Title:
Evolution of shock waves in dusty nonideal gas flow with magnetic field

dc.contributor.authorShweta
dc.contributor.authorPradeep
dc.contributor.authorShobhit Kumar Srivastava
dc.contributor.authorLal Pratap Singh
dc.date.accessioned2026-02-09T04:30:40Z
dc.date.issued2024
dc.description.abstractThis paper deals with the study of propagation of shock waves in 2-D steady supersonic magnetogasdynamics flow of nonideal dusty gas using wavefront analysis method. We derived the transport equation, which determines the condition for the shock formation. Our aim is to analyze the effect of interaction of dust particles with magnetic field in nonideal gas on the evolution of shock formation and to examine how the flow patterns of the disturbance vary with respect to the variations in the physical parameters of the medium. It is found that the presence of magnetic field plays an essential role in the wave propagation phenomena. The nature of the solution with respect to the Mach number is analyzed, and it is examined how the shock formation distance changes with an increase or decrease in the value of Mach number. Also, the combined effect of nonidealness, magnetic field, and dust particles on the shock formation distance is elucidated and examined how the formation of shocks is affected by the increase in the value of corresponding physical parameters. © 2024 Walter de Gruyter GmbH, Berlin/Boston.
dc.identifier.doi10.1515/zna-2023-0254
dc.identifier.issn9320784
dc.identifier.urihttps://doi.org/10.1515/zna-2023-0254
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/48008
dc.publisherWalter de Gruyter GmbH
dc.subjectdusty gas
dc.subjectmagnetic field
dc.subjectnonideal gas
dc.subjectshock wave
dc.titleEvolution of shock waves in dusty nonideal gas flow with magnetic field
dc.typePublication
dspace.entity.typeArticle

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