Synthesis of superheavy nuclei: Obstacles and opportunities
There are only 3 methods for the production of heavy and superheavy (SH) nuclei, namely, fusion reactions, a sequence of neutron capture and beta(-) decay and multinucleon transfer reactions. Low values of the fusion cross sections and very short half-lives of nuclei with Z<120 put obstacles in s...
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EDP Sciences
2015-01-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20158600066 |
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author | Zagrebaev V.I. Karpov A.V. Greiner Walter |
author_facet | Zagrebaev V.I. Karpov A.V. Greiner Walter |
author_sort | Zagrebaev V.I. |
collection | DOAJ |
description | There are only 3 methods for the production of heavy and superheavy (SH) nuclei, namely, fusion reactions, a sequence of neutron capture and beta(-) decay and multinucleon transfer reactions. Low values of the fusion cross sections and very short half-lives of nuclei with Z<120 put obstacles in synthesis of new elements. At the same time, an important area of SH isotopes located between those produced in the cold and hot fusion reactions remains unstudied yet. This gap could be filled in fusion reactions of 48Ca with available lighter isotopes of Pu, Am, and Cm. New neutron-enriched isotopes of SH elements may be produced with the use of a 48Ca beam if a 250Cm target would be prepared. In this case we get a real chance to reach the island of stability owing to a possible beta(+) decay of 291114 and 287112 nuclei formed in this reaction with a cross section of about 0.8 pb. A macroscopic amount of the long-living SH nuclei located at the island of stability may be produced by using the pulsed nuclear reactors of the next generation only if the neutron fluence per pulse will be increased by about three orders of magnitude. Multinucleon transfer processes look quite promising for the production and study of neutron-rich heavy nuclei located in upper part of the nuclear map not reachable by other reaction mechanisms. Reactions with actinide beams and targets are of special interest for synthesis of new neutron-enriched transfermium nuclei and not-yet-known nuclei with closed neutron shell N=126 having the largest impact on the astrophysical r-process. The estimated cross sections for the production of these nuclei allows one to plan such experiments at currently available accelerators. |
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spelling | doaj.art-5b6f579d0b274647a4ff23b9218b12412022-12-21T20:19:00ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01860006610.1051/epjconf/20158600066epjconf_fusion2015_00066Synthesis of superheavy nuclei: Obstacles and opportunitiesZagrebaev V.I.0Karpov A.V.1Greiner Walter2Flerov Laboratory of Nuclear ReactionsFlerov Laboratory of Nuclear ReactionsFrankfurt Institute for Advanced Studies, J.W. Goethe-UniversitätThere are only 3 methods for the production of heavy and superheavy (SH) nuclei, namely, fusion reactions, a sequence of neutron capture and beta(-) decay and multinucleon transfer reactions. Low values of the fusion cross sections and very short half-lives of nuclei with Z<120 put obstacles in synthesis of new elements. At the same time, an important area of SH isotopes located between those produced in the cold and hot fusion reactions remains unstudied yet. This gap could be filled in fusion reactions of 48Ca with available lighter isotopes of Pu, Am, and Cm. New neutron-enriched isotopes of SH elements may be produced with the use of a 48Ca beam if a 250Cm target would be prepared. In this case we get a real chance to reach the island of stability owing to a possible beta(+) decay of 291114 and 287112 nuclei formed in this reaction with a cross section of about 0.8 pb. A macroscopic amount of the long-living SH nuclei located at the island of stability may be produced by using the pulsed nuclear reactors of the next generation only if the neutron fluence per pulse will be increased by about three orders of magnitude. Multinucleon transfer processes look quite promising for the production and study of neutron-rich heavy nuclei located in upper part of the nuclear map not reachable by other reaction mechanisms. Reactions with actinide beams and targets are of special interest for synthesis of new neutron-enriched transfermium nuclei and not-yet-known nuclei with closed neutron shell N=126 having the largest impact on the astrophysical r-process. The estimated cross sections for the production of these nuclei allows one to plan such experiments at currently available accelerators.http://dx.doi.org/10.1051/epjconf/20158600066 |
spellingShingle | Zagrebaev V.I. Karpov A.V. Greiner Walter Synthesis of superheavy nuclei: Obstacles and opportunities EPJ Web of Conferences |
title | Synthesis of superheavy nuclei: Obstacles and opportunities |
title_full | Synthesis of superheavy nuclei: Obstacles and opportunities |
title_fullStr | Synthesis of superheavy nuclei: Obstacles and opportunities |
title_full_unstemmed | Synthesis of superheavy nuclei: Obstacles and opportunities |
title_short | Synthesis of superheavy nuclei: Obstacles and opportunities |
title_sort | synthesis of superheavy nuclei obstacles and opportunities |
url | http://dx.doi.org/10.1051/epjconf/20158600066 |
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