Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium

Details Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..462i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, May 1991, p. 462-468. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Gas Dynamics, Relaxation (Mechanics), Stellar Radiation, Thermodynamic Equilibrium, Energy Transfer, Finite Difference Theory, Nonequilibrium Radiation

Scientific paper

The validity of a two-temperature approximation is discussed in a general formulation of relaxation to thermodynamic equilibrium. It is shown that the energy exchange rates calculated by Imshennik and Molodtsov (1990) have a clear quantitative physical meaning for arbitrary parameters of nonequilibrium radiation. It is argued that the two-temperature approximation for the arbitrary finite difference of the radiation temperature and the matter temperature is an efficient and simple means for studying stellar radiation gas dynamics.

Affiliated with

Also associated with

No associations

Rating

Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Processes of the relaxation of matter and radiation to the state of thermodynamic equilibrium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1039965