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Isotopes of americium

From Wikipedia, the free encyclopedia

Isotopes ofamericium (95Am)
Main isotopes[1]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
241Amsynth432.6 yα237Np
SF
242Amsynth16.02 hβ242Cm
ε242Pu
242m1Amsynth141 yIT242Am
α238Np
243Amsynth7350 yα239Np
SF

Americium (95Am) is anartificial element, and thus astandard atomic weight cannot be given. Like all artificial elements, it has no knownstable isotopes. The firstisotope to be synthesized was241Am in 1944. The artificial element decays by ejectingalpha particles. Americium has an atomic number of 95 (the number of protons in the nucleus of the americium atom). Despite243
Am
being an order of magnitude longer lived than241
Am
, the former is harder to obtain than the latter as more of it is present inspent nuclear fuel.

Eighteenradioisotopes of americium, ranging from229Am to247Am with the exception of231Am, have been characterized; another isotope,223Am, has also been reported but is unconfirmed. The most stable isotopes are243Am with ahalf-life of 7,350 years and241Am with a half-life of 432.6 years. All of the remainingradioactive isotopes have half-lives that are less than seven days, the majority of which are shorter than two hours. This element also has fourteenmeta states, with the most stable being242m1Am (half-life 141 years). This isomer is unusual in that its half-life is far longer than that of the ground state of the same isotope.

List of isotopes

[edit]

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

Spin and
parity[1]
[n 5][n 6]
Excitation energy[n 6]
223Am[n 7]95128223.04584(32)#10(9) msα219Np9/2–#
229Am95134229.04528(11)1.8(15) sα225Np5/2–#
230Am95135230.04603(15)#40(9) sβ+ (<70%)230Pu1–#
β+,SF (>30%)(various)
232Am95137232.04661(32)#1.31(4) minβ+ (97%)232Pu1–#
α? (3%)228Np
β+, SF (0.069%)(various)
233Am95138233.04647(12)#3.2(8) minβ+? (95.5%)233Pu5/2–#
α (4.5%)229Np
234Am95139234.04773(17)#2.32(8) minβ+ (99.95%)234Pu0–#
α (0.039%)230Np
β+, SF (0.0066%)(various)
235Am95140235.04791(6)10.3(6) minβ+ (99.60%)235Pu5/2−#
α (0.40%)231Np
236Am95141236.04943(13)#3.6(1) minβ+236Pu5−
α (4×10−3%)232Np
236mAm50(50)# keV2.9(2) minβ+236Pu(1−)
237Am95142237.05000(6)#73.6(8) minβ+ (99.975%)237Pu5/2−
α (0.025%)233Np
238Am95143238.05198(6)98(3) minβ+238Pu1+
α (1.0×10−4%)234Np
238mAm2500(200)# keV35(18) μsSF(various)
239Am95144239.0530227(21)11.9(1) hEC (99.990%)239Pu5/2−
α (0.010%)235Np
239mAm2500(200) keV163(12) nsSF(various)(7/2+)
240Am95145240.055298(15)50.8(3) hβ+240Pu(3−)
α (1.9×10−4%)236Np
240mAm3000(200) keV940(40) μsSF(various)
241Am95146241.0568273(12)432.6(6) yα237Np5/2−
SF (3.6×10−10%)(various)
241mAm2200(200) keV1.2(3) μsSF(various)
242Am95147242.0595474(12)16.02(2) hβ (82.7%)242Cm1−
EC (17.3%)242Pu
242m1Am48.60(5) keV141(2) yIT (99.55%)242Am5−
α (0.45%)238Np
SF (<4.7×10−9%)(various)
242m2Am2200(80) keV14.0(10) msSF(various)(2+, 3−)
IT242Am
243Am95148243.0613799(15)7350(9) yα239Np5/2−
SF (3.7×10−9%)(various)
243mAm2300(200) keV5.5(5) μsSF(various)
244Am95149244.0642829(16)10.01(3) hβ244Cm(6−)
244m1Am89.3(16) keV26.13(43) minβ (99.96%)244Cm1+
EC (0.0364%)244Pu
244m2Am2000(200)# keV0.90(15) msSF(various)
244m3Am2200(200)# keV~6.5 μsSF(various)
245Am95150245.0664528(20)2.05(1) hβ245Cm5/2+
245mAm2400(400)# keV0.64(6) μsSF(various)
246Am95151246.069774(19)#39(3) minβ246Cm7−
246m1Am30(10)# keV25.0(2) minβ246Cm2(−)
246m2Am2000(800)# keV73(10) μsSF(various)
247Am95152247.07209(11)#23.0(13) minβ247Cm5/2#
This table header & footer:
  1. ^mAm – 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. ^Modes of decay:
    EC:Electron capture
    CD:Cluster decay
    IT:Isomeric transition
    SF:Spontaneous fission
  5. ^( ) spin value – Indicates spin with weak assignment arguments.
  6. ^ab# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  7. ^The discovery of this isotope is uncertain due to disagreements between theoretical predictions and reported experimental data.[3]

