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词条 Isotopes of tennessine
释义

  1. List of isotopes

      Notes  

  2. Isotopes and nuclear properties

     Nucleosynthesis  Target-projectile combinations leading to Z=117 compound nuclei  Hot fusion  249Bk (48Ca, xn)297−xTs (x=3,4)  Chronology of isotope discovery  Theoretical calculations  Evaporation residue cross sections  Decay characteristics 

  3. References

  4. External sources

{{infobox tennessine isotopes}}

Tennessine (117Ts) is the most-recently synthesized synthetic element, and much of the data is hypothetical. As for any synthetic element, a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first (and so far only) isotopes to be synthesized were 293Ts and 294Ts in 2009. The longer-lived isotope is 294Ts with a half-life of 51 ms.

List of isotopes

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)
 
half-life decay mode(s) daughter
isotope(s)
nuclear
spin and
parity

293Ts117176 293.20824(89)# 22 (+8−4) ms[1] α 289Mc
294Ts117177 294.21046(74)# 51 (+41−16) ms[2] α 290Mc

Notes

  • Values marked # are not purely derived from experimental data, but at least partly from systematic trends.
  • Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values from Ame2003 denote one standard deviation. Values from IUPAC are expanded uncertainties.

Isotopes and nuclear properties

Nucleosynthesis

Target-projectile combinations leading to Z=117 compound nuclei

The below table contains various combinations of targets and projectiles that could be used to form compound nuclei with atomic number 117.

Target Projectile CN Attempt result
208Pb81Br289TsReaction yet to be attempted}}
209Bi82Se291TsReaction yet to be attempted}}
238U55Mn293TsReaction yet to be attempted}}
243Am50Ti293TsPlanned reaction}}
249Bk48Ca297TsSuccessful reaction}}

Hot fusion

249Bk (48Ca, xn)297−xTs (x=3,4)

Between July 2009 and February 2010, the team at the JINR (Flerov Laboratory of Nuclear Reactions) ran a 7-month-long experiment to synthesize tennessine using the reaction above.[3]

The expected cross-section was of the order of 2 pb. The expected evaporation residues, 293Ts and 294Ts, were predicted to decay via relatively long decay chains as far as isotopes of dubnium or lawrencium.


The team published a scientific paper in April 2010 (first results were presented in January 2010[5]) that six atoms of the neighbouring isotopes 294Ts (one atom) and 293Ts (five atoms) were detected. The heavier isotope decayed by the successive emission of six alpha particles down as far as the new isotope 270Db, which underwent apparent spontaneous fission. On the other hand, the lighter odd-even isotope decayed by the emission of just three alpha particles, as far as 281Rg, which underwent spontaneous fission. The reaction was run at two different excitation energies of 35 MeV (dose 2×1019) and 39 MeV (dose 2.4×1019). Initial decay data was published as a preliminary presentation on the JINR website.[6]

A further experiment in May 2010, aimed at studying the chemistry of the granddaughter of tennessine, nihonium, identified a further two atoms of 286Nh from the decay of 294Ts.

Chronology of isotope discovery

IsotopeYear discoveredDiscovery reaction
294Ts2009249Bk(48Ca,3n)
293Ts2009249Bk(48Ca,4n)

Theoretical calculations

Evaporation residue cross sections

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
209Bi82Se291Ts1n (290Ts)15 fbDNS[7]
209Bi79Se288Ts1n (287Ts)0.2 pbDNS[7]
232Th59Co291Ts2n (289Ts)0.1 pbDNS[7]
238U55Mn293Ts2-3n (291,290Ts)70 fbDNS[7]
244Pu51V295Ts3n (292Ts)0.6 pbDNS[7]
248Cm45Sc293Ts4n (289Ts)2.9 pbDNS[7]
246Cm45Sc291Ts4n (287Ts)1 pbDNS[7]
249Bk48Ca297Ts3n (294Ts)2.1 pb ; 3 pbDNS[7][8]
247Bk48Ca295Ts3n (292Ts)0.8, 0.9 pbDNS[7][8]

Decay characteristics

Theoretical calculations in a quantum tunneling model with mass estimates from a macroscopic-microscopic model predict the alpha-decay half-lives of isotopes of tennessine (namely, 289–303Ts) to be around 0.1–40 ms.[9][10][11]

