1990
DOI: 10.1016/0375-9474(90)90174-k
|View full text |Cite
|
Sign up to set email alerts
|

Multifragment break-up of nuclei by intermediate-energy protons

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

10
95
0
4

Year Published

1992
1992
2008
2008

Publication Types

Select...
5
3

Relationship

1
7

Authors

Journals

citations
Cited by 144 publications
(109 citation statements)
references
References 15 publications
10
95
0
4
Order By: Relevance
“…For the simulation of the initial stage of the collision the intranuclear cascade (INC) model developed in Dubna was used [20,21]. The INC describes the process of the hadron-nucleon collisions inside the target nucleus.…”
Section: Initial Dynamical Stagementioning
confidence: 99%
“…For the simulation of the initial stage of the collision the intranuclear cascade (INC) model developed in Dubna was used [20,21]. The INC describes the process of the hadron-nucleon collisions inside the target nucleus.…”
Section: Initial Dynamical Stagementioning
confidence: 99%
“…This assumption is not made in the statistical multifragmentation model [35,36,37]. Within this model, a microcanonical ensemble of all break-up channels composed of nucleons and excited fragments of different masses is considered.…”
Section: Comparison With Smm Calculationsmentioning
confidence: 99%
“…Presently, the SMM is one of the most successful models to describe fragmentation and multifragmentation data (see e.g. References [1,4,34,37,38]). U + Pb at 1⋅A GeV (data points) compared to the prediction of the three-stage code (full line) and to the prediction of the SMM code (dotted line).…”
Section: Comparison With Smm Calculationsmentioning
confidence: 99%
“…This can be ascribed to the fact that ABLA is a "classical" de-excitation model in which only the evaporation of neutrons, protons and alpha particles is possible. To account for the emission of IMF, several de-excitation mechanisms can be envisaged: A generalized evaporation, as modeled in GEM [8] which evaporates particles up to Mg; a binary splitting as described in GEMINI [9], which uses the Moretto-type transition state model [10] for the emission of intermediate mass fragments down to a certain limit, the evaporation of lighter fragments being treated within the HauserFeshbach formalism; the opening of multifragmentation channels, as included in SMM [11]. Default parameters of the models have been used except for GEMINI for which the transition from the Hauser-Feshbach to the Transition State Model is made for Z≥4 as recommended by the author [12].…”
mentioning
confidence: 99%