Decay chain explained

In nuclear science, the decay chain refers to a series of radioactive decays of different radioactive decay products as a sequential series of transformations. It is also known as a "radioactive cascade". The typical radioisotope does not decay directly to a stable state, but rather it decays to another radioisotope. Thus there is usually a series of decays until the atom has become a stable isotope, meaning that the nucleus of the atom has reached a stable state.

Decay stages are referred to by their relationship to previous or subsequent stages. A parent isotope is one that undergoes decay to form a daughter isotope. One example of this is uranium (atomic number 92) decaying into thorium (atomic number 90). The daughter isotope may be stable or it may decay to form a daughter isotope of its own. The daughter of a daughter isotope is sometimes called a granddaughter isotope. Note that the parent isotope becomes the daughter isotope, unlike in the case of a biological parent and daughter.

The time it takes for a parent atom to decay to its daughter nuclei can vary widely, based on the material's half-life. For individual nuclei, the process behaves as a random Poisson process, as the decay of each single atom occurs spontaneously.

The decay of an initial population of identical atoms over time t follows a decaying exponential distribution e−λt, where λ is the decay constant. An important property of a radioactive material is its half-life, the time by which half of an initial number of identical parent radioisotopes can be expected statistically to have decayed to their daughters, which is inversely related to λ. Half-lives have been determined in laboratories for many radionuclides, and can range from nearly instantaneous (less than 10−21 seconds) to more than 1019 years.

At equilibrium, each intermediate stage of the decay chain emit the same amount of radioactivity as the original radioisotope (i.e., a one-to-one relationship between the numbers of decays in each successive stage). However each stage can release a different quantity of energy, as the decay energy is specific to each radionuclide. If and when equilibrium is achieved, each successive daughter isotope is present in direct proportion to its half-life; but since its activity is inversely proportional to its half-life, each nuclide in the decay chain contributes as many individual transformations as the head of the chain. For example, uranium-238 is weakly radioactive, but pitchblende, a uranium ore, is 13 times more radioactive than the pure uranium metal because of the presence of shorter-lived decay products, such as radium and the noble gas radon. Rock containing thorium and/or uranium (such as some types of granite) emits radon gas, which tends to accumulate in enclosed places such as basements or underground mines due to its high density.[1]

The quantity of isotopes in the decay chains at a certain time is described by the Bateman equation. Due to its peculiarities, isotopically enriched materials out of equilibrium with its natural decay products can occasionally increase in radioactivity for an amount of time, contrary to common intuition about radioactive decay.[2] Depleted uranium is an example of such material.

History

With the exceptions of hydrogen-1, hydrogen-2 (deuterium), helium-3, helium-4, and perhaps trace amounts of stable lithium and beryllium isotopes which were created in the Big Bang, all the elements and isotopes found on Earth were created by the s-process or the r-process in stars or stellar collisions, and for those to be today a part of the Earth, must have been created not later than 4.5 billion years ago. All the elements created 4.5 billion years ago or earlier are termed primordial, meaning they were generated by the universe's stellar processes. At the time when they were created, those that were unstable began decaying immediately. All the isotopes which have half-lives less than 100 million years have been reduced to or less of whatever original amounts were created and captured by Earth's accretion; they are of trace quantity today, or have decayed away altogether. There are only two other methods to create isotopes: artificially, inside a man-made (or perhaps a natural) reactor, or through decay of a parent isotopic species, the process known as the decay chain.

