The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss

Details The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cha%26a...8..223w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 8, Issue 3, p. 223-227.

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we investigate the stability of solar-type stars whose structure is determined by the PPI reaction according to the criterion of excess entropy production [1] of non-linear, non-equilibrium thermodynamics, taking into account the mass loss in the reaction. Our result is: the star is certainly stable if the hydrogen-to-helium ratio satisfies the inequality x/y<8.916(1+0.563A3/A1β -0.163ay1/1- ay1) This is to be compared with x/y<9.2, derived previously [2], on neglecting the mass loss. (β~10-4, a ~10-2)

Affiliated with

Also associated with

No associations

Rating

The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss 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 The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stability of stellar structure in non-equilbrium thermodynamics III. The PPI reaction allowing for mass loss will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1393272