Fission in the landscape of heaviest elements: Some recent examples
Khuyagbaatar, J., Yakushev, A., Düllmann, Ch.E., Ackermann, D., Andersson, L.-L., Block, M., Brand, H., Even, J., Forsberg, U., Hartmann, W., Herzberg, R.-D., Heßberger, F.P., Hoffmann, J., Hübner, A., Jäger, E., Jeppsson, J., Kindler, B., Kratz, J.V., Krier, J., . . . Yakusheva, V. (2016). Fission in the landscape of heaviest elements: Some recent examples. In D. Rudolph (Ed.), Nobel Symposium NS 160 - Chemistry and Physics of Heavy and Superheavy Elements (Article 03003). EDP Sciences. EPJ Web of Conferences, 131. https://doi.org/10.1051/epjconf/201613103003
Julkaistu sarjassa
EPJ Web of ConferencesToimittajat
Päivämäärä
2016Tekijänoikeudet
© the Authors, published by EDP Sciences. This is an Open Access article distributed under the terms of the
Creative Commons Attribution License 4.0.
The fission process still remains a main factor that determines the
stability of the atomic nucleus of heaviest elements. Fission half-lives vary
over a wide range, 10−19−1024 s. Present experimental techniques for the
synthesis of the superheavy elements that usually measure -decay chains
are sensitive only in a limited range of half-lives, often 10−5−103 s. In
the past years, measurement techniques for very short-lived and very longlived
nuclei were significantly improved at the gas-filled recoil separator
TASCA at GSI Darmstadt. Recently, several experimental studies of fissionrelated
phenomena have successfully been performed. In this paper, results
on 254−256Rf and 266Lr are presented and corresponding factors for retarding
the fission process are discussed.
Julkaisija
EDP SciencesISBN
978-2-7598-9011-8Emojulkaisun ISBN
Konferenssi
Nobel SymposiumKuuluu julkaisuun
Nobel Symposium NS 160 - Chemistry and Physics of Heavy and Superheavy ElementsISSN Hae Julkaisufoorumista
2100-014XAsiasanat
Julkaisu tutkimustietojärjestelmässä
https://converis.jyu.fi/converis/portal/detail/Publication/26358940
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Ellei muuten mainita, aineiston lisenssi on © the Authors, published by EDP Sciences. This is an Open Access article distributed under the terms of the
Creative Commons Attribution License 4.0.
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Stability and synthesis of superheavy elements: Fighting the battle against fission – example of 254No
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First prompt in-beam gamma-ray spectroscopy of a superheavy element: the 256Rf
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Exploring the stability of super heavy elements: First Measurement of the Fission Barrier of 254No
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Fusion-fission and quasifission of superheavy systems with Z=110-116 formed in Ca 48 -induced reactions
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