References

1. ^{{cite journal |last1=Oganessian |first1=Yu. Ts. |year=2013 |title=Experimental studies of the 249Bk + 48Ca reaction including decay properties and excitation function for isotopes of element 117, and discovery of the new isotope 277Mt |journal=Physical Review C |volume=87 |issue=5 |pages=054621 |bibcode=2013PhRvC..87e4621O |doi=10.1103/PhysRevC.87.054621|display-authors=etal}}
2. ^{{cite journal |last1=Khuyagbaatar |first1=J. |last2=Yakushev |first2=A. |last3=Düllmann |first3=Ch. E. |title=48Ca+249Bk Fusion Reaction Leading to Element Z=117: Long-Lived α-Decaying 270Db and Discovery of 266Lr |journal=Physical Review Letters |volume=112 |issue=17 |pages=172501 |year=2014 |doi=10.1103/PhysRevLett.112.172501 |display-authors=etal |pmid=24836239|bibcode=2014PhRvL.112q2501K }}
3. ^Tennessine – the 117th element at AtomInfo.ru
4. ^{{cite web |author=Roman Sagaidak |title=Experiment setting on synthesis of superheavy nuclei in fusion-evaporation reactions. Preparation to synthesis of new element with Z=117 |url=http://159.93.28.88/linkc/education/SHE_Sagaidak.pdf |accessdate=2009-07-07}}
5. ^Recommendations: 31st meeting, PAC for Nuclear Physics {{webarchive|url=https://web.archive.org/web/20100414173735/http://www.jinr.ru/img_sections/PAC/NP/31/PAK_NP_31_recom_eng.pdf |date=2010-04-14 }}
6. ^Walter Grenier: Recommendations, a PowerPoint presentation at the January 2010 meeting of the PAC for Nuclear Physics
7. ^{{cite journal |arxiv=0708.0159 |doi=10.1088/0256-307X/24/9/024 |title=Possible Way to Synthesize Superheavy Element Z = 117 |year=2007 |last=Zhao-Qing |first=Feng |journal=Chinese Physics Letters |volume=24 |page=2551 |last2=Gen-Ming |first2=Jin |last3=Ming-Hui |first3=Huang |last4=Zai-Guo |first4=Gan |last5=Nan |first5=Wang |last6=Jun-Qing |first6=Li |issue=9 |bibcode = 2007ChPhL..24.2551F }}
8. ^{{cite journal |arxiv=0803.1117 |doi=10.1016/j.nuclphysa.2008.11.003 |title=Production of heavy and superheavy nuclei in massive fusion reactions |year=2009 |last=Feng |first=Z |journal=Nuclear Physics A |volume=816 |issue=1–4 |page=33 |last2=Jin |first2=G |last3=Li |first3=J |last4=Scheid |first4=W |bibcode=2009NuPhA.816...33F}}
9. ^{{cite journal |journal=Nuclear Physics A |volume=789 |issue=1–4 |pages=142–154 |year=2007 |title=Predictions of alpha decay half lives of heavy and superheavy elements |author=C. Samanta |author2=P. Roy Chowdhury |author3=D. N. Basu |doi=10.1016/j.nuclphysa.2007.04.001 |bibcode=2007NuPhA.789..142S |arxiv = nucl-th/0703086 }}
10. ^{{cite journal |journal=Physical Review C |volume=77 |page=044603 |year=2008|title=Search for long lived heaviest nuclei beyond the valley of stability |author=P. Roy Chowdhury |author2=C. Samanta |author3=D. N. Basu |doi=10.1103/PhysRevC.77.044603 |bibcode=2008PhRvC..77d4603C |issue=4 |arxiv = 0802.3837 }}
11. ^{{cite journal |journal=Atomic Data and Nuclear Data Tables |volume=94 |pages=781–806 |year=2008 |title=Nuclear half-lives for α -radioactivity of elements with 100 ≤ Z ≤ 130 |author=P. Roy Chowdhury |author2=C. Samanta |author3=D. N. Basu |doi=10.1016/j.adt.2008.01.003 |bibcode=2008ADNDT..94..781C |issue=6 |arxiv = 0802.4161 }}

External sources

  • Isotope masses from:
    • {{cite journal |author=M. Wang |author2=G. Audi |author3=A. H. Wapstra |author4=F. G. Kondev |author5=M. MacCormick |author6=X. Xu|year=2012 |title=The AME2012 atomic mass evaluation (II). Tables, graphs and references. |url=http://amdc.in2p3.fr/masstables/Ame2012/Ame2012b-v2.pdf |journal=Chinese Physics C |volume=36 |issue= 12 |pages=1603–2014 |doi=10.1088/1674-1137/36/12/003|bibcode = 2012ChPhC..36....3M |display-authors=etal}}
    • {{NUBASE 2003}}
  • Isotopic compositions and standard atomic masses from:
    • {{CAWIA 2003}}
{{Navbox element isotopes}}

3 : Tennessine|Isotopes of tennessine|Lists of isotopes by element

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