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- W2384487935 abstract "The emission time of intermediate mass fragments (IMF) has been studied as a function of spatial evolution of the emission source for ~40 Ar+ ~natAg reaction at 30MeV / u, and the spatial-time evolution of projectile-like fragments emission has also been discussed. The investigation for spatial-time evolution of the reaction system shows that the emission time of the IMF mainly depends on the correlation functions and the density of nuclear matter, and that it is not sensitive to the mass number of emitting sources. For high-energy fragments, a smaller nuclear density would lead to a smaller assignment for emission time τ; therefor the τ values extracted from the normal nuclear density could be taken as upper limits of real τ values. For the mid-velocity fragments, their emission times do not change with size of the source and these τ values could be taken as the real values directly." @default.
- W2384487935 created "2016-06-24" @default.
- W2384487935 creator A5031086885 @default.
- W2384487935 date "2000-01-01" @default.
- W2384487935 modified "2023-09-23" @default.
- W2384487935 title "Space-Time Evolution of Projectile-Like Fragment Emission for ~(40) Ar + ~(nat)Ag Reaction at 30MeV/u" @default.
- W2384487935 hasPublicationYear "2000" @default.
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