Unstable isotopes decay to their daughter products (which may sometimes be even more unstable) at a given rate; eventually, often after a series of decays, a stable isotope is reached: there are 251 stable isotopes in the universe. In stable isotopes, light elements typically have a lower ratio of neutrons to protons in their nucleus than heavier elements. Light elements such as helium-4 have close to a 1:1 neutron:proton ratio. The heaviest elements such as lead have close to 1.5 neutrons per proton (e.g. 1.536 in lead-208). No nuclide heavier than lead-208 is stable; these heavier elements have to shed mass to achieve stability, mostly by alpha decay. The other common way for isotopes with a high neutron to proton ratio (n/p) to decay is beta decay, in which the nuclide changes elemental identity while keeping the same mass number and lowering its n/p ratio. For some isotopes with a relatively low n/p ratio, there is an inverse beta decay, by which a proton is transformed into a neutron, thus moving towards a stable isotope; however, since fission almost always produces products which are neutron heavy, positron emission or electron capture are rare compared to electron emission. There are many relatively short beta decay chains, at least two (a heavy, beta decay and a light, positron decay) for every discrete weight up to around 207 and some beyond, but for the higher mass elements (isotopes heavier than lead) there are only four pathways which encompass all decay chains. This is because there are just two main decay methods: alpha radiation, which reduces the mass by 4 atomic mass units (amu), and beta, which does not change the mass number (just the atomic number and the p/n ratio). The four paths are termed 4n, 4n + 1, 4n + 2, and 4n + 3; the remainder from dividing the atomic mass by four gives the chain the isotope will use to decay. There are other decay modes, but they invariably occur at a lower probability than alpha or beta decay. (It should not be supposed that these chains have no branches: the diagram below shows a few branches of chains, and in reality there are many more, because there are many more isotopes possible than are shown in the diagram.) For example, the third atom of nihonium-278 synthesised underwent six alpha decays down to mendelevium-254, followed by an electron capture (a form of beta decay) to fermium-254, and then a seventh alpha to californium-250,[3] upon which it would have followed the 4n + 2 chain as given in this article. However, the heaviest superheavy nuclides synthesised do not reach the four decay chains, because they reach a spontaneously fissioning nuclide after a few alpha decays that terminates the chain: this is what happened to the first two atoms of nihonium-278 synthesised,[4] [5] as well as to all heavier nuclides produced.

Three of those chains have a long-lived isotope (or nuclide) near the top; this long-lived nuclide is a bottleneck in the process through which the chain flows very slowly, and keeps the chain below them "alive" with flow. The three long-lived nuclides are uranium-238 (half-life 4.5 billion years), uranium-235 (half-life 700 million years) and thorium-232 (half-life 14 billion years). The fourth chain has no such long-lasting bottleneck nuclide near the top, so almost all of the nuclides in that chain have long since decayed down to just before the end: bismuth-209. This nuclide was long thought to be stable, but in 2003 it was found to be unstable, with a very long half-life of 20.1 billion billion years;[6] it is the last step in the chain before stable thallium-205. Because this bottleneck is so long-lived, very small quantities of the final decay product have been produced, and for most practical purposes bismuth-209 is the final decay product.

In the distant past, during the first few million years of the history of the Solar System, there were more kinds of unstable high-mass nuclides in existence, and the four chains were longer, as they included nuclides that have since decayed away. Notably, 244Pu, 237Np, and 247Cm have half-lives over a million years and would have then been lesser bottlenecks high in the 4n, 4n+1, and 4n+3 chains respectively.[7] (There is no nuclide with a half-life over a million years above 238U in the 4n+2 chain.) Today some of these formerly extinct isotopes are again in existence as they have been manufactured. Thus they again take their places in the chain: plutonium-239, used in nuclear weapons, is the major example, decaying to uranium-235 via alpha emission with a half-life 24,500 years. There has also been large-scale production of neptunium-237, which has resurrected the hitherto extinct fourth chain.[8] The tables below hence start the four decay chains at isotopes of californium with mass numbers from 249 to 252.

Name of series
ThoriumNeptuniumUraniumActinium
Mass numbers4n4n+14n+24n+3
Long-lived nuclide232Th
(244Pu)
209Bi
(237Np)
238U
 
235U
(247Cm)
Half-life
(billions of years)
14
(0.08)

(0.00214)
4.5
 
0.7
(0.0156)
End of chain208Pb205Tl206Pb207Pb

These four chains are summarised in the chart in the following section.

Types of decay

The four most common modes of radioactive decay are: alpha decay, beta decay, inverse beta decay (considered as both positron emission and electron capture), and isomeric transition. Of these decay processes, only alpha decay (fission of a helium-4 nucleus) changes the atomic mass number (A) of the nucleus, and always decreases it by four. Because of this, almost any decay will result in a nucleus whose atomic mass number has the same residue mod 4. This divides the list of nuclides into four classes. All the members of any possible decay chain must be drawn entirely from one of these classes.

Three main decay chains (or families) are observed in nature. These are commonly called the thorium series, the radium or uranium series, and the actinium series, representing three of these four classes, and ending in three different, stable isotopes of lead. The mass number of every isotope in these chains can be represented as A = 4n, A = 4n + 2, and A = 4n + 3, respectively. The long-lived starting isotopes of these three isotopes, respectively thorium-232, uranium-238, and uranium-235, have existed since the formation of the Earth, ignoring the artificial isotopes and their decays created since the 1940s.

