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Isotopes of livermorium

From Wikipedia, the free encyclopedia

Isotopes oflivermorium (116Lv)
Main isotopes[1]Decay
abun­dancehalf-life(t1/2)modepro­duct
290Lvsynth9 msα286Fl
SF
291Lvsynth26 msα287Fl
292Lvsynth16 msα288Fl
293Lvsynth70 msα289Fl
293mLvsynth80 msα?

Livermorium (116Lv) is asynthetic element, and thus astandard atomic weight cannot be given. Like all artificial elements, it has nostable isotopes. The firstisotope to be synthesized was293Lv in 2000. There are six knownradioisotopes, withmass numbers 288–293, as well as a few suggestive indications of a possible heavier isotope294Lv. The longest-lived known isotope is293Lv with ahalf-life of 70 ms.[2]

List of isotopes

[edit]


Nuclide
[n 1]
ZNIsotopic mass(Da)[3]
[n 2][n 3]
Half-life[1]
[n 4]
Decay
mode
[1]
Daughter
isotope

Spin and
parity[1]
Excitation energy[n 4]
288Lv[4]116172<1 msα284Fl0+
289Lv[5]116173289.19802(54)#α285Fl
290Lv116174290.19864(59)#9(3) msα286Fl0+
291Lv116175291.20101(67)#26(12) msα287Fl
292Lv116176292.20197(82)#16(6) msα288Fl0+
293Lv116177293.20458(55)#70(30) msα289Fl
293mLv[n 5]720(290)# keV80(60) msα
294Lv[n 6]11617854# ms[6]α ?290Fl0+
This table header & footer:
  1. ^mLv – Excitednuclear isomer.
  2. ^( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  3. ^# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  4. ^ab# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  5. ^This isomer is unconfirmed
  6. ^This isotope is unconfirmed

Nucleosynthesis

[edit]

Target-projectile combinations leading to Z=116 compound nuclei

[edit]

The below table contains various combinations of targets and projectiles which could be used to form compound nuclei with atomic number 116.

TargetProjectileCNAttempt result
208Pb82Se290LvFailure to date
238U54Cr292LvSuccessful reaction
244Pu50Ti294LvSuccessful reaction
242Pu50Ti292LvSuccessful reaction
250Cm48Ca298LvReaction yet to be attempted
248Cm48Ca296LvSuccessful reaction
246Cm48Ca294LvReaction yet to be attempted
245Cm48Ca293LvSuccessful reaction
243Cm48Ca291LvReaction yet to be attempted
248Cm44Ca292LvReaction yet to be attempted
251Cf40Ar291LvReaction yet to be attempted

Cold fusion

[edit]

208Pb(82Se,xn)290−xLv

[edit]

In 1995, the team at GSI attempted the synthesis of290Lv as a radiative capture (x=0) product. Noatoms were detected during a six-week experimental run, reaching a cross section limit of 3 pb.[7]

Hot fusion

[edit]

This section deals with the synthesis of nuclei of livermorium 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 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(54Cr,xn)292−xLv (x=4)

[edit]

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 for238U targets.[8]

In 2023, this reaction was studied again at the JINR's Superheavy Element Factory in Dubna, in preparation for a future synthesis attempt ofelement 120 using54Cr projectiles. One atom of288Lv was reported; it underwent alpha decay with a lifetime of less than 1 millisecond. Further analysis of the reaction and its cross section are underway.[4]

244Pu(50Ti,xn)294−xLv (x=4)

[edit]

In 2024, this reaction was performed at the LBNL, in preparation for a future synthesis attempt of element 120 using50Ti projectiles. Two atoms of the known isotope290Lv were successfully produced.[9][10][11] This was the first successful synthesis of a superheavy element using50Ti projectiles and an actinide target; the cross section was reported to be0.44+0.58
−0.28
 pb
.[12]

242Pu(50Ti,xn)292−xLv (x=3,4)

[edit]

In 2024, this reaction was studied at the JINR, as a next step after the successful238U+54Cr reaction. Two atoms of288Lv were detected, as well as three atoms of the new alpha-decaying isotope289Lv. One atom of289Mc was found in the p2n channel, which was the first time any pxn channel had been detected in a reaction of actinides with48Ca,50Ti, or54Cr projectiles.[5]

248Cm(48Ca,xn)296−xLv (x=2?,3,4,5?)

