
dc.contributor.author Fortov, Vladimir E. es_ES
dc.contributor.author Reshetniak, V.V. es_ES
dc.contributor.author Starostin, A.N. es_ES
dc.date.accessioned 2023-07-10T18:02:14Z
dc.date.available 2023-07-10T18:02:14Z
dc.date.issued 2020-04 es_ES
dc.identifier.issn 2158-3226 es_ES
dc.identifier.uri http://hdl.handle.net/10251/194766
dc.description.abstract [EN] Using the Ornstein-Zernike integral fluid equation for multi-component plasma, the dielectric properties and thermodynamical stability of dusty plasmas are studied. For the most non-ideal dust plasma subsystem, a transition to the one-component approximation is carried out. It is shown that the effective pseudopotential for determining the correlation functions in the selected subsystem should not include the contribution of this subsystem to the screening constant but also take into account the condition of total plasma quasineutrality. It is demonstrated that when the coupling parameter of the dust subsystem is smaller than unity, Gamma(00) < 1, the interaction potential between the charged plasma particles is fairly well described by the Debye potential with a full screening constant. For Gamma(00) > 1, the static dielectric function in the long wavelength domain becomes negative, and this domain expands when Gamma(00) increases. This leads to the appearance of attraction of particles with charges of the same sign and repulsion of particles with charges of the opposite sign. In this case, both the total pressure and the isothermal compressibility in the entire studied range of the coupling parameter Gamma(00) < 250 remain positive, but the isothermal compressibility of the dust subsystem becomes negative at Gamma(00) approximate to 2 within the studied range of variation of the plasma parameters. The sign of the derivative of the chemical potential with respect to the total number of dust particles, the positiveness of which is the third condition for the thermodynamic stability, is shown to coincide with the sign of the isothermal compressibility of the dust subsystem. Therefore, it is concluded that the equilibrium dusty plasma at Gamma(00) > 2 is thermodynamically unstable. es_ES
dc.description.sponsorship This study was developed within Project No. 16-12-10424 supported by the grant from the Russian Science Foundation, and the numerical simulations were carried out as a part of the State assignment financed by the Ministry of Science and Higher Education of the Russian Federation (Project No. 0038-2019-0005). es_ES
dc.language Inglés es_ES
dc.publisher American Institute of Physics es_ES
dc.relation.ispartof AIP Advances es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Dusty plasmas es_ES
dc.subject Thermodynamics es_ES
dc.subject Stability es_ES
dc.subject.classification MATEMATICA APLICADA es_ES
dc.title Electrostatic interactions and stability of dusty plasmas and the multicomponent Ornstein-Zernike equation es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1063/1.5144901 es_ES
dc.relation.projectID info:eu-repo/grantAgreement/RSF//16-12-10424/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/Ministry of Science and Higher Education of the Russian Federation//0038-2019-0005/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Escuela Técnica Superior de Ingenieros Industriales - Escola Tècnica Superior d'Enginyers Industrials es_ES
dc.description.bibliographicCitation Tkachenko Gorski, IM.; Filippov, A.; Fortov, VE.; Reshetniak, V.; Starostin, A. (2020). Electrostatic interactions and stability of dusty plasmas and the multicomponent Ornstein-Zernike equation. AIP Advances. 10(4):1-14. https://doi.org/10.1063/1.5144901 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1063/1.5144901 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 14 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 10 es_ES
dc.description.issue 4 es_ES
dc.relation.pasarela S\425011 es_ES
dc.contributor.funder Russian Science Foundation es_ES
dc.contributor.funder Ministry of Science and Higher Education of the Russian Federation es_ES


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