Due to the relatively short half-life of its starting isotope neptunium-237 (2.14 million years), the fourth chain, the neptunium series with A = 4n + 1, is already extinct in nature, except for the final rate-limiting step, decay of bismuth-209. Traces of 237Np and its decay products do occur in nature, however, as a result of neutron capture in uranium ore. The ending isotope of this chain is now known to be thallium-205. Some older sources give the final isotope as bismuth-209, but in 2003 it was discovered that it is very slightly radioactive, with a half-life of .

There are also non-transuranic decay chains of unstable isotopes of light elements, for example those of magnesium-28 and chlorine-39. On Earth, most of the starting isotopes of these chains before 1945 were generated by cosmic radiation. Since 1945, the testing and use of nuclear weapons has also released numerous radioactive fission products. Almost all such isotopes decay by either β or β+ decay modes, changing from one element to another without changing atomic mass. These later daughter products, being closer to stability, generally have longer half-lives until they finally decay into stability.

Actinide alpha decay chains

In the four tables below, the minor branches of decay (with the branching probability of less than 0.0001%) are omitted. The energy release includes the total kinetic energy of all the emitted particles (electrons, alpha particles, gamma quanta, neutrinos, Auger electrons and X-rays) and the recoil nucleus, assuming that the original nucleus was at rest. The letter 'a' represents a year (from the Latin annus).

In the tables below (except neptunium), the historic names of the naturally occurring nuclides are also given. These names were used at the time when the decay chains were first discovered and investigated. From these historical names one can locate the particular chain to which the nuclide belongs, and replace it with its modern name.

The three naturally-occurring actinide alpha decay chains given below—thorium, uranium/radium (from uranium-238), and actinium (from uranium-235)—each ends with its own specific lead isotope (lead-208, lead-206, and lead-207 respectively). All these isotopes are stable and are also present in nature as primordial nuclides, but their excess amounts in comparison with lead-204 (which has only a primordial origin) can be used in the technique of uranium–lead dating to date rocks.

Thorium series

The 4n chain of thorium-232 is commonly called the "thorium series" or "thorium cascade". Beginning with naturally occurring thorium-232, this series includes the following elements: actinium, bismuth, lead, polonium, radium, radon and thallium. All are present, at least transiently, in any natural thorium-containing sample, whether metal, compound, or mineral. The series terminates with lead-208.

Plutonium-244 (which appears several steps above thorium-232 in this chain if one extends it to the transuranics) was present in the early Solar System,[7] and is just long-lived enough that it should still survive in trace quantities today,[9] though it is uncertain if it has been detected.[10]

The total energy released from thorium-232 to lead-208, including the energy lost to neutrinos, is 42.6 MeV.

NuclideHistoric namesDecay modeHalf-life
(a = years)
Energy released
MeV
Decay
product
ShortLong
252Cfα2.645 a6.1181248Cm
248Cmα3.4 a5.162244Pu
244Puα8 a4.589240U
240Uβ14.1 h0.39240Np
240Npβ1.032 h2.2240Pu
240Puα6561 a5.1683236U
236UThoruranium[11] α2.3 a4.494232Th
232ThThThoriumα1.405 a4.081228Ra
228RaMsTh1Mesothorium 1β5.75 a0.046228Ac
228AcMsTh2Mesothorium 2β6.25 h2.124228Th
228ThRdThRadiothoriumα1.9116 a5.520224Ra
224RaThXThorium Xα3.6319 d5.789220Rn
220RnTnThoron,
Thorium Emanation
α55.6 s6.404216Po
216PoThAThorium Aα0.145 s6.906212Pb
212PbThBThorium Bβ10.64 h0.570212Bi
212BiThCThorium Cβ 64.06%
α 35.94%
60.55 min2.252
6.208
212Po
208Tl
212PoThC′Thorium C′α294.4 ns8.954[12] 208Pb
208TlThC″Thorium C″β3.053 min1.803[13] 208Pb
208PbThDThorium Dstable

