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 in | The European physical journal. A, Hadrons and nuclei Vol. 52; no. 11; pp. 1 - 6 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
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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. |
Author_xml | – sequence: 1 givenname: D. N. surname: Poenaru fullname: Poenaru, D. N. email: poenaru@fias.uni-frankfurt.de organization: Horia Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Frankfurt Institute for Advanced Studies (FIAS), Johann Wolfgang Goethe University – sequence: 2 givenname: R. A. surname: Gherghescu fullname: Gherghescu, R. A. organization: Horia Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Frankfurt Institute for Advanced Studies (FIAS), Johann Wolfgang Goethe University |
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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 |
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