Light fragment preformation in cold fission of 282Cn

. In a previous article, published in Phys. Rev. C 94 , 014309 (2016), we have shown for the first time that the best dynamical trajectory during the deformation toward fission of the superheavy nucleus 286 Fl is a linearly increasing radius of the light fragment, R 2 . This macroscopic-microscopic...

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Published inThe European physical journal. A, Hadrons and nuclei Vol. 52; no. 11; pp. 1 - 6
Main Authors Poenaru, D. N., Gherghescu, R. A.
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Published Berlin/Heidelberg Springer Berlin Heidelberg 2016
Springer Nature B.V
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Abstract . In a previous article, published in Phys. Rev. C 94 , 014309 (2016), we have shown for the first time that the best dynamical trajectory during the deformation toward fission of the superheavy nucleus 286 Fl is a linearly increasing radius of the light fragment, R 2 . This macroscopic-microscopic result reminds us about the α or cluster preformation at the nuclear surface, assumed already in 1928, and proved microscopically many times. This time we give more detailed arguments for the nucleus 282 Cn. Also similar figures are presented for heavy nuclei 240 Pu and 252 Cf. The deep minimum of the total deformation energy near the surface is shown for the first time as a strong argument for cluster preformation.
AbstractList . In a previous article, published in Phys. Rev. C 94 , 014309 (2016), we have shown for the first time that the best dynamical trajectory during the deformation toward fission of the superheavy nucleus 286 Fl is a linearly increasing radius of the light fragment, R 2 . This macroscopic-microscopic result reminds us about the α or cluster preformation at the nuclear surface, assumed already in 1928, and proved microscopically many times. This time we give more detailed arguments for the nucleus 282 Cn. Also similar figures are presented for heavy nuclei 240 Pu and 252 Cf. The deep minimum of the total deformation energy near the surface is shown for the first time as a strong argument for cluster preformation.
In a previous article, published in Phys. Rev. C 94, 014309 (2016), we have shown for the first time that the best dynamical trajectory during the deformation toward fission of the superheavy nucleus 286Fl is a linearly increasing radius of the light fragment, R 2 . This macroscopic-microscopic result reminds us about the α or cluster preformation at the nuclear surface, assumed already in 1928, and proved microscopically many times. This time we give more detailed arguments for the nucleus 282Cn. Also similar figures are presented for heavy nuclei 240Pu and 252 Cf. The deep minimum of the total deformation energy near the surface is shown for the first time as a strong argument for cluster preformation.
ArticleNumber 349
Author Poenaru, D. N.
Gherghescu, R. A.
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  givenname: R. A.
  surname: Gherghescu
  fullname: Gherghescu, R. A.
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Snippet . In a previous article, published in Phys. Rev. C 94 , 014309 (2016), we have shown for the first time that the best dynamical trajectory during the...
In a previous article, published in Phys. Rev. C 94, 014309 (2016), we have shown for the first time that the best dynamical trajectory during the deformation...
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SubjectTerms Clusters
Deformation
Hadrons
Heavy Ions
Heavy nuclei
Nuclear fission
Nuclear Fusion
Nuclear Physics
Nuclei
Particle and Nuclear Physics
Physics
Physics and Astronomy
Regular Article - Theoretical Physics
Title Light fragment preformation in cold fission of 282Cn
URI https://link.springer.com/article/10.1140/epja/i2016-16349-9
https://www.proquest.com/docview/1880833255
Volume 52
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