Isotopes of moscovium: Difference between revisions
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====<sup>238</sup>U(<sup>51</sup>V,''x''n)<sup>289−''x''</sup>Uup==== |
====<sup>238</sup>U(<sup>51</sup>V,''x''n)<sup>289−''x''</sup>Uup==== |
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There are strong indications that this reaction was performed in late 2004 as part of a uranium(IV) fluoride target test at the GSI. No reports have been published suggesting that no products atoms were detected, as anticipated by the team.<ref>{{cite web|url= |
There are strong indications that this reaction was performed in late 2004 as part of a uranium(IV) fluoride target test at the GSI. No reports have been published suggesting that no products atoms were detected, as anticipated by the team.<ref>{{cite web|url=http://opal.dnp.fmph.uniba.sk/~beer/experiments.php |work=Univerzita Komenského v Bratislave |title=List of experiments 2000–2006 |deadurl=yes |archiveurl=https://web.archive.org/web/20070723094218/http://opal.dnp.fmph.uniba.sk/~beer/experiments.php |archivedate=July 23, 2007 }}</ref> |
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====<sup>243</sup>Am(<sup>48</sup>Ca,''x''n)<sup>291−''x''</sup>Uup (x=2,3,4)==== |
====<sup>243</sup>Am(<sup>48</sup>Ca,''x''n)<sup>291−''x''</sup>Uup (x=2,3,4)==== |
Revision as of 02:35, 1 April 2016
Ununpentium (Uup) is a synthetic element, and thus a standard atomic mass cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 288Uup in 2004. There are four known radioisotopes from 287Uup to 290Uup.
Table
nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | decay mode(s) | daughter isotope(s) |
nuclear spin |
---|---|---|---|---|---|---|---|
287Uup | 115 | 172 | 287.19070(52)# | 32(+155−14) ms | α | 283Uut | |
288Uup | 115 | 173 | 288.19274(62)# | 87(+105−30) ms | α | 284Uut | |
289Uup[n 1] | 115 | 174 | 289.19363(89)# | 220 ms[1] | α | 285Uut | |
290Uup[n 2] | 115 | 175 | 290.19598(73)# | 16 ms[1] | α | 286Uut |
- ^ Not directly synthesized, created as decay product of 293Uus
- ^ Not directly synthesized, created as decay product of 294Uus
Notes
- Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
- Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC, which use expanded uncertainties.
Nucleosynthesis
Isotope | Year discovered | Discovery reaction |
---|---|---|
287Uup | 2003 | 243Am(48Ca,4n) |
288Uup | 2003 | 243Am(48Ca,3n) |
289Uup | 2009 | 249Bk(48Ca,4n)[1] |
290Uup | 2009 | 249Bk(48Ca,3n)[1] |
Target-projectile combinations
The table below contains various combinations of targets and projectiles which could be used to form compound nuclei with Z=115. Each entry is acombination for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.
Target | Projectile | CN | Attempt result |
---|---|---|---|
208Pb | 75As | 283Uup | Reaction yet to be attempted |
232Th | 55Mn | 287Uup | Reaction yet to be attempted |
238U | 51V | 289Uup | Failure to date |
237Np | 50Ti | 287Uup | Reaction yet to be attempted |
244Pu | 45Sc | 289Uup | Reaction yet to be attempted |
243Am | 48Ca | 291Uup[2][3] | Successful reaction |
241Am | 48Ca | 289Uup | Planned Reaction |
248Cm | 41K | 289Uup | Reaction yet to be attempted |
249Bk | 40Ar | 289Uup | Reaction yet to be attempted |
249Cf | 37Cl | 286Uup | Reaction yet to be attempted |
Hot fusion
Hot fusion reactions are processes that 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.
238U(51V,xn)289−xUup
There are strong indications that this reaction was performed in late 2004 as part of a uranium(IV) fluoride target test at the GSI. No reports have been published suggesting that no products atoms were detected, as anticipated by the team.[4]
243Am(48Ca,xn)291−xUup (x=2,3,4)
This reaction was first performed by the team in Dubna in July–August 2003. In two separate runs they were able to detect 3 atoms of 288Uup and a single atom of 287Uup. The reaction was studied further in June 2004 in an attempt to isolate the descendant 268Db from the 288Uup decay chain. After chemical separation of a +4/+5 fraction, 15 SF decays were measured with a lifetime consistent with 268Db. In order to prove that the decays were from dubnium-268, the team repeated the reaction in August 2005 and separated the +4 and +5 fractions and further separated the +5 fractions into tantalum-like and niobium-like ones. Five SF activities were observed, all occurring in the +5 fractions and none in the tantalum-like fractions, proving that the product was indeed isotopes of dubnium.
