1997/09/09 by Miguel H. Iba nez S., Miguel H. Iba~nez S., S., Miguel H. Iba~nez
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High-pressure geophysics and materials #Laser-induced spectroscopy and plasma #Magnetic confinement fusion research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9709079
20 pages, Latex 6.1, 21 EPS figures. to appear 1997, ApJ, Dic 10 issue
arxiv created 1997/09/09 · openalex publication_date 1997/09/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.