Ontology type: schema:Chapter Open Access: True
1994
AUTHORSTh. Blaich , Th. W. Elze , H. Emling , H. Freiesleben , K. Grimm , W. Henning , R. Holzmann , J. G. Keller , H. Klingler , J. V. Kratz , R. Kulessa , D. Lambrecht , S. Lange , Y. Leifels , E. Lubkiewicz , E. F. Moore , W. Prokopowicz , R. Schmidt , C. Schütter , H. Spies , K. Stelzer , J. Stroth , E. Wajda , W. Waluś , M. Zinser , E. Zude , FOPI-Collaboration
ABSTRACTCollective flow of nuclear matter is one important aspect of the research performed at heavy ion accelerator laboratories. The phenomenon was predicted on the basis of hydrodynamical calculations [1], and experimental evidence was first presented for the systems 93 Nb + 93 Nb and 197 Au + 197 Au in the projectile energy range between 150 and 1050 MeV/u [2]. The comparison to microscopic calculations shows that nuclear matter is compressed to about two to three times the ground state density and that a substantial fraction of the kinetic energy in the entrance channel is converted into compressional energy [3]. In these calculations, the relation between density and compressional energy depends on the parameterization of the nucleon-nucleon inter-action. The values of its parameters will hopefully be restricted by a comparison of the calculations to experimental data, and thus one can obtain information on the nucleon-nucleon interaction within the nuclear medium which is not accessible from other sources. More... »
PAGES677-686
Hot and Dense Nuclear Matter
ISBN
978-1-4613-6071-1
978-1-4615-2516-5
http://scigraph.springernature.com/pub.10.1007/978-1-4615-2516-5_60
DOIhttp://dx.doi.org/10.1007/978-1-4615-2516-5_60
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