[edit]

The first attempt to synthesise livermorium 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 livermorium.[13] Yuri Oganessian and his team at the Flerov Laboratory of Nuclear Reactions (FLNR) subsequently attempted the reaction in 1978 and met 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.[14]

In 2000, Russian scientists at Dubna finally succeeded in detecting a single atom of livermorium, assigned to the isotope292Lv.[15]In 2001, they repeated the reaction and formed a further 2 atoms in a confirmation of their discovery experiment. A third atom was tentatively assigned to293Lv on the basis of a missed parental alpha decay.[16]In April 2004, the team ran the experiment again at higher energy and were able to detect a new decay chain, assigned to292Lv. On this basis, the original data were reassigned to293Lv. The tentative chain is therefore possibly associated with a rare decay branch of this isotope or an isomer,293mLv; given the possible reassignment of its daughter to290Fl instead of289Fl, it could also conceivably be294Lv, although all these assignments are tentative and need confirmation in future experiments aimed at the 2n channel.[17][18] In this reaction, two additional atoms of293Lv were detected.[19]

In 2007, in a GSI-SHIP experiment, besides four292Lv chains and one293Lv chain, another chain was observed, initially not assigned but later shown to be291Lv. However, it is unclear whether it comes from the248Cm(48Ca,5n) reaction or from a reaction with a lighter curium isotope (present in the target as an admixture), such as246Cm(48Ca,3n).[20][21]

In an experiment run at the GSI during June–July 2010, scientists detected six atoms of livermorium; two atoms of293Lv and four atoms of292Lv. They were able to confirm both the decay data and cross sections for the fusion reaction.[22]

A 2016 experiment atRIKEN aimed at studying the48Ca+248Cm reaction seemingly detected one atom that may be assigned to294Lv alpha decaying to290Fl and286Cn, which underwent spontaneous fission; however, the first alpha from the livermorium nuclide produced was missed.[6]

245Cm(48Ca,xn)293−xLv (x=2,3)

[edit]

In order to assist in the assignment of isotope mass numbers for livermorium, in March–May 2003 the Dubna team bombarded a245Cm target with48Ca ions. They were able to observe two new isotopes, assigned to291Lv and290Lv.[23] This experiment was successfully repeated in February–March 2005 where 10 atoms were created with identical decay data to those reported in the 2003 experiment.[24]

As a decay product

[edit]

Livermorium has also been observed in the decay ofoganesson. In October 2006 it was announced that three atoms of oganesson had been detected by the bombardment ofcalifornium-249 with calcium-48 ions, which then rapidly decayed into livermorium.[24]

The observation of the daughter290Lv allowed the assignment of the parent to294Og and confirmed the synthesis of oganesson.

Fission of compound nuclei with Z=116

[edit]

Several experiments have been performed between 2000 and 2006 at theFlerov Laboratory of Nuclear Reactions in Dubna studying the fission characteristics of thecompound nuclei296,294,290Lv. Four nuclear reactions have been used, namely248Cm+48Ca,246Cm+48Ca,244Pu+50Ti, and232Th+58Fe. The results have revealed how nuclei such as this fission predominantly by expelling closed shell nuclei such as132Sn (Z = 50,N = 82). It was also found that the yield for the fusion-fission pathway was similar between48Ca and58Fe projectiles, indicating a possible future use of58Fe projectiles in superheavy element formation. In addition, in comparative experiments synthesizing294Lv using48Ca and50Ti projectiles, the yield from fusion-fission was roughly three times smaller for50Ti, also suggesting a future use in SHE production.[25]

Retracted isotopes

[edit]

289Lv

[edit]

In 1999, researchers atLawrence Berkeley National Laboratory announced the synthesis of293Og (seeoganesson), in a paper published inPhysical Review Letters.[26] The claimed isotope289Lv decayed by 11.63 MeV alpha emission with a half-life of 0.64 ms. The following year, they published aretraction after other researchers were unable to duplicate the results.[27] 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 authorVictor Ninov. This isotope of livermorium was finally discovered in 2024 by the JINR, in the242Pu(50Ti,3n) reaction.[5]

Chronology of isotope discovery

[edit]
IsotopeYear discoveredDiscovery reaction
288Lv2023238U(54Cr,4n)[4]
289Lv2024242Pu(50Ti,3n)[5]
290Lv2002249Cf(48Ca,3n)[24]
291Lv2003245Cm(48Ca,2n)[23]
292Lv2004248Cm(48Ca,4n)[19]
293Lv2000248Cm(48Ca,3n)[15]
294Lv ??2016248Cm(48Ca,2n) ?

