1986
DOI: 10.1016/0370-2693(86)90640-4
|View full text |Cite
|
Sign up to set email alerts
|

Intermediate structure in strongly damped 12C + 24Mg reactions of the orbiting type

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

1
14
0

Year Published

1987
1987
1997
1997

Publication Types

Select...
6
1

Relationship

1
6

Authors

Journals

citations
Cited by 39 publications
(15 citation statements)
references
References 17 publications
1
14
0
Order By: Relevance
“…However, it is relevant to also comment briefly on the possible manifestation of this phenomenon in heavy-ion collisions. In particular, memory effects are suggested [24] to be a sufficient condition to explain nonselfaveraging of the excitation function oscillations in dissipative heavy-ion collisions [31][32][33][34][35][36][37][38][39][40][41][42][43][44][45][46]. It has also been found that spin and parity S-matrix correlation allows one to account for the oscillating non-Lorentzian behaviour of the cross section energy autocorrelation functions in 58 Ni + 62 Ni elastic and inelastic scattering [47].…”
Section: Resultsmentioning
confidence: 99%
“…However, it is relevant to also comment briefly on the possible manifestation of this phenomenon in heavy-ion collisions. In particular, memory effects are suggested [24] to be a sufficient condition to explain nonselfaveraging of the excitation function oscillations in dissipative heavy-ion collisions [31][32][33][34][35][36][37][38][39][40][41][42][43][44][45][46]. It has also been found that spin and parity S-matrix correlation allows one to account for the oscillating non-Lorentzian behaviour of the cross section energy autocorrelation functions in 58 Ni + 62 Ni elastic and inelastic scattering [47].…”
Section: Resultsmentioning
confidence: 99%
“…The experimental results obtained for the 24Mg § 12C [8,11,13], 28Si, + lZC [6], 24Mg+ 160 [7,9] and 28Si+ ~4N [10,12] reactions have been interpreted in terms of the formation and decay of a long-lived rotating di-nuclear complex. This di-nuclear system can be formed in the early stages of the collision and then breaks apart in two pieces, while the longer-lived and relaxed complexes will evolve continuously towards more compact fusion configurations which consequently undergo binary fission.…”
Section: Equilibrium Model For Orbitingmentioning
confidence: 95%
“…This coexistence has been experimentally observed in the formation of the 20,22 Ne [4], 28 Al [5], 36 Ar [6], 40 Ca [7], 47 V [8], and 48 Cr [9] dinuclear systems. In these studies, most of these dinuclear systems were formed via different entrance channels, in order to ascertain whether the CN was playing a key role in the reaction mechanism.…”
mentioning
confidence: 97%