Neptunium series

The 4n + 1 chain of neptunium-237 is commonly called the "neptunium series" or "neptunium cascade". In this series, only two of the isotopes involved are found naturally in significant quantities, namely the final two: bismuth-209 and thallium-205. Some of the other isotopes have been detected in nature, originating from trace quantities of 237Np produced by the (n,2n) knockout reaction in primordial 238U.[14] A smoke detector containing an americium-241 ionization chamber accumulates a significant amount of neptunium-237 as its americium decays. The following elements are also present in it, at least transiently, as decay products of the neptunium: actinium, astatine, bismuth, francium, lead, polonium, protactinium, radium, radon, thallium, thorium, and uranium. Since this series was only discovered and studied in 1947–1948, its nuclides do not have historic names. One unique trait of this decay chain is that the noble gas radon is only produced in a rare branch (not shown in the illustration) but not the main decay sequence; thus, radon from this decay chain does not migrate through rock nearly as much as from the other three. Another unique trait of this decay sequence is that it ends in thallium rather than lead. This series terminates with the stable isotope thallium-205.

The total energy released from californium-249 to thallium-205, including the energy lost to neutrinos, is 66.8 MeV.

NuclideDecay modeHalf-life
(a = years)
Energy released
MeV
Decay product
249Cfα351 a5.813+.388245Cm
245Cmα8500 a5.362+.175241Pu
241Puβ14.4 a0.021241Am
241Amα432.7 a5.638237Np
237Npα2.14×106 a4.959233Pa
233Paβ27.0 d0.571233U
233Uα1.592×105 a4.909229Th
229Thα7340 a5.168225Ra
225Raβ 99.998%
α 0.002%
14.9 d0.36
5.097
225Ac
221Rn
225Acα10.0 d5.935221Fr
221Rnβ 78%
α 22%
25.7 min1.194
6.163
221Fr
217Po
221Frα 99.9952%
β 0.0048%
4.8 min6.458
0.314
217At
221Ra
221Raα28 s6.880217Rn
217Poα 97.5%
β 2.5%
1.53 s6.662
1.488
213Pb
217At
217Atα 99.992%
β 0.008%
32 ms7.201
0.737
213Bi
217Rn
217Rnα540 μs7.887213Po
213Pbβ10.2 min2.028213Bi
213Biβ 97.80%
α 2.20%
46.5 min1.423
5.87
213Po
209Tl
213Poα3.72 μs8.536209Pb
209Tlβ2.2 min3.99209Pb
209Pbβ3.25 h0.644209Bi
209Biα2.01×1019 a3.137205Tl
205Tl.stable..

Uranium series

The 4n+2 chain of uranium-238 is called the "uranium series" or "radium series". Beginning with naturally occurring uranium-238, this series includes the following elements: astatine, bismuth, lead, mercury, polonium, protactinium, radium, radon, thallium, and thorium. All are present, at least transiently, in any natural uranium-containing sample, whether metal, compound, or mineral. The series terminates with lead-206.

The total energy released from uranium-238 to lead-206, including the energy lost to neutrinos, is 51.7 MeV.

Parent
nuclide
Historic nameDecay mode [15] Half-life
(a= years)
Energy released
MeV
Decay
product
ShortLong
250Cfα13.08 a6.12844246Cm
246Cmα4800 a5.47513242Pu
242Puα3.8×105 a4.98453238U
238UUIUranium Iα4.468×109 a4.26975234Th
234ThUX1Uranium X1β24.10 d0.273088234mPa
234mPaUX2, BvUranium X2
Brevium
IT, 0.16%
β, 99.84%
1.159 min0.07392
2.268205
234Pa
234U
234PaUZUranium Zβ6.70 h2.194285234U
234UUIIUranium IIα2.45×105 a4.8698230Th
230ThIoIoniumα7.54×104 a4.76975226Ra
226RaRaRadiumα1600 a4.87062222Rn
222RnRnRadon,
Radium Emanation
α3.8235 d5.59031218Po
218PoRaARadium Aα, 99.980%
β, 0.020%
3.098 min6.11468
0.259913
214Pb
218At
218Atα, 99.9%
β, 0.1%
1.5 s6.874
2.881314
214Bi
218Rn
218Rnα35 ms7.26254214Po
214PbRaBRadium Bβ26.8 min1.019237214Bi
214BiRaC Radium Cβ, 99.979%
α, 0.021%
19.9 min3.269857
5.62119
214Po
210Tl
214PoRaC'Radium C'α164.3 μs7.83346210Pb
210TlRaC"Radium C"β1.3 min5.48213210Pb
210PbRaDRadium Dβ, 100%
α, 1.9×10−6%
22.20 a0.063487
3.7923
210Bi
206Hg
210BiRaERadium E β, 100%
α, 1.32×10−4%
5.012 d1.161234
5.03647
210Po
206Tl
210PoRaFRadium Fα138.376 d5.03647206Pb
206Hgβ8.32 min1.307649206Tl
206Tlβ4.202 min1.5322211206Pb
206PbRaG[16] Radium Gstable---

