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[en] The relevance of relativistic gravitation and of the properties of nuclear matter at high density to supernova explosions is examined in detail. The existing empirical knowledge on the nuclear equation of state at densities greater than saturation, extracted from analysis of heavy ion collisions and from the breathing mode in heavy nuclei, is also considered. Particulars of the prompt explosions recently obtained theoretically by recent workers are presented. (author)
Source
Faessler, Amand (ed.) (Tuebingen Univ. (Germany, F.R.)); Progress in Particle and Nuclear Physics; v. 17; 472 p; ISBN 0 08 035185 9; 
; 1986; p. 231-247; Pergamon Press; Oxford (UK); The early universe and its evolution: proceedings of the International School of Nuclear Physics; Erice (Italy); 2-14 Apr 1986; CONTRACT DE-AC02-76CH00016
; 1986; p. 231-247; Pergamon Press; Oxford (UK); The early universe and its evolution: proceedings of the International School of Nuclear Physics; Erice (Italy); 2-14 Apr 1986; CONTRACT DE-AC02-76CH00016