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| Name, Symbol, Number | ununhexium, Uuh, 116 | ||||||||||||||||||||||||||||||
| Chemical series | presumably poor metal | ||||||||||||||||||||||||||||||
| Group, Period, Block | 16, 7, p | ||||||||||||||||||||||||||||||
| Standard atomic weight | [293] g·mol−1 | ||||||||||||||||||||||||||||||
| Electron configuration | perhaps [Rn] 5f14 6d10 7s2 7p4 (guess based on polonium) | ||||||||||||||||||||||||||||||
| Electrons per shell | 2, 8, 18, 32, 32, 18, 6 | ||||||||||||||||||||||||||||||
| CAS registry number | 54100-71-9 | ||||||||||||||||||||||||||||||
| Selected isotopes | |||||||||||||||||||||||||||||||
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| References | |||||||||||||||||||||||||||||||
Ununhexium /un.unˈhex.ium/ is the temporary name of a synthetic superheavy element in the periodic table that has the temporary symbol Uuh and has the atomic number 116. Recent research has referred to it as eka-polonium.
On July 19, 2000, scientists at Dubna (FLNR) detected a single decay from an atom of ununhexium following the irradiation of a Cm-248 target with Ca-48 ions. The results were published in December, 2000. "Observation of the decay of 292116", Oganessian et al., Phys. Rev. C 63, 011301 (2000). Retrieved on 2008-03-03 This 10.54 MeV alpha-emitting activity was originally assigned to 292Uuh due to the correlation of the daughter to previously assigned 288Uuq. However, that assignment was later altered to 289Uuq, and hence this activity was correspondingly changed to 293Uuh. Two further atoms were reported by the institute during their second experiment between April-May 2001."Confirmed results of the 248Cm(48Ca,4n)292116 experiment", Patin et al., LLNL report (2003). Retrieved on 2008-03-03
In the same experiment they also detected a decay chain which corresponded to the first observed decay of ununquadium and assigned to 289Uuq. This activity has not been observed again in a repeat of the same reaction. However, its detection in this series of experiments indicates the possibility of the decay of a meta-stable isomer of ununhexium, namely 293m116, or a rare decay branch of the already discovered ground state isomer, in which the first alpha particle was missed. Further research is required to positively assign this activity.
The team repeated the experiment in April-May 2005 and detected 8 atoms of ununhexium. The measured decay data confirmed the assignment of the discovery isotope as 293116. In this run, the team also observed 292116 in the 4n channel for the first time."Measurements of cross sections and decay properties of the isotopes of elements 112, 114, and 116 produced in the fusion reactions 233,238U , 242Pu , and 248Cm+48Ca", Oganessian et al., Phys. Rev. C 70, 064609 (2004). Retrieved on 2008-03-03
The IUPAC/IUPAP Joint Working Party (JWP) are currently assessing the claim of discovery for this element by the Dubna team.
The element with Z=116 is historically known as eka-polonium. Ununhexium (Uuh) is a temporary IUPAC systematic element name. Research scientists usually refer to the element simply as element 116 (E116).
Claims to the discovery of element 116 have been put forward by Dmitriev of the Dubna team. The JWP will decide to whom the right to suggest a name will be given. The IUPAC have the final say on the official adoption of a name. No name for element 116 has yet been suggested by the Dubna team.
According to IUPAC rules, names used for previous elements that have ultimately not been adopted are not allowed to be proposed for future use. The table below summarises those names which are probably not allowed to be proposed by the claimant laboratories under the rules.
| Name | Symbol | Reason |
|---|---|---|
| Russium | Rs | Used for claimed discovery of element 43 |
| Kurchatovium | Ku | Used for claimed discovery of element 104 |
| Flerovium | Fl | Used for claimed discovery of element 102For use, see http://www.mi.infn.it/conferences/zhuikov/italy1c.pdf |
Many speculative names appear in popular literature. The table below lists these names in the case where they obey IUPAC rules and are plausible with regard to the claimant laboratories. Rumored suggestions linked to the claimant laboratories are also included.
| Name | Synbol | Derivation | Comments |
|---|---|---|---|
| Flyorovium | Fl; Fv | Georgy Flyorov, head of the Dubna team | Fl symbol unlikely due to confusion with fluorine (F); flerovium linked to element 118 |
| Butlerovium | Bu; Bv | Aleksandr Butlerov, Russian chemist | unlikely—not a nuclear chemist |
| Rossijium | Ro; Rs | Rossija, translation of Russian name for Russia | |
| Taldomskium | Taldomsky, District of Moscow where Dubna lies |
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Ununhexium has 6 full shells, 7s+5p+4d+2f=18 full subshells, and 116 orbitals:
Bohr model: 2, 8, 18, 32, 32, 18, 6
Quantum mechanical model: 1s22s22p63s23p64s23d10 4p65s24d105p66s24f145d10 6p67s25f146d107p4
Element 116 is projected to be the fourth member of the 7p series of non-metals and the heaviest member of group 16 (VIA) in the Periodic Table, below polonium. The group oxidation state of +VI is known for all the members apart from oxygen which lacks available d-orbitals for expansion and is limited to a maximum +II state, exhibited in the fluoride OF2. The +IV is known for sulfur, selenium, tellurium, and polonium, undergoing a shift in stability from reducing for S(IV) and Se(IV) to oxidising in Po(IV). Tellurium(IV) is the most stable for this element. This suggests a decreasing stability for the higher oxidation states as the group is descended and element 116 should portray an oxidising +IV state and a more stable +II state. The lighter members are also known to form a −II state as oxide, sulfide, selenide, and telluride. Polonide formation is nonconfirmed or only transient. The extrapolated electronegativity of ununhexium should eliminate this low oxidation state.