Yields of isotopes

[edit]

Hot fusion

[edit]

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

ProjectileTargetCN2n3n4n5n
48Ca248Cm296Lv1.1 pb, 38.9 MeV[19]3.3 pb, 38.9 MeV[19]
48Ca245Cm293Lv0.9 pb, 33.0 MeV[23]3.7 pb, 37.9 MeV[23]

Theoretical calculations

[edit]

Decay characteristics

[edit]

Theoretical calculation in a quantum tunneling model supports the experimental data relating to the synthesis of293Lv and292Lv.[28][29]

Evaporation residue cross sections

[edit]

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

TargetProjectileCNChannel (product)σmaxModelRef
208Pb82Se290Lv1n (289Lv)0.1 pbDNS[30]
208Pb79Se287Lv1n (286Lv)0.5 pbDNS[30]
238U54Cr292Lv2n (290Lv)0.1 pbDNS[31]
250Cm48Ca298Lv4n (294Lv)5 pbDNS[31]
248Cm48Ca296Lv4n (292Lv)2 pbDNS[31]
247Cm48Ca295Lv3n (292Lv)3 pbDNS[31]
245Cm48Ca293Lv3n (290Lv)1.5 pbDNS[31]
243Cm48Ca291Lv3n (288Lv)1.53 pbDNS[32]
248Cm44Ca292Lv4n (288Lv)0.43 pbDNS[32]