Actinides vs fission products

[edit]
Actinides and fission products by half-life
Actinides[4] bydecay chainHalf-life
range (a)
Fission products of235U byyield[5]
4n
(Thorium)
4n + 1
(Neptunium)
4n + 2
(Radium)
4n + 3
(Actinium)
4.5–7%0.04–1.25%<0.001%
228Ra4–6 a155Euþ
248Bk[6]> 9 a
244Cmƒ241Puƒ250Cf227Ac10–29 a90Sr85Kr113mCdþ
232Uƒ238Puƒ243Cmƒ29–97 a137Cs151Smþ121mSn
249Cfƒ242mAmƒ141–351 a

No fission products have ahalf-life
in the range of 100 a–210 ka ...

241Amƒ251Cfƒ[7]430–900 a
226Ra247Bk1.3–1.6 ka
240Pu229Th246Cmƒ243Amƒ4.7–7.4 ka
245Cmƒ250Cm8.3–8.5 ka
239Puƒ24.1 ka
230Th231Pa32–76 ka
236Npƒ233Uƒ234U150–250 ka99Tc126Sn
248Cm242Pu327–375 ka79Se
1.33 Ma135Cs
237Npƒ1.61–6.5 Ma93Zr107Pd
236U247Cmƒ15–24 Ma129I
244Pu80 Ma

... nor beyond 15.7 Ma[8]

232Th238U235Uƒ№0.7–14.1 Ga

Americium-241

[edit]
Americium-241, as used in ionizationsmoke detectors.
Main article:Americium-241

Americium-241 (alpha emitter, half-life 432.6 years) is the most common isotope of americium in nuclear waste.[9] It is the isotope used in normalionization smoke detectors, which work as anionization chamber. It is a potential fuel for long-lifetimeradioisotope thermoelectric generators, with a half-life longer than that of the standardplutonium-238 (87.7 years) or the alternativestrontium-90 (28.91 years). Itsdecay heat is 0.114 W/g; its rate ofspontaneous fission 1.2/g/s.

The alpha decay of241Am is accompanied by a significant emission ofgamma rays. Its presence in plutonium is determined by the original concentration of241Pu (which decays to it) and the sample age. Older samples of plutonium containing plutonium-241 build up241Am, and chemical separation of americium from such plutonium (e.g. during reworking ofplutonium pits) may be required.

Americium-242m

[edit]
Transmutation flow between238Pu and244Cm in LWR.[10]
Fission percentage is 100 minus shown percentages.
Total rate of transmutation varies greatly by nuclide.
245Cm–248Cm are long-lived with negligible decay.

Americium-242m (half-life 141 years) is one of the rare cases, like108mAg,166mHo,180mTa,186mRe,192mIr,210mBi,212mPo and others, where a higher-energynuclear isomer is more stable than its ground state. While that ground state,242Am, decays with half-life 16.02 hours bybeta emission orelectron capture, in a typical example of spin-forbiddenness the isomer does not decay by those modes, but falls to the ground state very slowly (99.55% of decays) or emits analpha particle (0.45%, partial half-life 31 ky).

242mAm isfissile with a lowcritical mass, comparable to that of239Pu.[11] It has a very high fissioncross section, and is quickly destroyed if it is produced in a nuclear reactor. It has been investigated whether this isotope could be used for a novel type ofnuclear rocket.[12][13]

Americium-243

[edit]
A sample of Am-243

Americium-243, an alpha emitter, has ahalf-life of 7350 years[1], the longest of all americium isotopes. It is formed in thenuclear fuel cycle mainly byneutron capture onplutonium-242 followed bybeta decay.[14] Production increases exponentially with increasingburnup as a total of 5 neutron captures on238U are required. IfMOX-fuel is used, particularly MOX-fuel high in241
Pu
and242
Pu
, more americium overall and more243
Am
will be produced.

