Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Isotopes of moscovium

From Wikipedia, the free encyclopedia

Isotopes ofmoscovium (115Mc)
Main isotopesDecay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
286Mcsynth20 ms[1]α282Nh
287Mcsynth38 msα283Nh
288Mcsynth193 msα284Nh
289Mcsynth250 ms[2][3]α285Nh
290Mcsynth650 ms[2][3]α286Nh

Moscovium (115Mc) is asynthetic element, and thus astandard atomic weight cannot be given. Like all synthetic elements, it has no knownstable isotopes. The firstisotope to be synthesized was288Mc in 2004. There are five knownradioisotopes from286Mc to290Mc. The longest-lived isotope is290Mc with ahalf-life of 0.65 seconds.

List of isotopes

[edit]


The isotopes undergoalpha decay into the correspondingisotope of nihonium, with half-lives increasing as neutron numbers increase.

Nuclide
ZNIsotopic mass(Da)[4]
[n 1][n 2]
Half-life[5]
Decay
mode
[5]
Daughter
isotope

Spin and
parity[5]
286Mc[6]11517120+98
−9
 ms
α282Nh
287Mc115172287.19082(48)#38+22
−10
 ms
[6]
α283Nh
288Mc115173288.19288(58)#193+15
−13
 ms
[6]
α284Nh
289Mc115174289.19397(83)#250+51
−35
 ms
[6]
α285Nh
290Mc[n 3]115175290.19624(64)#650+490
−200
 ms

[0.84(36) s]
α286Nh
This table header & footer:
  1. ^( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  2. ^# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  3. ^Not directly synthesized, created as decay product of294Ts

Nucleosynthesis

[edit]
Chronology of isotope discovery
IsotopeYear discoveredDiscovery reaction
286Mc2021243Am(48Ca,5n)
287Mc2003243Am(48Ca,4n)
288Mc2003243Am(48Ca,3n)
289Mc2009249Bk(48Ca,4n)[2]
290Mc2009249Bk(48Ca,3n)[2]

Target-projectile combinations

[edit]

The table below contains various combinations of targets and projectiles which could be used to form compound nuclei withZ = 115. Each entry is a combination for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.

TargetProjectileCNAttempt result
208Pb75As283McReaction yet to be attempted
209Bi76Ge285McReaction yet to be attempted
238U51V289McFailure to date
243Am48Ca291Mc[7][8]Successful reaction
241Am48Ca289McPlanned reaction
243Am44Ca287McReaction yet to be attempted

Hot fusion

[edit]

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 utilizing48Ca 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−xMc

[edit]

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 product atoms were detected, as anticipated by the team.[9]

243Am(48Ca,xn)291−xMc (x=2,3,4,5)

[edit]

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 of288Mc and a single atom of287Mc. The reaction was studied further in June 2004 in an attempt to isolate the descendant268Db from the288Mc decay chain. After chemical separation of a +4/+5 fraction, 15 SF decays were measured with a lifetime consistent with268Db. 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 niobium-like 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 of288Mc and one atom of289Mc, from the 2n exit channel. This latter result was used to support the synthesis oftennessine. 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.

This reaction was run again at five different energies in 2021 to test the new gas-filled separator at Dubna's SHE-factory. They detected 6 chains of289Mc, 58 chains of288Mc, and 2 chains of287Mc. For the first time the 5n channel was observed with 2 atoms of286Mc.[10]

242Pu(50Ti,pxn)291−xMc (x=2)

[edit]

This reaction was studied by the team in Dubna in 2024. For the first time, a pxn reaction was successful with actinide targets and48Ca/50Ti/54Cr projectiles, producing one atom of the known289Mc in the p2n channel (evaporating one proton and two neutrons).[11]

Reaction yields

[edit]

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

ProjectileTargetCN2n3n4n5n
48Ca243Am291Mc3.7 pb, 39.0 MeV0.9 pb, 44.4 MeV

Theoretical calculations

[edit]

Decay characteristics

[edit]

Theoretical calculations using a quantum-tunneling model support the experimental alpha-decay half-lives.[12]

Evaporation residue cross sections

[edit]