In a series of experiments between October 2010 – February 2011, scientists at the FLNR studied this reaction at a range of excitation energies. They were able to detect 21 atoms of 288115 and one atom of 289115, from the 2n exit channel. This latter result was used to support the synthesis of ununseptium. The 3n excitation function was completed with a maximum at ~8 pb. The data was consistent with that found in the first experiments in 2003.
Reaction yields
The table below provides cross-sections and excitation energies for hot fusion reactions producing ununpentium 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 | 243Am | 291Uup | 3.7 pb, 39.0 MeV | 0.9 pb, 44.4 MeV |
Theoretical calculations
Decay characteristics
Theoretical calculations using a quantum-tunneling model support the experimental alpha-decay half-lives.[5]
Evaporation residue cross sections
The table below contains various target-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.
MD = multi-dimensional; DNS = Di-nuclear system; σ = cross section
Target | Projectile | CN | Channel (product) | σmax | Model | Ref |
---|---|---|---|---|---|---|
243Am | 48Ca | 291Uup | 3n (288Uup) | 3 pb | MD | [2] |
243Am | 48Ca | 291Uup | 4n (287Uup) | 2 pb | MD | [2] |
243Am | 48Ca | 291Uup | 3n (288Uup) | 1 pb | DNS | [3] |
242Am | 48Ca | 290Uup | 3n (287Uup) | 2.5 pb | DNS | [3] |
References
- ^ a b c d Oganessian, Yuri Ts.; Abdullin, F. Sh.; Bailey, P. D.; Benker, D. E.; Bennett, M. E.; Dmitriev, S. N.; Ezold, J. G.; Hamilton, J. H.; Henderson, R. A. (2010-04-09). "Synthesis of a New Element with Atomic Number Z=117". Physical Review Letters. 104 (142502). American Physical Society: 142502. Bibcode:2010PhRvL.104n2502O. doi:10.1103/PhysRevLett.104.142502. PMID 20481935.
{{cite journal}}
: Unknown parameter|displayauthors=
ignored (|display-authors=
suggested) (help) - ^ a b c Zagrebaev, V. (2004). "Fusion-fission dynamics of super-heavy element formation and decay" (PDF). Nuclear Physics A. 734: 164–167. Bibcode:2004NuPhA.734..164Z. doi:10.1016/j.nuclphysa.2004.01.025.
- ^ a b c Feng, Z; Jin, G; Li, J; Scheid, W (2009). "Production of heavy and superheavy nuclei in massive fusion reactions". Nuclear Physics A. 816: 33–51. arXiv:0803.1117. Bibcode:2009NuPhA.816...33F. doi:10.1016/j.nuclphysa.2008.11.003.
- ^ "List of experiments 2000–2006". Univerzita Komenského v Bratislave. Archived from the original on July 23, 2007.
{{cite web}}
: Unknown parameter|deadurl=
ignored (|url-status=
suggested) (help) - ^ C. Samanta; P. Roy Chowdhury; D. N. Basu (2007). "Predictions of alpha decay half lives of heavy and superheavy elements". Nucl. Phys. A. 789: 142–154. arXiv:nucl-th/0703086. Bibcode:2007NuPhA.789..142S. doi:10.1016/j.nuclphysa.2007.04.001.
- Isotope masses from:
- M. Wang; G. Audi; A. H. Wapstra; F. G. Kondev; M. MacCormick; X. Xu; et al. (2012). "The AME2012 atomic mass evaluation (II). Tables, graphs and references" (PDF). Chinese Physics C. 36 (12): 1603–2014. Bibcode:2012ChPhC..36....3M. doi:10.1088/1674-1137/36/12/003.
- G. Audi; A. H. Wapstra; C. Thibault; J. Blachot; O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.
- Isotopic compositions and standard atomic masses from:
- J. R. de Laeter; J. K. Böhlke; P. De Bièvre; H. Hidaka; H. S. Peiser; K. J. R. Rosman; P. D. P. Taylor (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry. 75 (6): 683–800. doi:10.1351/pac200375060683.
- M. E. Wieser (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure and Applied Chemistry. 78 (11): 2051–2066. doi:10.1351/pac200678112051.
{{cite journal}}
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ignored (help)
- Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
- G. Audi; A. H. Wapstra; C. Thibault; J. Blachot; O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.
- National Nuclear Data Center. "NuDat 2.1 database". Brookhaven National Laboratory. Retrieved September 2005.
{{cite web}}
: Check date values in:|accessdate=
(help) - N. E. Holden (2004). "Table of the Isotopes". In D. R. Lide (ed.). CRC Handbook of Chemistry and Physics (85th ed.). CRC Press. Section 11. ISBN 978-0-8493-0485-9.
{{cite book}}
: Unknown parameter|nopp=
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