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词条 Isotopes of neptunium
释义

  1. Actinides vs fission products

  2. Notable isotopes

     Neptunium-235  Neptunium-236  Neptunium-237  Use in plutonium-238 production 

  3. List of isotopes

      Notes  

  4. References

{{infobox neptunium isotopes}}

Neptunium (93Np) is usually considered an artificial element, although trace quantities are found in nature, so a standard atomic weight cannot be given. Like all trace or artificial elements, it has no stable isotopes. The first isotope to be synthesized and identified was 239Np in 1940, produced by bombarding 238U with neutrons to produce 239U, which then underwent beta decay to 239Np.

Trace quantities are found in nature from neutron capture reactions by uranium atoms, a fact not discovered until 1951.

Twenty-three neptunium radioisotopes have been characterized, with the most stable being {{SimpleNuclide2|Neptunium|237}} with a half-life of 2.14 million years, {{SimpleNuclide2|Neptunium|236}} with a half-life of 154,000 years, and {{SimpleNuclide2|Neptunium|235}} with a half-life of 396.1 days. All of the remaining radioactive isotopes have half-lives that are less than 4.5 days, and the majority of these have half-lives that are less than 50 minutes. This element also has 4 meta states, with the most stable being {{SimpleNuclide2|Neptunium|236m}} (t1/2 22.5 hours).

The isotopes of neptunium range from {{SimpleNuclide2|Neptunium|219}} to {{SimpleNuclide2|Neptunium|244}}, though the intermediate isotopes {{SimpleNuclide2|Neptunium|220-222}} have not yet been observed. The primary decay mode before the most stable isotope, {{SimpleNuclide2|Neptunium|237}}, is electron capture (with a good deal of alpha emission), and the primary mode after is beta emission. The primary decay products before {{SimpleNuclide2|Neptunium|237}} are isotopes of uranium and protactinium, and the primary products after are isotopes of plutonium. Uranium-237 and neptunium-239 are regarded as the leading hazardous radioisotopes in the first hour-to-week period following nuclear fallout from a nuclear detonation, with Np-239 dominating "the spectrum for several days".[1][2]

Actinides vs fission products

{{Actinidesvsfissionproducts}}{{clear}}

Notable isotopes

Neptunium-235

Neptunium-235 has 142 neutrons and a half-life of 396.1 days. This isotope decays by:

  • Alpha emission: the decay energy is 5.2 MeV and the decay product is protactinium-231.
  • Electron capture: the decay energy is 0.125 MeV and the decay product is uranium-235

This isotope of neptunium has a weight of 235.044 063 3 u.

Neptunium-236

Neptunium-236 has 143 neutrons and a half-life of 154,000 years. It can decay by the following methods:

  • Electron capture: the decay energy is 0.93 MeV and the decay product is uranium-236. This usually decays (with a half-life of 23 million years) to thorium-232.
  • Beta emission: the decay energy is 0.48 MeV and the decay product is plutonium-236. This usually decays (half-life 2.8 years) to uranium-232, which usually decays (half-life 69 years) to thorium-228, which decays in a few years to lead-208.
  • Alpha emission: the decay energy is 5.007 MeV and the decay product is protactinium-232. This decays with a half-life of 1.3 days to uranium-232.

This particular isotope of neptunium has a mass of 236.04657 u. It is a fissile material with a critical mass of 6.79 kg.[3]

{{SimpleNuclide2|Neptunium|236}} is produced in small quantities via the (n,2n) and (γ,n) capture reactions of {{SimpleNuclide2|Neptunium|237}},[4] however, it is nearly impossible to separate in any significant quantities from its parent {{SimpleNuclide2|Neptunium|237}}.[5] It is for this reason that despite its low critical mass and high neutron cross section, it has not been researched as a nuclear fuel in weapons or reactors. Nevertheless, {{SimpleNuclide2|Neptunium|236}} has been considered for use in mass spectrometry and as a radioactive tracer, because it decays predominantly by beta emission with a long half-life.[6] Several alternative production routes for this isotope have been investigated, namely those that reduce isotopic separation from {{SimpleNuclide2|Neptunium|237}} or the isomer {{SimpleNuclide2|Neptunium|236m}}. The most favorable reactions to accumulate {{SimpleNuclide2|Neptunium|236}} were shown to be proton and deuteron irradiation of uranium-238.[6]

Neptunium-237

{{SimpleNuclide2|Neptunium|237}} decays via the neptunium series, which terminates with thallium-205, which is stable, unlike most other actinides, which decay to stable isotopes of lead.

In 2002, {{SimpleNuclide2|Neptunium|237}} was shown to be capable of sustaining a chain reaction with fast neutrons, as in a nuclear weapon, with a critical mass of around 60 kg.[7] However, it has a low probability of fission on bombardment with thermal neutrons, which makes it unsuitable as a fuel for conventional nuclear power plants (as opposed to accelerator-driven systems, etc.).

{{SimpleNuclide2|Neptunium|237}} is the only neptunium isotope produced in significant quantity in the nuclear fuel cycle, both by successive neutron capture by uranium-235 (which fissions most but not all of the time) and uranium-236, or (n,2n) reactions where a fast neutron occasionally knocks a neutron loose from uranium-238 or isotopes of plutonium. Over the long term, {{SimpleNuclide2|Neptunium|237}} also forms in spent nuclear fuel as the decay product of americium-241.{{SimpleNuclide2|Neptunium|237}} was projected to be one of the most mobile nuclides at the Yucca Mountain nuclear waste repository.

Use in plutonium-238 production

When exposed to neutron bombardment {{SimpleNuclide2|Neptunium|237}} can capture a neutron and become {{SimpleNuclide2|Plutonium|238|link=yes}}, this product being useful as an thermal energy source in a radio-isotope thermoelectric generator for the production of electricity and heat in deep space probes (such as the New Horizons and Voyager probes) and, of recent note, the Mars Science Laboratory (Curiosity rover). These applications are economically practical where photovoltaic power sources are weak or inconsistent due to probes being too far from the sun or rovers facing climate events that may obstruct sunlight for long periods. Space probes and rovers also make use of the heat output of the generator to keep their instruments and internals warm.[8]

List of isotopes

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)[9]
 
half-lifedecay
mode(s)[10][11]
daughter
isotope(s)
nuclear
spin and
parity
excitation energy
Neptunium|219}}[12]93126 219.03162(9) 0.15(+0.72-0.07) ms α 215Pa (9/2−)
Neptunium|223}}[13]93130 223.03285(21)# 2.15(+100-52) µs α 219Pa 9/2−
{{SimpleNuclide2|Neptunium|224}}[14]93131224.03422(21)#38(+26-11) µs α (83%) 220m1Pa1-#
α (17%) 220m2Pa
Neptunium|225}}93132 225.03391(8) 6(5) ms α 221Pa 9/2−#
Neptunium|226}}93133 226.03515(10)# 35(10) ms α 222Pa
{{SimpleNuclide2|Neptunium|227}}93134227.03496(8)510(60) ms α (99.95%) 223Pa5/2−#
β+ (.05%) 227U
{{SimpleNuclide2|Neptunium|228}}93135228.03618(21)#61.4(14) s β+ (59%) 228U
α (41%) 224Pa
β+, SF (.012%) (various)
{{SimpleNuclide2|Neptunium|229}}93136229.03626(9)4.0(2) min α (51%) 225Pa5/2+#
β+ (49%) 229U
{{SimpleNuclide2|Neptunium|230}}93137230.03783(6)4.6(3) min β+ (97%) 230U
α (3%) 226Pa
{{SimpleNuclide2|Neptunium|231}}93138231.03825(5)48.8(2) min β+ (98%) 231U(5/2)(+#)
α (2%) 227Pa
{{SimpleNuclide2|Neptunium|232}}93139232.04011(11)#14.7(3) min β+ (99.99%) 232U(4+)
α (.003%) 228Pa
{{SimpleNuclide2|Neptunium|233}}93140233.04074(5)36.2(1) min β+ (99.99%) 233U(5/2+)
α (.001%) 229Pa
Neptunium|234}}93141 234.042895(9) 4.4(1) d β+ 234U (0+)
{{SimpleNuclide2|Neptunium|235}}93142235.0440633(21)396.1(12) d EC 235U5/2+
α (.0026%) 231Pa
{{SimpleNuclide2|Neptunium|236}}[15]93143236.04657(5)1.54(6)×105 y EC (87.3%) 236U(6−)
β (12.5%) 236Pu
α (.16%) 232Pa
{{SimpleNuclide2|Neptunium|236m}}60(50) keV22.5(4) h EC (52%) 236U1
β (48%) 236Pu
{{SimpleNuclide2|Neptunium|237}}[15][16]93144237.0481734(20)2.144(7)×106 y α 233Pa5/2+
SF (2×10−10%) (various)
CD (4×10−12%) 207Tl
30Mg
Neptunium|238}}93145 238.0509464(20) 2.117(2) d β 238Pu 2+
{{SimpleNuclide2|Neptunium|238m}}2300(200)# keV 112(39) ns
Neptunium|239}}93146 239.0529390(22) 2.356(3) d β 239Pu 5/2+
Neptunium|240}}93147 240.056162(16) 61.9(2) min β 240Pu (5+)
{{SimpleNuclide2|Neptunium|240m}}20(15) keV7.22(2) min β (99.89%) 240Pu1(+)
IT (.11%) 240Np
Neptunium|241}}93148 241.05825(8) 13.9(2) min β 241Pu (5/2+)
Neptunium|242}}93149 242.06164(21) 2.2(2) min β 242Pu (1+)
{{SimpleNuclide2|Neptunium|242m}}0(50)# keV 5.5(1) min 6+#
Neptunium|243}}93150 243.06428(3)# 1.85(15) min β 243Pu (5/2−)
Neptunium|244}}93151 244.06785(32)# 2.29(16) min β 244Pu (7−)
1. ^[Film Badge Dosimetry in Atmospheric Nuclear Tests, By Committee on Film Badge Dosimetry in Atmospheric Nuclear Tests, Commission on Engineering and Technical Systems, Division on Engineering and Physical Sciences, National Research Council. pg24-35]
2. ^Bounding Analysis of Effects of Fractionation of Radionuclides in Fallout on Estimation of Doses to Atomic Veterans DTRA-TR-07-5. 2007
3. ^Final Report, Evaluation of nuclear criticality safety data and limits for actinides in transport {{webarchive|url=https://web.archive.org/web/20110519171204/http://ec.europa.eu/energy/nuclear/transport/doc/irsn_sect03_146.pdf |date=2011-05-19 }}, Republic of France, Institut de Radioprotection et de Sûreté Nucléaire, Département de Prévention et d'étude des Accidents.
4. ^Analysis of the Reuse of Uranium Recovered from the Reprocessing of Commercial LWR Spent Fuel, United States Department of Energy, Oak Ridge National Laboratory.
5. ^**{{cite book |author=Jukka Lehto |author2=Xiaolin Hou |year=2011|chapter=15.15: Neptunium |title=Chemistry and Analysis of Radionuclides |page=231 |nopp=yes |edition=1st |publisher=John Wiley & Sons |isbn=3527633022}}
6. ^{{cite journal|last=Jerome|first=S.M.|last2=Ivanov|first2=P.|last3=Larijani|first3=C. |last4=Parker|first4=D.J.|last5=Regan|first5=P.H.|title=The production of Neptunium-236g|date=2014|journal=Journal of Environmental Radioactivity|volume=138|pages=315–322|doi=10.1016/j.jenvrad.2014.02.029}}
7. ^{{cite journal |author=P. Weiss |date=26 October 2002 |title=Neptunium Nukes? Little-studied metal goes critical |url=http://www.sciencenews.org/view/generic/id/3246/title/Neptunium_Nukes%3F_Little-studied_metal_goes_critical |archiveurl=https://www.webcitation.org/6Cw9Vnt0Q?url=http://www.sciencenews.org/view/generic/id/3246/title/Neptunium_Nukes?_Little-studied_metal_goes_critical |archivedate=15 December 2012 |journal=Science News |volume=162 |issue=17 |page=259 |accessdate=7 November 2013 |deadurl=yes |df= }}
8. ^{{Cite journal|last=Witze|first=Alexandra|date=2014-11-27|title=Nuclear power: Desperately seeking plutonium|url=http://www.nature.com/news/nuclear-power-desperately-seeking-plutonium-1.16411|journal=Nature|language=en|volume=515|issue=7528|pages=484–486|doi=10.1038/515484a|bibcode=2014Natur.515..484W}}
9. ^{{NUBASE 2016 II}}
10. ^{{cite web |url=http://www.nucleonica.net/unc.aspx |title=Universal Nuclide Chart |publisher=nucleonica |registration=yes}}
11. ^Abbreviations:
CD: Cluster decay
EC: Electron capture
IT: Isomeric transition
SF: Spontaneous fission
12. ^Yang H, Ma L, Zhang Z, Yang C, Gan Z, Zhang M, et al. Alpha decay properties of the semi-magic nucleus 219 Np. Physics Letters B. 2018;777:212–6.
13. ^New short-lived isotope 223 Np and the absence of the Z = 92 subshell closure near N = 126M.d. Sun-Z. Liu-T.h. Huang-W.q. Zhang-J.g. Wang-X.y. Liu-B. Ding-Z.g. Gan-L. Ma-H.b. Yang-Z.y. Zhang-L. Yu-J. Jiang-K.l. Wang-Y.s. Wang-M.l. Liu-Z.h. Li-J. Li-X. Wang-H.y. Lu-C.j. Lin-L.j. Sun-N.r. Ma-C.x. Yuan-W. Zuo-H.s. Xu-X.h. Zhou-G.q. Xiao-C. Qi-F.s. Zhang - Physics Letters B - 2017
14. ^{{cite journal|last=Huang|first=T.H.|display-authors=etal|date=2018|title=Identification of the new isotope 224Np|url=https://www.researchgate.net/publication/328038265_Identification_of_the_new_isotope_Np_224|format=pdf|journal=Physical Review C|volume=98|issue=4|pages=044302|doi=10.1103/PhysRevC.98.044302}}
15. ^Fissile nuclide
16. ^Most common nuclide

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.

References

  • Isotope masses from:
    • {{NUBASE 2003}}
  • Isotopic compositions and standard atomic masses from:
    • {{CAWIA 2003}}
    • {{CIAAW 2005}}
  • Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
    • {{NUBASE 2003}}
    • {{NNDC}}
    • {{CRC85|chapter=11}}
{{Navbox element isotopes}}

3 : Neptunium|Isotopes of neptunium|Lists of isotopes by element

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