Non-Similarity Solutions for Explosion Waves in Stellar Interiors

Details Non-Similarity Solutions for Explosion Waves in Stellar Interiors Non-Similarity Solutions for Explosion Waves in Stellar Interiors

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..209r&link_type=abstract

Astrophysics and Space Science, Volume 232, Issue 2, pp.209-216

Astronomy and Astrophysics

Astrophysics

Scientific paper

Non-similarity solutions in closed-forms, for propagation of explosion (instantaneous or non-instantaneous) waves in stellar models, in which the density falls off inversely as a power of distance, has been obtained in this paper. The power indexα lies in the interval 1 <α < 3. The similarity solutions forα = 2 ṡ 5, valid only for an instantaneous explosion, follows as a particular one. Unlike the case of similarity solutions, the total energy of the wave as well as the strength of the shock varies with time. Besides, the solutions are applicable for arbitrary values of time. The results are extensions of my previous work (1969).

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