Curium

Not to be confused with cerium.

This article is about the chemical element. For the ancient city located in Cyprus, see Kourion.

Curium, ₉₆Cm

Curium
Pronunciation	/ˈkjʊəriəm/ ​(KURE-ee-əm)
Appearance	silvery metallic, glows purple in the dark
Mass number	[247]
Curium in the periodic table
Hydrogen Helium Lithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine Neon Sodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine Argon Potassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine Krypton Rubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine Xenon Caesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury (element) Thallium Lead Bismuth Polonium Astatine Radon Francium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson Gd ↑ Cm ↓ (Upn) americium ← curium → berkelium
Atomic number (Z)	96
Group	f-block groups (no number)
Period	period 7
Block	f-block
Electron configuration	[ Rn ] 5f7 6d1 7s2
Electrons per shell	2, 8, 18, 32, 25, 9, 2
Physical properties
Phase at  STP	solid
Melting point	1613  K ​(1340 °C,​2444 °F)
Boiling point	3383 K​(3110 °C,​5630 °F)
Density (near r.t.)	13.51 g/cm3
Heat of fusion	13.85  kJ/mol
Vapor pressure P (Pa) 1 10 100 1 k 10 k 100 k at T (K) 1788 1982
Atomic properties
Oxidation states	+3, +4, +5, [1] +6 [2] (an  amphoteric oxide)
Electronegativity	Pauling scale: 1.3
Ionization energies	1st: 581 kJ/mol
Atomic radius	empirical:174  pm
Covalent radius	169±3 pm
Spectral lines of curium
Other properties
Natural occurrence	synthetic
Crystal structure	​ double hexagonal close-packed (dhcp)
Electrical resistivity	1.25 µΩ⋅m [3]
Magnetic ordering	antiferromagnetic-paramagnetic transition at 52 K [3]
CAS Number	7440-51-9
History
Naming	named after Marie Skłodowska-Curie and Pierre Curie
Discovery	Glenn T. Seaborg, Ralph A. James, Albert Ghiorso (1944)
Isotopes of curium v e
Main isotopes [4] Decay abun­dance half-life (t1/2) mode pro­duct 242Cm synth 162.8 d α 238Pu SF – 34Si 208Pb 243Cm synth 29.1 y α 239Pu ε 243Am SF – 244Cm synth 18.11 y α 240Pu SF – 245Cm synth 8250 y α 241Pu SF – 246Cm synth 4760 y α 242Pu SF – 247Cm synth 1.56×107 y α 243Pu 248Cm synth 3.480×105 y α 244Pu SF – 250Cm synth 8300 y SF – α 246Pu β− 250Bk
Category: Curium view talk edit | references

Curium is a synthetic chemical element; it has symbol Cm and atomic number 96. This transuranic actinide element was named after eminent scientists Marie and Pierre Curie, both known for their research on radioactivity. Curium was first intentionally made by the team of Glenn T. Seaborg, Ralph A. James, and Albert Ghiorso in 1944, using the cyclotron at Berkeley. They bombarded the newly discovered element plutonium (the isotope ²³⁹Pu) with alpha particles. This was then sent to the Metallurgical Laboratory at University of Chicago where a tiny sample of curium was eventually separated and identified. The discovery was kept secret until after the end of World War II. The news was released to the public in November 1947. Most curium is produced by bombarding uranium or plutonium with neutrons in nuclear reactors – one tonne of spent nuclear fuel contains ~20 grams of curium.

Curium is a hard, dense, silvery metal with a high melting and boiling point for an actinide. It is paramagnetic at ambient conditions, but becomes antiferromagnetic upon cooling, and other magnetic transitions are also seen in many curium compounds. In compounds, curium usually has valence +3 and sometimes +4; the +3 valence is predominant in solutions. Curium readily oxidizes, and its oxides are a dominant form of this element. It forms strongly fluorescent complexes with various organic compounds, but there is no evidence of its incorporation into bacteria and archaea. If it gets into the human body, curium accumulates in bones, lungs, and liver, where it promotes cancer.

All known isotopes of curium are radioactive and have small critical mass for a nuclear chain reaction. They mostly emit α-particles; radioisotope thermoelectric generators can use the heat from this process, but this is hindered by the rarity and high cost of curium. Curium is used in making heavier actinides and the ²³⁸Pu radionuclide for power sources in artificial cardiac pacemakers and RTGs for spacecraft. It served as the α-source in the alpha particle X-ray spectrometers of several space probes, including the Sojourner , Spirit , Opportunity , and Curiosity Mars rovers and the Philae lander on comet 67P/Churyumov–Gerasimenko, to analyze the composition and structure of the surface.

History

Glenn T. Seaborg

The 60-inch (150 cm) cyclotron at the Lawrence Radiation Laboratory, University of California, Berkeley, in August 1939.