Actinium series

The 4n+3 chain of uranium-235 is commonly called the "actinium series" or "actinium cascade". Beginning with the naturally-occurring isotope uranium-235, this decay series includes the following elements: actinium, astatine, bismuth, francium, lead, polonium, protactinium, radium, radon, thallium, and thorium. All are present, at least transiently, in any sample containing uranium-235, whether metal, compound, ore, or mineral. This series terminates with the stable isotope lead-207.

In the early Solar System this chain went back to 247Cm. This manifests itself today as variations in 235U/238U ratios, since curium and uranium have noticeably different chemistries and would have separated differently.[7] [17]

The total energy released from uranium-235 to lead-207, including the energy lost to neutrinos, is 46.4 MeV.

NuclideHistoric nameDecay modeHalf-life
(a = years)
Energy released
MeV
Decay
product
ShortLong
251Cfα900.6 a6.176247Cm
247Cmα1.56×107 a5.353243Pu
243Puβ-4.95556 h0.579243Am
243Amα7388 a5.439239Np
239Npβ-2.3565 d0.723239Pu
239Puα2.41×104 a5.244235U
235UAcUActin Uraniumα7.04×108 a4.678231Th
231ThUYUranium Yβ25.52 h0.391231Pa
231PaPaProtactiniumα32760 a5.150227Ac
227AcAcActiniumβ 98.62%
α 1.38%
21.772 a0.045
5.042
227Th
223Fr
227ThRdAcRadioactiniumα18.68 d6.147223Ra
223FrAcKActinium Kβ 99.994%
α 0.006%
22.00 min1.149
5.340
223Ra
219At
223RaAcXActinium Xα11.43 d5.979219Rn
219Atα 97.00%
β 3.00%
56 s6.275
1.700
215Bi
219Rn
219RnAnActinon,
Actinium Emanation
α3.96 s6.946215Po
215Biβ7.6 min2.250 215Po
215PoAcAActinium Aα 99.99977%
β 0.00023%
1.781 ms7.527
0.715
211Pb
215At
215Atα0.1 ms8.178211Bi
211PbAcBActinium Bβ36.1 min1.367211Bi
211BiAcCActinium Cα 99.724%
β 0.276%
2.14 min6.751
0.575
207Tl
211Po
211PoAcC'Actinium C'α516 ms7.595207Pb
207TlAcC"Actinium C"β4.77 min1.418207Pb
207PbAcDActinium D.stable..