The possible chemistry of element 116 can be extrapolated from that of polonium. It should therefore undergo oxidation to a dioxide, UuhO2, although a trioxide, UuhO3 is plausible, but unlikely. The stability of a +II state should manifest itself in the formation of a simple monoxide, UuhO. Fluorination will likely result in a tetrafluoride, UuhF4 and/or a difluoride, UuhF2. Chlorination and bromination may well stop at the corresponding dihalides, UuhCl2 and UuhI2. Oxidation by iodine should certainly stop at UuhI2 and may even be inert to this element.
In 1995, the team at GSI attempted the synthesis of 290116 as a radiative capture (x=0) product. No atoms were detected providing a cross section limit of 4.8 pb.
There are sketchy indications that this reaction was attempted by the team at GSI in 2006. There are no published results on the outcome, presumably indicating that no atoms were detected. This is expected from a study of the systematics of cross sections for U-238 targets."List of experiments 2000-2006"
The first attempt to synthesise element 116 was performed in 1977 by Ken Hulet and his team at the Lawrence Livermore National Laboratory (LLNL). They were unable to detect any atoms of ununhexium.Search for Superheavy Elements in the Bombardment of 248Cm with 48Ca. Yuri Oganessian and his team at the Flerov Laboratory of Nuclear Reactions (FLNR) subsequently attempted the reaction in 1978 and were met by failure. In 1985, a joint experiment between Berkeley and Peter Armbruster\'s team at GSI, the result was again negative with a calculated cross-section limit of 10–100 pb.Attempts to Produce Superheavy Elements by Fusion of 48Ca with 248Cm in the Bombarding Energy Range of 4.5-5.2 MeV/u.
In order to assist in the assignment of isotope mass numbers for ununhexium, in March-May 2003 the Dubna team bombarded a Cm-245 target with Ca-48 ions. They were able to observe two new isotopes, assigned to 291116 and 290116."Measurements of cross sections for the fusion-evaporation reactions 244Pu(48Ca,xn)292−x114 and 245Cm(48Ca,xn)293−x116", Oganessian et al., Phys. Rev. C 69, 054607 (2004). Retrieved on 2008-03-03 This experiment was successfully repeated in Feb-March 2005 where 10 atoms were created with identical decay data to those reported in the 2003 experiment."Synthesis of the isotopes of elements 118 and 116 in the 249Cf and 245Cm+48Ca fusion reactions", Oganessian et al., Phys. Rev. C 74, 044602 (2006). Retrieved on 2008-03-03
Ununhexium has also been observed in the decay of ununoctium. In October 2006 it was announced that 3 atoms of ununoctium had been detected by the bombardment of californium-249 with calcium-48 ions, which then rapidly decayed into ununhexium.
The observation of 290116 allowed the assignment of the product to 294118 and proved the synthesis of a nucleus with Z=118 (see ununoctium).
| Isotope | Year discovered | Discoverer reaction |
|---|---|---|
| 290Uuh | 2002 | 249Cf(48Ca,3n)see ununoctium |
| 291Uuh | 2003 | 245Cm(48Ca,2n) |
| 292Uuh | 2004 | 248Cm(48Ca,4n) |
| 293Uuh | 2000 | 248Cm(48Ca,3n) |
The table below provides cross-sections and excitation energies for hot fusion reactions producing ununhexium isotopes directly. Data in bold represent maxima derived from excitation function measurements. + represents an observed exit channel.
| Projectile | Target | CN | 2n | 3n | 4n | 5n |
|---|---|---|---|---|---|---|
| 48Ca | 248Cm | 296Uuh | 1.1 pb, 38.9 MeV | 3.3 pb, 38.9 MeV | ||
| 48Ca | 245Cm | 293Uuh | 0.9 pb, 33.0 MeV | 3.7 pb, 37.9 MeV |
In 1999, researchers at Lawrence Berkeley National Laboratory announced the synthesis of 293118 (see ununoctium), in a paper published in Physical Review Letters.Ninov, V.; et al. (1999). "Observation of Superheavy Nuclei Produced in the Reaction of 86Kr with 208Pb". Physical Review Letters 83: 1104. doi:10.1103/PhysRevLett.83.1104. The claimed isotope 289116 decayed by 11.63MeV alpha emission with a halflife of 0.64 ms. The following year, they published a retraction after other researchers were unable to duplicate the results.Editorial note on the preceding. In June 2002, the director of the lab announced that the original claim of the discovery of these two elements had been based on data fabricated by the principal author Victor Ninov. As such, this ununhexium isotope is currently unknown or deconfirmed.
The team at Dubna are planning to revisit the synthesis in 2008. They will bombard a plutonium-244 target with titanium-50 ions. This experiment will allow them to assess the feasibility of using projectiles with Z>20 required in the synthesis of SHE\'s with Z>118. There are also plans to repeat the Cm-248 reaction at different projectile energies in order to probe the 2n channel, leading to the new isotope 294116. In addition they hope to complete the excitation function of the 4n channel product, 292116, which will allow them to assess the stabilising effect of the N=184 shell on the yield of evaporation residues.
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