Physics
Scientific paper
Oct 1960
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1960pthph..24..825o&link_type=abstract
Progress of Theoretical Physics, Vol. 24, No. 4, pp. 825-828
Physics
14
Scientific paper
The propagation of spherical shock waves in the stellar interior is considered, extending the method developed in previous papers. A differential equation of the shock strength is derived, which can be applied to any stellar models. It is found that the spherical damping effect is pronounced near the center of stars, and this guarantees the stability of the stellar core in general. In the envelope, this effect becomes negligible, and it is justified near the stellar surface to treat the shock waves as plane.
No associations
LandOfFree
Propagation of Shock Waves in Inhomogeneous Gases. III ---Spherical Shock Waves--- 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 Propagation of Shock Waves in Inhomogeneous Gases. III ---Spherical Shock Waves---, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of Shock Waves in Inhomogeneous Gases. III ---Spherical Shock Waves--- will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1653555