See also

References

External links

Notes and References

  1. Web site: Radon | Indoor Air Quality | Air | US EPA . 2008-06-26 . live . https://web.archive.org/web/20080920014042/http://www.epa.gov/radon/ . 2008-09-20 .
  2. Web site: Uranium Radiation Properties . WISE Uranium Project . 2024-01-26 . 2024-06-20.
  3. Journal of the Physical Society of Japan. 81. 103201 . 2012. New Results in the Production and Decay of an Isotope, 278113, of the 113th Element. K. Morita. 10.1143/JPSJ.81.103201. Morimoto. Kouji. Kaji. Daiya. Haba. Hiromitsu. Ozeki. Kazutaka. Kudou. Yuki. Sumita. Takayuki. Wakabayashi. Yasuo. Yoneda. Akira. Kengo . Tanaka. Sayaka . Yamaki. Ryutaro . Sakai. Takahiro . Akiyama. Shin-ichi . Goto. Hiroo . Hasebe. Minghui . Huang. Tianheng . Huang. Eiji . Ideguchi. Yoshitaka . Kasamatsu. Kenji . Katori. Yoshiki . Kariya. Hidetoshi . Kikunaga. Hiroyuki . Koura. Hisaaki . Kudo. Akihiro . Mashiko. Keita . Mayama. Shin-ichi . Mitsuoka. Toru . Moriya. Masashi . Murakami. Hirohumi . Murayama. Saori . Namai. Akira . Ozawa. Nozomi . Sato. Keisuke . Sueki. Mirei . Takeyama. Fuyuki . Tokanai. Takayuki . Yamaguchi. Atsushi . Yoshida. 10. 10. 1209.6431 . 2012JPSJ...81j3201M . 119217928 .
  4. Experiment on the Synthesis of Element 113 in the Reaction 209Bi(70Zn, n)278113. 10.1143/JPSJ.73.2593. 2004. Morita . Kosuke . Journal of the Physical Society of Japan . 73 . 2593–2596 . Morimoto . Kouji . Kaji . Daiya . Akiyama . Takahiro . Goto . Sin-Ichi . Haba . Hiromitsu . Ideguchi . Eiji . Kanungo . Rituparna . Katori . Kenji . Koura . Hiroyuki . Kudo . Hisaaki . Ohnishi . Tetsuya . Ozawa . Akira . Suda . Toshimi . Sueki . Keisuke . Xu . Hushan . Yamaguchi . Takayuki . Yoneda . Akira . Yoshida . Atsushi . Zhao . Yuliang . 8 . 10 . 2004JPSJ...73.2593M .
  5. Barber . Robert C. . Karol . Paul J . Nakahara . Hiromichi . Vardaci . Emanuele . Vogt . Erich W. . Discovery of the elements with atomic numbers greater than or equal to 113 (IUPAC Technical Report). 10.1351/PAC-REP-10-05-01 . Pure and Applied Chemistry . 2011 . 83. 7 . 1485. free .
  6. J.W. Beeman. et al. 2012. First Measurement of the Partial Widths of 209Bi Decay to the Ground and to the First Excited States. Physical Review Letters . 108 . 6 . 062501. 10.1103/PhysRevLett.108.062501. 22401058. 1110.3138. 118686992 .
  7. Davis . Andrew M. . 2022 . Short-Lived Nuclides in the Early Solar System: Abundances, Origins, and Applications . Annual Review of Nuclear and Particle Science . 72 . 339–363 . 10.1146/annurev-nucl-010722-074615 . 23 November 2023. free .
  8. Book: Koch. Lothar. Transuranium Elements, in Ullmann's Encyclopedia of Industrial Chemistry. Wiley. 2000. 10.1002/14356007.a27_167.
  9. Hoffman . D. C. . Lawrence . F. O. . Mewherter . J. L. . Rourke . F. M. . 1971. Detection of Plutonium-244 in Nature . . 234. 5325 . 132–134. 10.1038/234132a0 . 1971Natur.234..132H . 4283169 .
  10. Lachner. J.. etal. 2012. Attempt to detect primordial 244Pu on Earth. Physical Review C. 85. 1 . 015801. 10.1103/PhysRevC.85.015801. 2012PhRvC..85a5801L.
  11. Trenn . Thaddeus J. . 1978 . Thoruranium (U-236) as the extinct natural parent of thorium: The premature falsification of an essentially correct theory . Annals of Science . 35 . 6 . 581–97 . 10.1080/00033797800200441.
  12. Web site: . NuDat 3.0 database . Brookhaven National Laboratory. 19 Feb 2022.
  13. Web site: Nuclear Data. nucleardata.nuclear.lu.se. 2023-03-21. 2018-12-28. https://web.archive.org/web/20181228184025/http://nucleardata.nuclear.lu.se/. dead.
  14. Peppard . D. F. . Mason . G. W. . Gray . P. R. . Mech . J. F. . Occurrence of the (4n + 1) series in nature . Journal of the American Chemical Society . 1952 . 74 . 23 . 6081–6084 . 10.1021/ja01143a074 .
  15. Web site: Evaluated Nuclear Structure Data File. National Nuclear Data Center.
  16. Kuhn. W.. 1929. LXVIII. Scattering of thorium C" γ-radiation by radium G and ordinary lead. The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science. 8. 52. 628. 10.1080/14786441108564923. 1941-5982.
  17. Tsaletka . R. . Lapitskii . A. V. . 1960 . Occurrence of the Transuranium Elements in Nature . Russian Chemical Reviews . 29 . 12 . 684–689 . 20 January 2024.