International Journal on Science and Technology

E-ISSN: 2229-7677   •   Impact Factor: 9.88

A Widely Indexed Open Access Peer Reviewed Multidisciplinary Bi-monthly Scholarly International Journal

Call for Paper Volume 16 Issue 3 July-September 2025 Submit your research before last 3 days of September to publish your research paper in the issue of July-September.
Submit Research Paper Join as a Reviewer

Plagiarism is checked by the leading plagiarism checker TurnItIn

Call for Paper

Volume 16 Issue 3
July-September 2025

Submit your research paper

Indexing Partners
Academia Advanced Sciences Index Bielefeld Academic Search Engine CiteSeer DRJI Google Scholar Independent Search Engine & Directory Network ISI (International Scientific Indexing) Issuu Mendeley Research Networks
RefSeek ResearcherId - Thomson Reuters ResearchGate Scirus Scribd Semantic Scholar UTeM - Universiti Teknikal Malaysia Melaka Wiki for Call for Papers WorldCat Zenodo

Self-similar dynamics of a cylindrical shock wave in a rotating, self-gravitating dusty gas under monochromatic radiation

Author(s) Gyanendra Kumar Chaudhary, Arvind Kumar Singh
Country India
Abstract The study explores the propagation of a cylindrical shock wave in a self-gravitating, rotat- ing axisymmetric dusty gas subjected to monochromatic radiation of constant intensity per unit area. The gas is considered grey and opaque, while the shock wave itself is transparent. The fluid velocity has variable azimuthal and axial components. The dusty gas is modeled as a mixture of a non-ideal gas and small solid particles, which are continuously distributed throughout. To capture key characteristics of shock propagation, the solid particles are treated as a pseudo-fluid, ensuring that equilibrium flow conditions are maintained across the entire flow field. Similarity solutions are derived, and the influence of various parame- ters—such as radiation, gravitation, gas non-idealness, mass concentration of solid particles, and the density ratio of solid particles to the initial gas density—is analyzed in detail. The similarity solution holds under the assumption of a constant initial angular velocity, and it is observed that shock strength remains unaffected by both the radiation and gravitation parameters. Additionally, the radiation parameter plays a dominant role in governing the effect of dusty gas parameters on radiation heat flux variation. Furthermore, the total en- ergy in the flow field behind the shock front is not conserved but instead varies as the fourth power of the shock radius.
Keywords Cylindrical shock wave, Dusty gas dynamics, Monochromatic radiation, Similarity solutions, Non-ideal gas.
Field Mathematics
Published In Volume 16, Issue 2, April-June 2025
Published On 2025-04-13
DOI https://doi.org/10.71097/IJSAT.v16.i2.3405
Short DOI https://doi.org/g9fmw6
View / Download PDF File

Share this


CrossRef

CrossRef DOI is assigned to each research paper published in our journal.

IJSAT DOI prefix is
10.71097/IJSAT

Downloads
Research Paper Format Copyright Permission Form and Undertaking Form Cover Page Vol 16 Isu 3Cover Page Vol 16 Isu 2Cover Page Vol 16 Isu 1

All research papers published on this website are licensed under Creative Commons Attribution-ShareAlike 4.0 International License, and all rights belong to their respective authors/researchers.

CC-BY-SA Open Access

About IJSAT
Fees & Payment
Current Issue
Publication Archive 		Submit Research Paper
Track Submission Status
Publication Guidelines
Publication Ethics
Peer Review & Plagiarism 		Join as a Reviewer
Editors & Reviewers
Reviewer Referral Program
Get Reviewer Membership Certi. 		Website/Journal Policies
Usage Policy
Content Policies
Privacy Policy
Contact Us Message on WhatsApp +91-9687-182-185 editor@ijsat.org