References

[edit]
  1. ^abcdKondev, 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.
  2. ^"Livermorium - Element Information (Uses and properties)".rsc.org. RetrievedOctober 27, 2020.
  3. ^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.
  4. ^abc"В ЛЯР ОИЯИ впервые в мире синтезирован ливерморий-288" [Livermorium-288 was synthesized for the first time in the world at FLNR JINR] (in Russian). Joint Institute for Nuclear Research. 23 October 2023. Retrieved18 November 2023.
  5. ^abcdIbadullayev, 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.
  6. ^abKaji, Daiya; Morita, Kosuke; Morimoto, Kouji; Haba, Hiromitsu; Asai, Masato; Fujita, Kunihiro; Gan, Zaiguo; Geissel, Hans; Hasebe, Hiroo; Hofmann, Sigurd; Huang, MingHui; Komori, Yukiko; Ma, Long; Maurer, Joachim; Murakami, Masashi; Takeyama, Mirei; Tokanai, Fuyuki; Tanaka, Taiki; Wakabayashi, Yasuo; Yamaguchi, Takayuki; Yamaki, Sayaka; Yoshida, Atsushi (2017). "Study of the Reaction48Ca +248Cm →296Lv* at RIKEN-GARIS".Journal of the Physical Society of Japan.86 (3): 034201–1–7.Bibcode:2017JPSJ...86c4201K.doi:10.7566/JPSJ.86.034201.
  7. ^Hoffman, Darleane C.; Ghiorso, Albert; Seaborg, Glenn T. (2000).The Transuranium People: The Inside Story. World Scientific. p. 367.ISBN 978-1-78-326244-1.
  8. ^"List of experiments 2000–2006"Archived 2007-07-23 at theWayback Machine
  9. ^Biron, Lauren (23 July 2024)."A New Way to Make Element 116 Opens the Door to Heavier Atoms".lbl.gov. Lawrence Berkeley National Laboratory. Retrieved24 July 2024.
  10. ^Bourzac, Katherine (23 July 2024)."Heaviest element yet within reach after major breakthrough".Nature.doi:10.1038/d41586-024-02416-3. Retrieved24 July 2024.
  11. ^Service, Robert F. (23 July 2024)."U.S. back in race to forge unknown, superheavy elements".Science. Retrieved24 July 2024.
  12. ^Gates, P. M.; et al. (2024). "Toward the Discovery of New Elements: Production of Livermorium(Z = 116) with50Ti".Physical Review Letters.133 (172502).doi:10.1103/PhysRevLett.133.172502.
  13. ^Hulet, E. K.; Lougheed, R.; Wild, J.; Landrum, J.; Stevenson, P.; Ghiorso, A.; Nitschke, J.; Otto, R.; et al. (1977). "Search for Superheavy Elements in the Bombardment of248Cm with48Ca".Physical Review Letters.39 (7):385–389.Bibcode:1977PhRvL..39..385H.doi:10.1103/PhysRevLett.39.385.
  14. ^Armbruster, P.; Agarwal, YK; Brüchle, W; Brügger, M; Dufour, JP; Gaggeler, H; Hessberger, FP; Hofmann, S; et al. (1985)."Attempts to Produce Superheavy Elements by Fusion of48Ca with248Cm in the Bombarding Energy Range of 4.5–5.2 MeV/u".Physical Review Letters.54 (5):406–409.Bibcode:1985PhRvL..54..406A.doi:10.1103/PhysRevLett.54.406.PMID 10031507.
  15. ^abOganessian, Yu. Ts.; Utyonkov, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Shirokovsky, I.; Tsyganov, Yu.; Gulbekian, G.; Bogomolov, S.; Gikal, B.; Mezentsev, A.; Iliev, S.; Subbotin, V.; Sukhov, A.; Ivanov, O.; Buklanov, G.; Subotic, K.; Itkis, M.; Moody, K.; Wild, J.; Stoyer, N.; Stoyer, M.; Lougheed, R.; Laue, C.; Karelin, Ye.; Tatarinov, A. (2000). "Observation of the decay of292116".Physical Review C.63 (1): 011301.Bibcode:2000PhRvC..63a1301O.doi:10.1103/PhysRevC.63.011301.
  16. ^"Confirmed results of the248Cm(48Ca,4n)292116 experiment"Archived 2016-01-30 at theWayback Machine,Patin et al.,LLNL report (2003). Retrieved 2008-03-03
  17. ^Hofmann, Sigurd (2019). "Synthesis and properties of isotopes of the transactinides".Radiochimica Acta.107 (9–11):879–915.doi:10.1515/ract-2019-3104.S2CID 203848120.
  18. ^Hofmann, S.; Heinz, S.; Mann, R.; Maurer, J.; Münzenberg, G.; Antalic, S.; Barth, W.; Burkhard, H. G.; Dahl, L.; Eberhardt, K.; Grzywacz, R.; Hamilton, J. H.; Henderson, R. A.; Kenneally, J. M.; Kindler, B.; Kojouharov, I.; Lang, R.; Lommel, B.; Miernik, K.; Miller, D.; Moody, K. J.; Morita, K.; Nishio, K.; Popeko, A. G.; Roberto, J. B.; Runke, J.; Rykaczewski, K. P.; Saro, S.; Scheidenberger, C.; Schött, H. J.; Shaughnessy, D. A.; Stoyer, M. A.; Thörle-Popiesch, P.; Tinschert, K.; Trautmann, N.; Uusitalo, J.; Yeremin, A. V. (2016)."Review of even element super-heavy nuclei and search for element 120".The European Physical Journal A.2016 (52): 180.Bibcode:2016EPJA...52..180H.doi:10.1140/epja/i2016-16180-4.S2CID 124362890.
