Ununtrium

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coperniciumununtriumununquadium
Tl

Uut

(Uht)
Appearance
Unknown
General properties
Name, symbol, number ununtrium, Uut, 113
Pronunciation Listeni/nˈntriəm/
oon-OON-tree-əm
Category notes presumably other metals
Group, period, block 137, p
Standard atomic weight [286]
Electron configuration [Rn] 5f14 6d10 7s2 7p1
(predicted)
Electrons per shell 2, 8, 18, 32, 32, 18, 3
(predicted) (Image)
Physical properties
Atomic properties
Miscellanea
CAS registry number 54084-70-7
Most stable isotopes
Main article: Isotopes of ununtrium
iso NA half-life DM DE (MeV) DP
286Uut syn 19.6 s α 9.63 282Rg
285Uut syn 5.5 s α 9.74,9.48 281Rg
284Uut syn 0.49 s α 10.00 280Rg
283Uut syn 0.10 s α 10.12 279Rg
282Uut syn 73 ms α 10.63 278Rg
278Uut syn 0.34 ms α 11.68 274Rg
· r

Ununtrium is the temporary name of a synthetic element with the temporary symbol Uut and atomic number 113.

It is placed as the heaviest member of the group 13 (IIIA) elements although a sufficiently stable isotope is not known at this time that would allow chemical experiments to confirm its position as a heavier homologue to thallium. It was first detected in 2003 in the decay of ununpentium and was synthesized directly in 2004. Only fourteen atoms of ununtrium have been observed to date. The longest-lived isotope known is 286Uut with a half-life of ~20 s,[1] allowing first chemical experiments to study its chemistry.

Contents

[edit] History

[edit] Discovery profile

The first report of ununtrium was in August 2003 when it was identified as a decay product of ununpentium. These results were published on February 1, 2004, by a team composed of Russian scientists at Dubna (Joint Institute for Nuclear Research), and American scientists at the Lawrence Livermore National Laboratory.[2][3]

\,^{48}_{20}\mathrm{Ca} + \,^{243}_{95}\mathrm{Am} \to \,^{288,287}\mathrm{Uup} \to \,^{284,283}\mathrm{Uut} \to\

On July 23, 2004, a team of Japanese scientists at RIKEN detected a single atom of 278Uut using the cold fusion reaction between bismuth-209 and zinc-70. They published their results on September 28, 2004.[4]

\,^{70}_{30}\mathrm{Zn} + \,^{209}_{83}\mathrm{Bi} \to \,^{279}_{113}\mathrm{Uut} ^{*} \to \,^{278}_{113}\mathrm{Uut} + \,^{1}_{0}\mathrm{n}

Support for their claim appeared in 2004 when scientists at the Institute of Modern Physics (IMP) identified 266Bh as decaying with identical properties to their single event (see bohrium).

The RIKEN team produced a further atom on April 2, 2005, although the decay data were different from the first chain, and may be due to the formation of a meta-stable isomer.

The Dubna-Livermore collaboration has strengthened their claim for the discovery of ununtrium by conducting chemical experiments on the decay daughter 268Db. In experiments in June 2004 and December 2005, the dubnium isotope was successfully identified by milking the Db fraction and measuring any SF activities. Both the half-life and decay mode were confirmed for the proposed 268Db which lends support to the assignment of Z=115 and Z=113 to the parent and daughter nuclei.[5][6]

Theoretical estimates of alpha-decay half-lives of alpha-decay chains from element 113 are in good agreement with the experimental data.[7]

Recent experiments at Dubna have fully confirmed the data for ununpentium and ununtrium but have yet to be fully published and reviewed by the JWP. This process is likely not to occur for some time.[citation needed]

[edit] Naming

The element with atomic number 113 is historically known as eka-thallium. Ununtrium (Uut) is a temporary IUPAC systematic element name. Research scientists usually refer to the element simply as element 113 (or E113).

[edit] Proposed names by claimants

Claims to the discovery of ununtrium have been put forward by Dmitriev of the Dubna team and Morita of the RIKEN team. The IUPAC/IUPAP Joint Working Party will decide to whom the right to suggest a name will be given. In 2011, the IUPAC has evaluated the 2004 RIKEN experiments and 2004 and 2007 Dubna experiments, and concluded that they did not meet the criteria for discovery.[8]

The following names have been suggested by the above-mentioned teams claiming discovery:

Group Proposed Name Derivation
RIKEN Japonium[9] Japan: country of group claimants
Rikenium[9] RIKEN: institute of group claimants
Dubna team Becquerelium Henri Becquerel, French physicist

[edit] Nucleosynthesis

Target-projectile combinations leading to Z=113 compound nuclei

The below table contains various combinations of targets and projectiles (both at max no. of neutrons) which could be used to form compound nuclei with an atomic number of 113.

