Abstract
Expansion of cylindrical shocks pushed out through a dynamic piston via rotating perfect dust-pervade gas in the presence of spatially diminishing magnetic field is inquired. The velocity and magnetic field are presumed to comply with power rules. The gas should be conducting electrically. The shock wave proceeds by mutable velocity as well as the total energy being non-stationary. Numerical calculations are accomplished to access the flow variable’s profiles. It is also assessed as to how the magnetic field affects the behaviour of the flow parameters. Further, it’s far exciting to word that in attendance of an azimuthal magnetic field the density and pressure evanesce at expansive region and therefore void is constituted at the symmetry’s axis, that’s in great accordance with laboratory situations to generate shock-wave.
Keywords
- Magnetic field
- Perfect dust-pervade gas
- Rotating medium
- Adiabatic and isothermal flows
- Mechanics of fluids
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References
Hartmann, L.: Accretion Processes in Star Formation. Cambridge University Press, Cambridge (1998)
Balick, B., Frank, A.: Shapes and shaping of planetary nebulae. Ann. Rev. Astron. Astrophys. 40(1), 439–486 (2002)
Nath, G.: Magnetogasdynamic shock wave generated by a moving piston in a rotational axisymmetric isothermal flow of perfect gas with variable density. Adv. Space Res. 47(9), 1463–1471 (2011)
Nath, G., Sahu, P.K.: Flow behind an exponential shock wave in a rotational axisymmetric perfect gas with magnetic field and variable density. SpringerPlus 5(1), 1–18 (2016)
Nath, G., Sahu, P.K., Chaurasia, S.: Modelling. Measur. Control B 87(4), 236–243 (2018)
Nath, G., Sahu, P.K., Chaurasia, S.: Self-similar solution for the flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with magnetic field. Chin. J. Phys. 58, 280–293 (2019)
Sahu, P.K.: Shock wave driven out by a piston in a mixture of a non-ideal gas and small solid particles under the influence of azimuthal or axial magnetic field. Braz. J. Phys. 50(5), 548–565 (2020)
Sahu, P.K.: Magnetogasdynamic exponential shock wave in a self-gravitating, rotational axisymmetric non-ideal gas under the influence of heat-conduction and radiation heat-flux. Ricerche di Matematica 1–37 (2021)
Sahu, P.K.: The influence of magnetic and gravitational fields in a non-ideal dusty gas with heat conduction and radiation heat flux. Indian J. Phys. 1–15 (2022)
Verma, M.K.: Statistical theory of magnetohydrodynamic turbulence: recent results. Phys. Rep. 401(5–6), 229–380 (2004)
Levin, V.A., Skopina, G.A.: Detonation wave propagation in rotational gas flows. J. Appl. Mech. Tech. Phys. 45(4), 457–460 (2004)
Nath, G.: Self-similar solution of cylindrical shock wave propagation in a rotational axisymmetric mixture of a non-ideal gas and small solid particles. Meccanica 47(7), 1797–1814 (2012)
Nath, G., Sahu, P.K., Dutta, M.: Magnetohydrodynamic cylindrical shock in a rotational axisymmetric non-ideal gas under the action of monochromatic radiation. Proc. Eng. 127, 1126–1133 (2015)
Nath, G., Sahu, P.K.: Unsteady adiabatic flow behind a cylindrical shock in a rotational axisymmetric non-ideal gas under the action of monochromatic radiation. Proc. Eng. 144, 1226–1233 (2016)
Nath, G., Sahu, P.K.: Flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with conduction and radiation heat flux. Int. J. Appl. Comput. Math. 3(4), 2785–2801 (2017)
Nath, G., Sahu, P.K.: Similarity solution for the flow behind a cylindrical shock wave in a rotational axisymmetric gas with magnetic field and monochromatic radiation. Ain Shams Eng. J. 9(4), 1151–1159 (2018)
Sahu, P.K.: Propagation of an exponential shock wave in a rotational axisymmetric isothermal or adiabatic flow of a self-gravitating non-ideal gas under the influence of axial or azimuthal magnetic field. Chaos Solitons Fractals 135, 109739 (2020)