  19. ^abcdOganessian, Yu. Ts.; Utyonkov, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Shirokovsky, I.; Tsyganov, Yu.; Gulbekian, G.; Bogomolov, S.; Gikal, B.; Mezentsev, A.; Iliev, S.; Subbotin, V.; Sukhov, A.; Voinov, A.; Buklanov, G.; Subotic, K.; Zagrebaev, V.; Itkis, M.; Patin, J.; Moody, K.; Wild, J.; Stoyer, M.; Stoyer, N.; Shaughnessy, D.; Kenneally, J.; Wilk, P.; Lougheed, R.; Il’kaev, R.; Vesnovskii, S. (2004)."Measurements of cross sections and decay properties of the isotopes of elements 112, 114, and 116 produced in the fusion reactions233,238U,242Pu, and248Cm+48Ca"(PDF).Physical Review C.70 (6): 064609.Bibcode:2004PhRvC..70f4609O.doi:10.1103/PhysRevC.70.064609.
  20. ^Hofmann, S.; Heinz, S.; Mann, R.; Maurer, J.; Khuyagbaatar, J.; Ackermann, D.; Antalic, S.; Barth, W.; Block, M.; Burkhard, H. G.; Comas, V. F.; Dahl, L.; Eberhardt, K.; Gostic, J.; Henderson, R. A.; Heredia, J. A.; Heßberger, F. P.; Kenneally, J. M.; Kindler, B.; Kojouharov, I.; Kratz, J. V.; Lang, R.; Leino, M.; Lommel, B.; Moody, K. J.; Münzenberg, G.; Nelson, S. L.; Nishio, K.; Popeko, A. G.; et al. (2012). "The reaction 48Ca + 248Cm → 296116* studied at the GSI-SHIP".The European Physical Journal A.48 (5): 62.Bibcode:2012EPJA...48...62H.doi:10.1140/epja/i2012-12062-1.S2CID 121930293.
  21. ^Oganessian, Yu. Ts.; Utyonkov, V. (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.
  22. ^Hoffman, S.; et al. (2012)."The reaction48Ca +248Cm →296116* studied at the GSI-SHIP".European Physical Journal A.48 (62): 62.Bibcode:2012EPJA...48...62H.doi:10.1140/epja/i2012-12062-1.S2CID 121930293.
  23. ^abcdOganessian, Yu. Ts.; Utyonkov, V.; Lobanov, Yu.; Abdullin, F.; Polyakov, A.; Shirokovsky, I.; Tsyganov, Yu.; Gulbekian, G.; et al. (2004)."Measurements of cross sections for the fusion-evaporation reactions244Pu(48Ca,xn)292−x114 and245Cm(48Ca,xn)293−x116".Physical Review C.69 (5): 054607.Bibcode:2004PhRvC..69e4607O.doi:10.1103/PhysRevC.69.054607.
  24. ^abcOganessian, Yu. Ts.; Utyonkov, V. K.; Lobanov, Yu. V.; Abdullin, F. Sh.; Polyakov, A. N.; Sagaidak, R. N.; Shirokovsky, I. V.; Tsyganov, Yu. S.; et al. (2006-10-09)."Synthesis of the isotopes of elements 118 and 116 in the249Cf and245Cm+48Ca fusion reactions".Physical Review C.74 (4): 044602.Bibcode:2006PhRvC..74d4602O.doi:10.1103/PhysRevC.74.044602. Retrieved2008-01-18.
  25. ^seeFlerov lab annual reports 2000–2006
  26. ^Ninov, V.; et al. (1999)."Observation of Superheavy Nuclei Produced in the Reaction of86Kr with208Pb".Physical Review Letters.83 (6):1104–1107.Bibcode:1999PhRvL..83.1104N.doi:10.1103/PhysRevLett.83.1104.
  27. ^Ninov, V.; Gregorich, K.; Loveland, W.; Ghiorso, A.; Hoffman, D.; Lee, D.; Nitsche, H.; Swiatecki, W.; Kirbach, U.; Laue, C.; Adams, J.; Patin, J.; Shaughnessy, D.; Strellis, D.; Wilk, P. (2002)."Editorial Note: Observation of Superheavy Nuclei Produced in the Reaction of ^{86}Kr with ^{208}Pb [Phys. Rev. Lett. 83, 1104 (1999)]".Physical Review Letters.89 (3): 039901.Bibcode:2002PhRvL..89c9901N.doi:10.1103/PhysRevLett.89.039901.
  28. ^P. Roy Chowdhury; C. Samanta; D. N. Basu (2006). "α decay half-lives of new superheavy elements".Physical Review C.73 (1): 014612.arXiv:nucl-th/0507054.Bibcode:2006PhRvC..73a4612C.doi:10.1103/PhysRevC.73.014612.S2CID 118739116.
  29. ^C. Samanta; P. Roy Chowdhury; D. N. Basu (2007). "Predictions of alpha decay half lives of heavy and superheavy elements".Nuclear Physics A.789 (1–4):142–154.arXiv:nucl-th/0703086.Bibcode:2007NuPhA.789..142S.doi:10.1016/j.nuclphysa.2007.04.001.S2CID 7496348.
  30. ^abFeng, 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.S2CID 711489.
  31. ^abcdeFeng, 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.
  32. ^abZhu, 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
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