It decays by either emitting analpha particle (decay energy 5.439 MeV)[15] to become239Np, which then quickly goes to239Pu, or, very rarely,spontaneous fission. The fission rate is about 60% that of americium-241 or about 0.7/g/s.[16]

As for the other americium isotopes, and more generally for all alpha emitters,243Am iscarcinogenic in case of internal contamination after being inhaled or ingested.243Am also presents a risk of external irradiation associated with the gamma ray emitted by its short-lived decay product239Np. The external irradiation risk for the other two americium isotopes (241Am and242mAm) is less than 10% of that for americium-243.[9]

References

[edit]
  1. ^abcdeKondev, 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. ^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.
  3. ^Sun, M. D.; et al. (2017)."New short-lived isotope223Np and the absence of the Z = 92 subshell closure near N = 126".Physics Letters B.771:303–308.Bibcode:2017PhLB..771..303S.doi:10.1016/j.physletb.2017.03.074.
  4. ^Plus radium (element 88). While actually a sub-actinide, it immediately precedes actinium (89) and follows a three-element gap of instability afterpolonium (84) where no nuclides have half-lives of at least four years (the longest-lived nuclide in the gap isradon-222 with a half life of less than fourdays). Radium's longest lived isotope, at 1,600 years, thus merits the element's inclusion here.
  5. ^Specifically fromthermal neutron fission of uranium-235, e.g. in a typicalnuclear reactor.
  6. ^Milsted, J.; Friedman, A. M.; Stevens, C. M. (1965). "The alpha half-life of berkelium-247; a new long-lived isomer of berkelium-248".Nuclear Physics.71 (2): 299.Bibcode:1965NucPh..71..299M.doi:10.1016/0029-5582(65)90719-4.
    "The isotopic analyses disclosed a species of mass 248 in constant abundance in three samples analysed over a period of about 10 months. This was ascribed to an isomer of Bk248 with a half-life greater than 9 [years]. No growth of Cf248 was detected, and a lower limit for the β half-life can be set at about 104 [years]. No alpha activity attributable to the new isomer has been detected; the alpha half-life is probably greater than 300 [years]."
  7. ^This is the heaviest nuclide with a half-life of at least four years before the "sea of instability".
  8. ^Excluding those "classically stable" nuclides with half-lives significantly in excess of232Th; e.g., while113mCd has a half-life of only fourteen years, that of113Cd is eightquadrillion years.
  9. ^ab"Americium"Archived 2012-07-30 at theWayback Machine. Argonne National Laboratory, EVS. Retrieved 25 December 2009.
  10. ^Sasahara, Akihiro; Matsumura, Tetsuo; Nicolaou, Giorgos; Papaioannou, Dimitri (April 2004)."Neutron and Gamma Ray Source Evaluation of LWR High Burn-up UO2 and MOX Spent Fuels".Journal of Nuclear Science and Technology.41 (4):448–456.doi:10.3327/jnst.41.448.
  11. ^"Critical Mass Calculations for241Am,242mAm and243Am"(PDF). Archived fromthe original(PDF) on July 22, 2011. RetrievedFebruary 3, 2011.
  12. ^"Extremely Efficient Nuclear Fuel Could Take Man To Mars In Just Two Weeks" (Press release). Ben-Gurion University Of The Negev. December 28, 2000.
  13. ^Ronen, Yigal; Shwageraus, E. (2000). "Ultra-thin 242mAm fuel elements in nuclear reactors".Nuclear Instruments and Methods in Physics Research A.455 (2):442–451.Bibcode:2000NIMPA.455..442R.doi:10.1016/s0168-9002(00)00506-4.
  14. ^"Americium-243"Archived 2011-02-25 at theWayback Machine. Oak Ridge National Laboratory. Retrieved 25 December 2009.
  15. ^National Nuclear Data Center."NuDat 3.0 database".Brookhaven National Laboratory.
  16. ^Calculated from Nubase data.

Sources

[edit]
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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