FY2010 - Oak Ridge National Laboratory
FY2010 - Oak Ridge National Laboratory
FY2010 - Oak Ridge National Laboratory
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Director’s R&D Fund—<br />
General<br />
05569<br />
Identification of New, Super Heavy Element Z=117 Using HFIR-<br />
Produced 249 Bk Target Material and Intense 48 Ca Beam at Dubna<br />
Krzysztof P. Rykaczewski, Robert K. Grzywacz, Jeffrey L. Binder, Julie G. Ezold, and J. H. Hamilton<br />
Project Description<br />
The project aimed and succeeded in the identification of a new super-heavy chemical element of the<br />
periodic table with atomic number Z=117. The short-lived radioactive 249 Bk target produced from the<br />
curium and americium seed material irradiated during two years at the ORNL High Flux Isotope Reactor<br />
(HFIR) was used in this experiment. Over 22 mg of 249 Bk, the radioactive isotope having Z=97 protons<br />
and N=152 neutrons, were chemically separated at the ORNL Radiochemical Engineering Development<br />
Center (REDC) in the first half of 2009. At the end of June 2009, the 249 Bk was transferred to the Institute<br />
of Atomic Reactors at Dimitrovgrad (Russia) for target fabrication. The rotating target wheel containing<br />
six 249 Bk target sectors was transferred to the Joint Institute for Nuclear Research (JINR) at Dubna<br />
(Russia) in July 2009. The irradiation of 249 Bk with a 48 Ca beam of 252 MeV and 245 MeV energy,<br />
started at the Flerov <strong>Laboratory</strong> of Nuclear Reactions (FLNR) of JINR at the end of July 2009 and lasted<br />
150 days. Two isotopes of new chemical element Z=117 were identified among fusion-evaporation<br />
reaction products. Five decay chains of 293(117) isotope and one long decay chain starting at 294(117)<br />
isotope were observed, leading to the identification of 11 new super heavy nuclei.<br />
The results were published by the Dubna–ORNL–Las Vegas–Livermore–Vanderbilt–Dimitrovgrad<br />
collaboration in Physical Review Letters 104, 142502 in April 2010. An increased stability with larger<br />
neutron number observed for newly identified super heavy nuclei represents an experimental verification<br />
for the existence of the predicted Island of (Enhanced) Stability for Super Heavy Elements. The original<br />
publication triggered over 200 articles in popular and scientific media, including New York Times,<br />
Science, Physics Today, and others.<br />
Mission Relevance<br />
The discovery of a new chemical element is an increasingly difficult high-profile scientific achievement,<br />
as could be seen from the media reaction to the announcement of the Z=117 discovery. The studies<br />
aiming for super heavy elements help to establish and understand the limits of the periodic table of<br />
elements and of atomic nuclei. The decay properties and production cross section of new isotopes<br />
identified in this study helped us to understand the structure of the heaviest nuclei and the underlying<br />
nuclear forces binding nucleons together. The decreasing alpha-decay energies and correspondingly<br />
increasing half-lives with the increasing neutron number of odd-Z isotopes created suggestive evidence<br />
for approaching the predicted magic neutron number N=184.<br />
New ideas related to the search for even heavier new chemical elements have been developed during this<br />
project. Upon success of the current experiment, the search for the new element Z=119 could be<br />
performed using the next batch of HFIR-REDC–produced 249 Bk material and an intense 50 Ti Z=22 beam<br />
either at JINR Dubna or GSI Darmstadt (Germany). Future studies of super heavy elements may use<br />
Z=98 251 Cf targets extracted from old californium material present in the ORNL inventory of transactinides<br />
isotopes. The amount of californium material of enhanced purity, at the level of 1 mg of 251 Cf to<br />
1 ng of 252 Cf, will allow the search of new isotopes of elements Z=118 (with 48 Ca beam) and for the<br />
isotopes of new element Z=120 (with 50 Ti beam). Since the alpha-decay half-lives of the isotopes of<br />
elements heavier than Z=117 may be in the microsecond region, the use of a fast digital data acquisition<br />
system designed at ORNL (at Holifield Radioactive Ion Beam Facility) will be essential in future studies<br />
of new elements. The development of new detector and digital data acquisition systems, recently<br />
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