Target Projectile CN Attempt result
208Pb 71Ga 279Uut Reaction yet to be attempted
209Bi 70Zn 279Uut Successful reaction
232Th 51V 283Uut Reaction yet to be attempted
238U 45Sc 283Uut Reaction yet to be attempted
237Np 48Ca 285Uut Successful reaction
244Pu 41K 285Uut Reaction yet to be attempted
243Am 40Ar 283Uut Reaction yet to be attempted
248Cm 37Cl 285Uut Reaction yet to be attempted
249Bk 36S 285Uut Reaction yet to be attempted
249Cf 31P 280Uut Reaction yet to be attempted

[edit] Cold fusion

This section deals with the synthesis of nuclei of ununtrium by so-called "cold" fusion reactions. These are processes which create compound nuclei at low excitation energy (~10–20 MeV, hence "cold"), leading to a higher probability of survival from fission. The excited nucleus then decays to the ground state via the emission of one or two neutrons only.

209Bi(70Zn,xn)279-xUut (x=1)

The synthesis of ununtrium was first attempted in 1998 by the team at GSI using the above cold fusion reaction. In two separate runs, they were unable to detect any atoms and calculated a cross section limit of 900 fb.[10] They repeated the experiment in 2003 and lowered the limit further to 400 fb.[10] In late 2003, the emerging team at RIKEN using their efficient apparatus GARIS attempted the reaction and reached a limit of 140 fb. In December 2003 – August 2004, they resorted to 'brute force' and performed an eight-month-long irradiation in which they increased the sensitivity to 51 fb. They were able to detect a single atom of 278Uut.[4] They repeated the reaction in several runs in 2005 and were able to synthesize a second atom. They calculated a record-low 31 fb for the cross section for the 2 atoms. The reaction was repeated again in 2006 with two long production runs but no further atoms were detected. This lowered the yield further to the current value of just 23 fb.

[edit] Hot fusion

This section deals with the synthesis of nuclei of ununtrium by so-called "hot" fusion reactions. These are processes which create compound nuclei at high excitation energy (~40–50 MeV, hence "hot"), leading to a reduced probability of survival from fission. The excited nucleus then decays to the ground state via the emission of 3–5 neutrons. Fusion reactions utilizing 48Ca nuclei usually produce compound nuclei with intermediate excitation energies (~30–35 MeV) and are sometimes referred to as "warm" fusion reactions. This leads, in part, to relatively high yields from these reactions.

237Np(48Ca,xn)285-xUut (x=3)

In June 2006, the Dubna-Livermore team synthesised ununtrium directly in the "warm" fusion reaction between neptunium-237 and calcium-48 nuclei. Two atoms of 282Uut were detected with a cross section of 900 fb.[11]

[edit] As decay product

Ununtrium has also been detected in the decay of ununpentium and ununseptium.


[edit] Yields of isotopes

The table below provides cross-sections and excitation energies for cold fusion reactions producing ununtrium isotopes directly. Data in bold represent maxima derived from excitation function measurements. + represents an observed exit channel.

Projectile Target CN 1n 2n 3n
70Zn 209Bi 279Uut 23 fb

The table below provides cross-sections and excitation energies for hot fusion reactions producing ununtrium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.

Projectile Target CN 3n 4n 5n
48Ca 237Np 285Uut 0.9 pb, 39.1 MeV [11]

[edit] Theoretical calculations

The below table contains various targets-projectile combinations for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.

DNS = Di-nuclear system; σ = cross section

Target Projectile CN Channel (product) σmax Model Ref
209Bi 70Zn 279Uut 1n (278113) 30 fb DNS [12]
237Np 48Ca 285Uut 3n (282113) 0.4 pb DNS [13]

[edit] Isotopes and nuclear properties

Chronology of isotope discovery
Isotope Year discovered Discovery reaction
278Uut 2004 209Bi(70Zn,n) [4]
279Uut unknown
280Uut unknown
281Uut unknown
282Uut 2006 237Np(48Ca,3n)[11]
283Uut 2003 243Am(48Ca,4n)[2]
284Uut 2003 243Am(48Ca,3n)[2]
285Uut 2009 249Bk(48Ca,4n)[1]
286Uut 2009 249Bk(48Ca,3n)[1]

[edit] Chemical properties

[edit] Extrapolated chemical properties

[edit] Oxidation states

Ununtrium is projected to be the first member of the 7p series of elements and the heaviest member of group 13 (IIIA) in the Periodic Table, below thallium. Each of the members of this group show the group oxidation state of +III. However, thallium has a tendency to form only a stable +I state due to the "inert pair effect", explained by the relativistic stabilisation of the 7s-orbitals, resulting in a higher ionisation potential and weaker tendency to participate in bonding.

