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Raj Kumar Anand

Publications and source records attributed to Raj Kumar Anand.

3 recordsLinked to original sources

MHD Rankine-Hugoniot jump conditions for shock waves in van der Waals gases

In this article, we have presented non-relativistic boundary conditions across a magnetohydrodynamic (MHD) shock front propagating in van der Waals gases. The expression for the strength of the non-relativistic MHD shock wave has been obtained, and the Rankine-Hugoniot (R-H) shock jump relations, or boundary conditions, for the pressure, the density, and the particle velocity across an MHD shock front have been derived in terms of a shock compression ratio. The simplified forms of shock jump relations have been written simultaneously for the weak and strong MHD shock waves in terms of the magnetic field strength, the non-idealness parameter, and the ratio of specific heats of the gas. Further, the case of weak shocks has been explored under two distinct conditions, viz., (i) when the applied magnetic field is weak and (ii) when the field is strong, respectively. The case of strong shocks has also been investigated under two distinct ways: (i) as in the purely non-magnetic case, when the ratio of densities on either side of the shock nearly equals $(γ+1)/(γ-1)$ or (ii) when the applied magnetic field is large. This is when the ambient magnetic pressure is large as compared with the ambient gas pressure. Finally, the effects on the shock strength and the pressure across the MHD shock front are studied due to the magnetic field strength and the non-idealness parameter of the gases. This study presents an overview of the influence of the magnetic field strength and the non-idealness parameter on the shock strength, the pressure, the density, and the particle velocity across the MHD shock front in van der Waals gases.

astro-ph.HE

Jump relations for magnetrohydrodynamic shock waves in a dusty gas atmosphere

In this article, we have derived Rankine-Hugoniot (RH) jump conditions across a magnetohydrodynamic (MHD) shock front propagating in a dusty gas atmosphere. The dusty gas atmosphere is assumed to be a mixture of a perfect gas and small solid particles, in which small spherical solid particles are continuously distributed. The non-relativistic RH conditions for the pressure, the density, and the fluid velocity across an MHD shock front have been derived in terms of a compression ratio. The simplified forms of RH conditions have been written simultaneously for the weak and strong MHD shock waves in terms of the initial volume fraction of solid particles, the ratio of specific heats of the mixture, and the strength of the magnetic field. Further, the weak and strong shocks have been explored under two distinct conditions, viz., (i) when the applied magnetic field is weak and (ii) when the field is strong. Finally, the effects on the shock velocity and the pressure across the MHD shock front are studied due to the strength of the magnetic field, the concentration of dust particles in the mixture, and the volumetric parameter. This study presents an overview of the influence of the strength of the magnetic field and the dust loading parameters on the shock velocity, the pressure, the density, and the fluid velocity across the MHD shock front.

astro-ph.HE

On the Jump Conditions for Shock Waves in Condensed Materials

In this article, we have proposed Rankine-Hugoniot (RH) boundary conditions at the normal shock front, which is passing through the condensed material. These RH conditions are quite general, and their convenient forms for the particle velocity, mass density, pressure, and temperature have been presented in terms of the upstream Mach number and the material parameters for the weak and the strong shocks, respectively. Finally, the effects on the mechanical quantities of the shock-compressed materials, e.g., titanium Ti6Al4V, stainless steel 304, aluminum 6061-T6, etc., have been discussed.

cond-mat.mtrl-sci