Sahu, P.K.: Shock wave propagation in perfectly conducting rotational axisymmetric two-phase medium with increasing energy under the action of heat conduction and radiation heat flux. Chin. J. Phys. 72, 176–190 (2021)
Sahu, P.K.: Flow behind the magnetogasdynamical cylindrical shock wave in rotating non-ideal dusty gas with monochromatic radiation. Plasma Res. Exp. 3(4), 045004 (2021)
Pai, S.I., Menon, S., Fan, Z.Q.: Similarity solutions of a strong shock wave propagation in a mixture of a gas and dusty particles. Int. J. Eng. Sci. 18(12), 1365–1373 (1980)
Higashino, F., Suzuki, T.: The effect of particles on blast waves in a dusty gas. Zeitschrift für Naturforschung A 35(12), 1330–1336 (1980)
Miura, H., Glass, I.I.: Proc. R. Soc. Lond. A. Math. Phys. Sci. 397, 295–309 (1985)
Popel, S.I., Gisko, A.A.: Nonlinear Process. Geophys. 13, 223–229 (2006)
Pai, S.I.: Two-Phase Flows, vol. 3. Springer (2013)
Nath, G., Sahu, P.K.: Self-similar solution of a cylindrical shock wave under the action of monochromatic radiation in a rotational axisymmetric dusty gas. Commun. Theor. Phys. 67(3), 327 (2017)
Nath, G., Sahu, P.K.: Propagation of a cylindrical shock wave in a mixture of a non-ideal gas and small solid particles under the action of monochromatic radiation. Combust. Explos. Shock Waves 53(3), 298–308 (2017)
Sahu, P.K.: Self-similar solution of spherical shock wave propagation in a mixture of a gas and small solid particles with increasing energy under the influence of gravitational field and monochromatic radiation. Commun. Theor. Phys. 70(2), 197 (2018)
Sahu, P.K.: Analysis of magnetogasdynamic spherical shock wave in dusty real gas with gravitational field and monochromatic radiation. Eur. Phys. J. Plus 136(4), 1–19 (2021)
Sedov, L.I.: Similarity and dimensional methods in mechanics. Academic Press, New York (1959)
Laumbach, D.D., Probstein, R.F.: Self-similar strong shocks with radiation in a decreasing exponential atmosphere. Phys. Fluids 13(5), 1178–1183 (1970)
Vishwakarma, J.P., Pandey, S.N.: Propagation of strong spherical shock waves in a dusty gas. Phys. Scripta 68(4), 259 (2003)
Steiner, H., Hirschler, T.: A self-similar solution of a shock propagation in a dusty gas. Eur. J. Mech. B Fluids 21(3), 371–380 (2002)
Zel’Dovich, Y.B., Raizer, Y.P.: Physics of shock waves and high-temperature hydrodynamic phenomena. Courier Corporation (2002)
Freeman, R.A., Craggs, J.D.: Shock waves from spark discharges. J. Phys. D Appl. Phys. 2(3), 421 (1969)
Sahu, P.K.: Similarity solution for a spherical shock wave in a non-ideal gas under the influence of gravitational field and monochromatic radiation with increasing energy. Math. Methods Appl. Sci. 42(14), 4734–4746 (2019)
Sahu, P.K.: Similarity solution for the flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas under the influence of gravitational field with conductive and radiative heat fluxes. In: International Conference on Innovation in Modern Science and Technology, pp. 1060-1070. Springer, Cham (2019)
Sahu, P.K.: Unsteady flow behind an MHD exponential shock wave in a rotational axisymmetric non-ideal gas with conductive and radiative heat fluxes. In: International Conference on Innovation in Modern Science and Technology, pp. 1049–1059. Springer, Cham (2019)
Acknowledgements
The author is thankful to Prof. M. K. Verma, Department of Physics, Indian Institute of Technology Kanpur, Kanpur–208016, India for fruitful discussions. This work was supported by the research grant no. TAR/2018/000150 under Teachers Associateship for Research Excellence (TARE) scheme from the Science and Engineering Research Board (SERB), India. The author gracefully acknowledges financial support from SERB.
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Sahu, P.K. (2022). Motion of Adiabatic or Isothermal Flow Headed by a Magnetogasdynamic Cylindrical Shock Through Rotating Dusty Gas. In: Banerjee, S., Saha, A. (eds) Nonlinear Dynamics and Applications. Springer Proceedings in Complexity. Springer, Cham. https://doi.org/10.1007/978-3-030-99792-2_7
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