Thermochemical Instabilities in Optically Thin Reacting Plasmas
Miguel H. Iba~nez S.
Abstract
The linear stability analysis of an optically thin plasma where a general reaction proceeds, including chemical relaxation time effects, is carried out . A fifth order dispersion equation (instead of the fourth order one resulting when such effects are neglected) is obtained. The new mode with the corresponding instability criterion as well as the modifications of the previous four modes and the corresponding instability criteria, are analyzed. Generally, a further stabilizing effect on the unstable modes and an increasing of the damping of stable modes appear because of the second viscosity generated by the chemical reaction. The results are applied to: (1) a collisionally ionized pure hydrogen plasma heated at a constant rate per unit mass and cooled by free-free transitions, ionization, and e-H collisional excitations; (2) a diffused gas with metallicity Z, photoionized and heated by a radiation field, and cooled by excitation of hydrogen and heavy metal lines.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka