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Formation and Decay of the Composite System Z = 120 in Reactions with Heavy Ions at Energies Near the Coulomb Barrier

Authors :
K. V. Novikov
B. Gall
M. G. Itkis
G. N. Knyazheva
M. Cheralu
I. M. Harca
Emanuele Vardaci
I. M. Itkis
N. Tortorelli
I. N. Diatlov
Zouhair Asfari
I. V. Vorobiev
Deepak Kumar
A. V. Karpov
I. V. Pchelintsev
Vladimir Loginov
N. I. Kozulina
A. Bondarchenko
Pushpendra Singh
C. Borcea
S. Heinz
E. M. Kozulin
Wladyslaw Henryk Trzaska
Novikov, K. V.
Kozulin, E. M.
Knyazheva, G. N.
Itkis, I. M.
Karpov, A. V.
Itkis, M. G.
Diatlov, I. N.
Cheralu, M.
Gall, B.
Asfari, Z.
Kozulina, N. I.
Kumar, D.
Pchelintsev, I. V.
Loginov, V. N.
Bondarchenko, A. E.
Singh, P. P.
Vorobiev, I. V.
Heinz, S.
Trzaska, W. H.
Vardaci, E.
Tortorelli, N.
Borcea, C.
Harca, I.
Institut Pluridisciplinaire Hubert Curien (IPHC)
Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Source :
Bull.Russ.Acad.Sci.Phys., Bull.Russ.Acad.Sci.Phys., 2020, 84 (4), pp.495-499. ⟨10.3103/S1062873820040206⟩
Publication Year :
2020

Abstract

International audience; The mass, energy and angular distributions of binary fragments formed in the reactions $^{64}$Ni + $^{238}$U, $^{58}$Fe + $^{244}$Pu, $^{52}$Cr + $^{248}$Cm, $^{54}$Cr + $^{248}$Cm at energies near the Coulomb barrier have been measured. The analysis of energy distributions of the symmetric fragments with mass numbers ${{{{A}_{{{\text{CN}}}}}} \mathord{\left/ {\vphantom {{{{A}_{{{\text{CN}}}}}} 2}} \right. \kern-0em} 2} \pm 20$ formed in these reactions have been applied to separate compound nucleus fission and quasi-fission. The estimated fusion probability for the reactions Cr, Fe, and Ni ions with actinide targets shows an exponential dependence on the mean fissility parameter of the system and shows also that reaction with Cr ions is more favorable for production of the super heavy element with Z = 120.

Details

Database :
OpenAIRE
Journal :
Bull.Russ.Acad.Sci.Phys., Bull.Russ.Acad.Sci.Phys., 2020, 84 (4), pp.495-499. ⟨10.3103/S1062873820040206⟩
Accession number :
edsair.doi.dedup.....a7a4f59d7edc75445f25068db7fae6b6