Abstract

The stability properties of strong shock waves in diatomic ideal gases are investigated. Shock instabilities in diatomic gases may play a role in the dynamics of astrophysical molecular clouds, hypersonic flight applications, and inertial confinement schemes. It is shown that the dissociation processes alone do not give rise to shock instabilities. It is further demonstrated that the shock’s front becomes unstable under spontaneous acoustic emission due to the ionization processes and only for those perturbations that are characterized by thermal nonequilibrium between the electrons and the heavy particles (atoms, ions, and molecules). To show that, the classical Dyakov–Kontorovich stability criterion is modified in order to take into account the effects of the perturbed electronic temperature. Numerical calculations for diatomic nitrogen indicate that the spontaneous acoustic instability occurs on the descending portion of the Hugoniot curve in the density–pressure plane. In addition, it is found that the threshold for spontaneous acoustic instability decreases with the upstream density.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.