Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.213p&link_type=abstract
Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:
Astronomy and Astrophysics
Astrophysics
Scientific paper
In modeling huge astrophysical phenomena exits the mechanizm of shock wave. One of the energetic resource for stability of shock wave propagation could be the creation of quark matter in dense slices of the mass distribution behind the shock wave front. We studied the thermo- and hydrodynamical conditions, when the matter compression by shock wave could result to a dissosiation of the nucleous into quasy quark plasma, and we obtain the products characteristics. The obtained results of calculations could be a criteria of the existance of quark matter in early stages of supernovae explosions. We studied the problem in frame of relativistic hydrodynamics, since the estimating velosities are at order to 0.3 c.
Grigorian H. A.
Poghosyan G. S.
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