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

TargetProjectileCNChannel (product)σmaxModelRef
243Am48Ca291Mc3n (288Mc)3 pbMD[7]
243Am48Ca291Mc4n (287Mc)2 pbMD[7]
243Am48Ca291Mc3n (288Mc)1 pbDNS[8]
242Am48Ca290Mc3n (287Mc)2.5 pbDNS[8]
241Am48Ca289Mc4n (285Mc)1.04 pbDNS[13]

References

[edit]
  1. ^Kovrizhnykh, N. (27 January 2022)."Update on the experiments at the SHE Factory". Flerov Laboratory of Nuclear Reactions. Retrieved28 February 2022.
  2. ^abcdOganessian, Yuri Ts.; Abdullin, F. Sh.; Bailey, P. D.; et al. (2010-04-09)."Synthesis of a New Element with Atomic NumberZ=117".Physical Review Letters.104 142502.Bibcode:2010PhRvL.104n2502O.doi:10.1103/PhysRevLett.104.142502.PMID 20481935.
  3. ^abOganessian, Y.T. (2015)."Super-heavy element research".Reports on Progress in Physics.78 (3) 036301.Bibcode:2015RPPh...78c6301O.doi:10.1088/0034-4885/78/3/036301.PMID 25746203.S2CID 37779526.
  4. ^Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*".Chinese Physics C.45 (3) 030003.doi:10.1088/1674-1137/abddaf.
  5. ^abcKondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021)."The NUBASE2020 evaluation of nuclear properties"(PDF).Chinese Physics C.45 (3) 030001.doi:10.1088/1674-1137/abddae.
  6. ^abcdOganessian, Yu. Ts.; Utyonkov, V. K.; Kovrizhnykh, N. D.; et al. (2022)."New isotope286Mc produced in the243Am+48Ca reaction".Physical Review C.106 (64306) 064306.Bibcode:2022PhRvC.106f4306O.doi:10.1103/PhysRevC.106.064306.S2CID 254435744.
  7. ^abcZagrebaev, 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.
  8. ^abcFeng, Z; Jin, G; Li, J; Scheid, W (2009). "Production of heavy and superheavy nuclei in massive fusion reactions".Nuclear Physics A.816 (1–4):33–51.arXiv:0803.1117.Bibcode:2009NuPhA.816...33F.doi:10.1016/j.nuclphysa.2008.11.003.S2CID 18647291.
  9. ^"List of experiments 2000–2006".Univerzita Komenského v Bratislave. Archived fromthe original on July 23, 2007.
  10. ^"Both neutron properties and new results at SHE Factory".
  11. ^Ibadullayev, Dastan (2024)."Synthesis and study of the decay properties of isotopes of superheavy element Lv in Reactions238U +54Cr and242Pu +50Ti".jinr.ru.Joint Institute for Nuclear Research. Retrieved2 November 2024.
  12. ^C. Samanta; P. Roy Chowdhury; D. N. Basu (2007). "Predictions of alpha decay half lives of heavy and superheavy elements".Nucl. Phys. A.789 (1–4):142–154.arXiv:nucl-th/0703086.Bibcode:2007NuPhA.789..142S.doi:10.1016/j.nuclphysa.2007.04.001.S2CID 7496348.
  13. ^Zhu, L.; Su, J.; Zhang, F. (2016)."Influence of the neutron numbers of projectile and target on the evaporation residue cross sections in hot fusion reactions".Physical Review C.93 (6) 064610.Bibcode:2016PhRvC..93f4610Z.doi:10.1103/PhysRevC.93.064610.
Group12 3456789101112131415161718
PeriodHydrogen and
alkali metals
Alkaline
earth metals
Pnicto­gensChal­co­gensHalo­gensNoble gases
12
345678910
1112131415161718
192021222324252627282930313233343536
373839404142434445464748495051525354
55561 asterisk71727374757677787980818283848586
87881 asterisk103104105106107108109110111112113114115116117118
119120
1 asterisk5758596061626364656667686970 
1 asterisk8990919293949596979899100101102
Retrieved from "https://en.wikipedia.org/w/index.php?title=Isotopes_of_moscovium&oldid=1322563285"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp