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Plutonium (Pu) has no stable isotopes. A standard atomic mass cannot be given.
Contents |
Decay modes
Twenty plutonium radioisotopes have been characterized. The most stable are Pu-244, with a half-life of 80.8 million years, Pu-242, with a half-life of 373,300 years, and Pu-239, with a half-life of 24,110 years. All of the remaining radioactive isotopes have half-lives that are less than 7,000 years. This element also has eight meta states, though none are very stable (all have half-lives less than one second).
The isotopes of plutonium range in atomic weight from 228.0387 u (Pu-228) to 247.074 u (Pu-247). The primary decay modes before the most stable isotope, Pu-244, are spontaneous fission and alpha emission; the primary mode after is beta emission. The primary decay products before Pu-244 are uranium and neptunium isotopes (neglecting the wide range of daughter nuclei created by fission processes), and the primary products after are americium isotopes.
Production and uses
Transmutation speed not shown and varies greatly by nuclide.
245Cm–248Cm are long-lived with negligible decay.
Pu-239, a fissile isotope which is the second most used nuclear fuel in nuclear reactors after U-235, and the most used fuel in the fission portion of nuclear weapons, is produced from U-238 by neutron capture followed by two beta decays.
Pu-240, Pu-241, Pu-242 are produced by further neutron capture. The odd-mass isotopes Pu-239 and Pu-241 have about a 3/4 chance of undergoing fission on capture of a thermal neutron and about a 1/4 chance of retaining the neutron and becoming the following isotope. The even-mass isotopes are fertile material but not fissile and also have a lower overall probability (cross section) of neutron capture; therefore, they tend to accumulate in nuclear fuel used in a thermal reactor, the design of all nuclear power plants today. In plutonium that has been used a second time in thermal reactors in MOX fuel, Pu-240 may even be the most common isotope. All plutonium isotopes and other actinides, however, are fissionable with fast neutrons. Pu-240 does have a moderate thermal neutron absorption cross section, so that Pu-241 production in a thermal reactor becomes a significant fraction as large as Pu-239 production.
Pu-241 has a halflife of 14 years, and has slightly higher thermal neutron cross sections than Pu-239 for both fission and absorption. While nuclear fuel is being used in a reactor, a Pu-241 nucleus is much more likely to fission or to capture a neutron than to decay. Pu-241 accounts for a significant proportion of fissions in thermal reactor fuel that has been used for some time. However, in spent nuclear fuel that does not quickly undergo nuclear reprocessing but instead is cooled for years after use, much or most of the Pu-241 will beta decay to americium-241, one of the minor actinides, a strong alpha emitter, and difficult to use in thermal reactors.
Pu-242 has a particularly low cross section for thermal neutron capture; and it takes four neutron absorptions to become another fissile isotope (either curium-245 or Pu-241) and fission. Even then, there is a chance either of those two fissile isotopes will fail to fission but instead absorb the fourth neutron, becoming curium-246 (on the way to even heavier actinides like californium, which is a neutron emitter by spontaneous fission and difficult to handle) or becoming Pu-242 again; so the mean number of neutrons absorbed before fission is even higher than 4. Therefore Pu-242 is particularly unsuited to recycling in a thermal reactor and would be better used in a fast reactor where it can be fissioned directly. However, Pu-242's low cross section means that relatively little of it will be transmuted during one cycle in a thermal reactor. Pu-242's halflife is about 15 times as long as Pu-239's halflife; therefore it is 1/15 as radioactive and not one of the larger contributors to nuclear waste radioactivity. 242Pu's gamma ray emissions are also weaker than those of the other isotopes.2
Pu-243 has a halflife of only 5 hours, beta decaying to americium-243. Because Pu-243 has little opportunity to capture an additional neutron before decay, the nuclear fuel cycle does not produce the extremely long-lived Pu-244 in significant quantity.
Pu-238 is not normally produced in as large quantity by the nuclear fuel cycle, but some is produced from neptunium-237 by neutron capture (this reaction can also be used with purified neptunium to produce Pu-238 relatively free of other plutonium isotopes for use in radioisotope thermoelectric generators), by the (n,2n) reaction of fast neutrons on Pu-239, or by alpha decay of curium-242 which is produced by neutron capture from Am-241. It has significant thermal neutron cross section for fission, but is more likely to capture a neutron and become Pu-239.
Manufacture
Pu-240, Pu-241 and Pu-242
The activation cross section for 239Pu is 270 barns, while the fission cross section is 747 barns for thermal neutrons. The higher plutonium isotopes are created when the uranium fuel is used for a long time. It is the case that for high burnup used fuel that the concentrations of the higher plutonium isotopes will be higher than the low burnup fuel which is reprocessed to obtain bomb grade plutonium.
| Isotope | Thermal neutron cross section |
decay mode | halflife | |
|---|---|---|---|---|
| Capture | Fission | |||
| 238U | 2.7 | α | 4.47 x 109 years | |
| 239U | β | 23 minutes | ||
| 239Np | β | 2.36 days | ||
| 239Pu | 270 | α | 24,110 years | |
| 240Pu | 289 | α | 6,564 years | |
| 241Pu | 362 | β | 14.35 years | |
| 242Pu | 18.8 | α | 373,300 years | |
Pu-239
Plutonium-239 is one of the three fissile materials used for the production of nuclear weapons and in some nuclear reactors as a source of energy. The other fissile materials are uranium-235 and uranium-233. Plutonium-239 is virtually nonexistent in nature. It is made by bombarding uranium-238 with neutrons in a nuclear reactor. Uranium-238 is present in quantity in most reactor fuel; hence plutonium-239 is continuously made in these reactors. Since plutonium-239 can itself be split by neutrons to release energy, plutonium-239 provides a portion of the energy generation in a nuclear reactor.
| Element | Isotope | Thermal neutron cross section |
decay mode | halflife |
|---|---|---|---|---|
| U | 238 | 2.7 | α | 4.47 x 109 years |
| U | 239 | - | β | 23 minutes |
| Np | 239 | - | β | 2.36 days |
| Pu | 239 | - | α | 24,110 years |
Pu-238
There are small amounts of Pu-238 in the plutonium of usual plutonium-producing reactors. However, isotopic separation would be quite expensive compared to another method: when a U-235 atom captures a neutron, it is converted to an excited state of U-236. Some of the excited U-236 nuclei undergo fission, but some decay to the ground state of U-236 by emitting gamma radiation. Further neutron capture creates U-237 which has a half-life of 7 days and thus quickly decays to Np-237. Since nearly all neptunium is produced in this way or consists of isotopes which decay quickly, one gets nearly pure Np-237 by chemical separation of neptunium. After this chemical separation, Np-237 is again irradiated by reactor neutrons to be converted to Np-238 which decays to Pu-238 with a half-life of 2 days.
| Element | Isotope | Thermal neutron cross section |
decay mode | halflife |
|---|---|---|---|---|
| U | 235 | 99 | α | 703,800,000 years |
| U | 236 | 5.3 | α | 23,420,000 years |
| U | 237 | - | β | 6.75 days |
| Np | 237 | 165 (capture) | α | 2,144,000 years |
| Np | 238 | - | β | 2.11 days |
| Pu | 238 | - | α | 87.7 years |
Pu-240 as obstacle to nuclear weapons
Pu-240 undergoes spontaneous fission as a secondary decay mode at a small but significant rate. The presence of Pu-240 limits the plutonium's nuclear bomb potential because the neutron flux from spontaneous fission, initiates the chain reaction prematurely and reduces the bomb's power by exploding the core before full implosion is reached. Plutonium consisting of more than about 90% Pu-239 is called weapons-grade plutonium; plutonium from spent nuclear fuel from commercial power reactors generally contains at least 20% Pu-240 and is called reactor-grade plutonium. However, modern nuclear weapons use fusion boosting which mitigates the predetonation problem; if the pit can generate a nuclear weapon yield of even a fraction of a kiloton, which is enough to start deuterium-tritium fusion, the resulting burst of neutrons will fission enough plutonium to ensure a yield of tens of kilotons.
Pu-240 contamination is the reason plutonium weapons must use the implosion method. Theoretically, pure Pu-239 could be used in a gun-type nuclear weapon, but achieving this level of purity is prohibitively difficult. Pu-240 contamination has proven a mixed blessing to nuclear weapons design. While it created delays and headaches during the Manhattan Project because of the need to develop implosion technology, those very same difficulties are currently a barrier to nuclear proliferation. Implosion devices are also inherently more efficient and less prone toward accidental detonation than are gun-type weapons.
Table
| nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | nuclear spin |
representative isotopic composition (mole fraction) |
range of natural variation (mole fraction) |
|---|---|---|---|---|---|---|---|
| excitation energy | |||||||
| 228Pu | 94 | 134 | 228.03874(3) | 1.1(+20-5) s | 0+ | ||
| 229Pu | 94 | 135 | 229.04015(6) | 120(50) s | 3/2+# | ||
| 230Pu | 94 | 136 | 230.039650(16) | 1.70(17) min | 0+ | ||
| 231Pu | 94 | 137 | 231.041101(28) | 8.6(5) min | 3/2+# | ||
| 232Pu | 94 | 138 | 232.041187(19) | 33.7(5) min | 0+ | ||
| 233Pu | 94 | 139 | 233.04300(5) | 20.9(4) min | 5/2+# | ||
| 234Pu | 94 | 140 | 234.043317(7) | 8.8(1) h | 0+ | ||
| 235Pu | 94 | 141 | 235.045286(22) | 25.3(5) min | (5/2+) | ||
| 236Pu | 94 | 142 | 236.0460580(24) | 2.858(8) a | 0+ | ||
| 237Pu | 94 | 143 | 237.0484097(24) | 45.2(1) d | 7/2- | ||
| 237m1Pu | 145.544(10) keV | 180(20) ms | 1/2+ | ||||
| 237m2Pu | 2900(250) keV | 1.1(1) µs | |||||
| 238Pu | 94 | 144 | 238.0495599(20) | 87.7(1) a | 0+ | ||
| 239Pu | 94 | 145 | 239.0521634(20) | 24.11(3)E+3 a | 1/2+ | ||
| 239m1Pu | 391.584(3) keV | 193(4) ns | 7/2- | ||||
| 239m2Pu | 3100(200) keV | 7.5(10) µs | (5/2+) | ||||
| 240Pu | 94 | 146 | 240.0538135(20) | 6561(7) a | 0+ | ||
| 241Pu | 94 | 147 | 241.0568515(20) | 14.290(6) a | 5/2+ | ||
| 241m1Pu | 161.6(1) keV | 0.88(5) µs | 1/2+ | ||||
| 241m2Pu | 2200(200) keV | 21(3) µs | |||||
| 242Pu | 94 | 148 | 242.0587426(20) | 3.75(2)E+5 a | 0+ | ||
| 243Pu | 94 | 149 | 243.062003(3) | 4.956(3) h | 7/2+ | ||
| 243mPu | 383.6(4) keV | 330(30) ns | (1/2+) | ||||
| 244Pu | 94 | 150 | 244.064204(5) | 8.00(9)E+7 a | 0+ | ||
| 245Pu | 94 | 151 | 245.067747(15) | 10.5(1) h | (9/2-) | ||
| 246Pu | 94 | 152 | 246.070205(16) | 10.84(2) d | 0+ | ||
| 247Pu | 94 | 153 | 247.07407(32)# | 2.27(23) d | 1/2+# | ||
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 Ame2003 Atomic Mass Evaluation by G. Audi, A.H. Wapstra, C. Thibault, J. Blachot and O. Bersillon in Nuclear Physics A729 (2003).
- Isotopic compositions and standard atomic masses from Atomic weights of the elements. Review 2000 (IUPAC Technical Report). Pure Appl. Chem. Vol. 75, No. 6, pp. 683-800, (2003) and Atomic Weights Revised (2005).
- Half-life, spin, and isomer data selected from these sources. Editing notes on this article's talk page.
- Audi, Bersillon, Blachot, Wapstra. The Nubase2003 evaluation of nuclear and decay properties, Nuc. Phys. A 729, pp. 3-128 (2003).
- National Nuclear Data Center, Brookhaven National Laboratory. Information extracted from the NuDat 2.1 database (retrieved Sept. 2005).
- David R. Lide (ed.), Norman E. Holden in CRC Handbook of Chemistry and Physics, 85th Edition, online version. CRC Press. Boca Raton, Florida (2005). Section 11, Table of the Isotopes.
- ^ "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. April 2004, http://www.jstage.jst.go.jp/article/jnst/41/4/448/_pdf.
- ^ "PLUTONIUM ISOTOPIC RESULTS OF KNOWN SAMPLES USING THE SNAP GAMMA SPECTROSCOPY ANALYSIS CODE AND THE ROBWIN SPECTRUM FITTING ROUTINE".
- ^ Miner 1968, p. 541
| Isotopes of neptunium | Isotopes of plutonium | Isotopes of americium |
| Index to isotope pages · Table of nuclides | ||
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