[edit] Chemistry

Ununtrium should portray eka-thallium chemical properties and should therefore form a monoxide, Uut2O, and monohalides, UutF, UutCl, UutBr, and UutI. If the +III state is accessible, it is likely that it is only possible in the oxide, Uut2O3, and fluoride, UutF3. Spin-orbit splitting of the 7p orbitals may stabilize the −1 state as well, as is seen with gold(−1) (aurides).

[edit] See also

[edit] References

  1. ^ a b c Oganessian, Yu. Ts.; Abdullin, F. Sh.; Bailey, P. D.; Benker, D. E.; Bennett, M. E.; Dmitriev, S. N.; Ezold, J. G.; Hamilton, J. H. et al (2010). "Synthesis of a New Element with Atomic Number Z=117". Physical Review Letters 104 (14). Bibcode 2010PhRvL.104n2502O. doi:10.1103/PhysRevLett.104.142502. PMID 20481935. 
  2. ^ a b c "Experiments on the synthesis of element 115 in the reaction 243Am(48Ca,xn)291-x115", Oganessian et al., JINR Preprints, 2003. Retrieved on 3 March 2008
  3. ^ Oganessian, Yu. Ts.; Utyonkoy, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Shirokovsky, I.; Tsyganov, Yu.; Gulbekian, G. et al (2004). "Experiments on the synthesis of element 115 in the reaction 243Am(48Ca,xn)291-x115". Physical Review C 69 (2): 021601. Bibcode 2004PhRvC..69b1601O. doi:10.1103/PhysRevC.69.021601. 
  4. ^ a b c Morita, Kosuke; Morimoto, Kouji; Kaji, Daiya; Akiyama, Takahiro; Goto, Sin-Ichi; Haba, Hiromitsu; Ideguchi, Eiji; Kanungo, Rituparna et al (2004). "Experiment on the Synthesis of Element 113 in the Reaction 209Bi(70Zn, n)278113". Journal of the Physical Society of Japan 73 (10): 2593. Bibcode 2004JPSJ...73.2593M. doi:10.1143/JPSJ.73.2593. 
  5. ^ "Results of the experiment on chemical identification of Db as a decay product of element 115", Oganessian et al., JINR preprints, 2004. Retrieved on 3 March 2008
  6. ^ Oganessian, Yu. Ts.; Utyonkov, V.; Dmitriev, S.; Lobanov, Yu.; Itkis, M.; Polyakov, A.; Tsyganov, Yu.; Mezentsev, A. et al (2005). "Synthesis of elements 115 and 113 in the reaction 243Am + 48Ca". Physical Review C 72 (3): 034611. Bibcode 2005PhRvC..72c4611O. doi:10.1103/PhysRevC.72.034611. 
  7. ^ P. Roy Chowdhury, D. N. Basu and C. Samanta (2007). "α decay chains from element 113". Phys. Rev. C 75 (4): 047306. Bibcode 2007PhRvC..75d7306C. doi:10.1103/PhysRevC.75.047306. 
  8. ^ Barber, Robert C.; Karol, Paul J.; Nakahara, Hiromichi; Vardaci, Emanuele; Vogt, Erich W. (2011). "Discovery of the elements with atomic numbers greater than or equal to 113 (IUPAC Technical Report)". Pure and Applied Chemistry: 1. doi:10.1351/PAC-REP-10-05-01. 
  9. ^ a b "RIKEN NEWS November 2004". http://www.riken.go.jp/engn/r-world/info/release/news/2004/nov/index.html. Retrieved 9 February 2008. 
  10. ^ a b "Search for element 113", Hofmann et al., GSI report 2003. Retrieved on 3 March 2008
  11. ^ a b c Oganessian et al.; Utyonkov, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Sagaidak, R.; Shirokovsky, I.; Tsyganov, Yu. et al (2007). "Synthesis of the isotope 282113 in the 237Np+48Ca fusion reaction". Phys. Rev. C 76: 011601(R). Bibcode 2007PhRvC..76a1601O. doi:10.1103/PhysRevC.76.011601. http://nrv.jinr.ru/pdf_file/PhysRevC_76_011601.pdf. 
  12. ^ Feng, Zhao-Qing; Jin, Gen-Ming; Li, Jun-Qing; Scheid, Werner (2007). "Formation of superheavy nuclei in cold fusion reactions". Physical Review C 76 (4): 044606. arXiv:0707.2588. Bibcode 2007PhRvC..76d4606F. doi:10.1103/PhysRevC.76.044606. 
  13. ^ Feng, Z; Jin, G; Li, J; Scheid, W (2009). "Production of heavy and superheavy nuclei in massive fusion reactions". Nuclear Physics A 816: 33. arXiv:0803.1117. Bibcode 2009NuPhA.816...33F. doi:10.1016/j.nuclphysa.2008.11.003. 

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