Though curium had likely been produced in previous nuclear experiments as well as the natural nuclear fission reactor at Oklo, Gabon, it was first intentionally synthesized, isolated and identified in 1944, at University of California, Berkeley, by Glenn T. Seaborg, Ralph A. James, and Albert Ghiorso. In their experiments, they used a 60-inch (150 cm) cyclotron. ^[5]

Curium was chemically identified at the Metallurgical Laboratory (now Argonne National Laboratory), University of Chicago. It was the third transuranium element to be discovered even though it is the fourth in the series – the lighter element americium was still unknown. ^{[6] [7]}

The sample was prepared as follows: first plutonium nitrate solution was coated on a platinum foil of ~0.5 cm² area, the solution was evaporated and the residue was converted into plutonium(IV) oxide (PuO₂) by annealing. Following cyclotron irradiation of the oxide, the coating was dissolved with nitric acid and then precipitated as the hydroxide using concentrated aqueous ammonia solution. The residue was dissolved in perchloric acid, and further separation was done by ion exchange to yield a certain isotope of curium. The separation of curium and americium was so painstaking that the Berkeley group initially called those elements pandemonium (from Greek for all demons or hell) and delirium (from Latin for madness). ^{[8] [9]}

Curium-242 was made in July–August 1944 by bombarding ²³⁹Pu with α-particles to produce curium with the release of a neutron:

${\displaystyle {\ce {^{239}_{94}Pu + ^{4}_{2}He -> ^{242}_{96}Cm + ^{1}_{0}n}}}$

Curium-242 was unambiguously identified by the characteristic energy of the α-particles emitted during the decay:

${\displaystyle {\ce {^{242}_{96}Cm -> ^{238}_{94}Pu + ^{4}_{2}He}}}$

The half-life of this alpha decay was first measured as 150 days and then corrected to 162.8 days. ^[10]

Another isotope ²⁴⁰Cm was produced in a similar reaction in March 1945:

${\displaystyle {\ce {^{239}_{94}Pu + ^{4}_{2}He -> ^{240}_{96}Cm + 3^{1}_{0}n}}}$

The α-decay half-life of ²⁴⁰Cm was correctly determined as 26.7 days. ^[10]

The discovery of curium and americium in 1944 was closely related to the Manhattan Project, so the results were confidential and declassified only in 1945. Seaborg leaked the synthesis of the elements 95 and 96 on the U.S. radio show for children, the Quiz Kids, five days before the official presentation at an American Chemical Society meeting on November 11, 1945, when one listener asked if any new transuranic element beside plutonium and neptunium had been discovered during the war. ^[8] The discovery of curium (²⁴²Cm and ²⁴⁰Cm), its production, and its compounds was later patented listing only Seaborg as the inventor. ^[11]

Marie and Pierre Curie

The element was named after Marie Curie and her husband Pierre Curie, who are known for discovering radium and for their work in radioactivity. It followed the example of gadolinium, a lanthanide element above curium in the periodic table, which was named after the explorer of rare-earth elements Johan Gadolin: ^[12]

"As the name for the element of atomic number 96 we should like to propose "curium", with symbol Cm. The evidence indicates that element 96 contains seven 5f electrons and is thus analogous to the element gadolinium, with its seven 4f electrons in the regular rare earth series. On this basis element 96 is named after the Curies in a manner analogous to the naming of gadolinium, in which the chemist Gadolin was honored." ^[6]

The first curium samples were barely visible, and were identified by their radioactivity. Louis Werner and Isadore Perlman made the first substantial sample of 30 µg curium-242 hydroxide at University of California, Berkeley in 1947 by bombarding americium-241 with neutrons. ^{[13] [14] [15]} Macroscopic amounts of curium(III) fluoride were obtained in 1950 by W. W. T. Crane, J. C. Wallmann and B. B. Cunningham. Its magnetic susceptibility was very close to that of GdF₃ providing the first experimental evidence for the +3 valence of curium in its compounds. ^[13] Curium metal was produced only in 1951 by reduction of CmF₃ with barium. ^{[16] [17]}

Characteristics

Physical

Double-hexagonal close packing with the layer sequence ABAC in the crystal structure of α-curium (A: green, B: blue, C: red)

Photoluminescence of the Cm(HDPA)₃·H₂O crystal upon irradiation with 420 nm light

A synthetic, radioactive element, curium is a hard, dense metal with a silvery-white appearance and physical and chemical properties resembling gadolinium. Its melting point of 1344 °C is significantly higher than that of the previous elements neptunium (637 °C), plutonium (639 °C) and americium (1176 °C). In comparison, gadolinium melts at 1312 °C. Curium boils at 3556 °C. With a density of 13.52 g/cm³, curium is lighter than neptunium (20.45 g/cm³) and plutonium (19.8 g/cm³), but heavier than most other metals. Of two crystalline forms of curium, α-Cm is more stable at ambient conditions. It has a hexagonal symmetry, space group P6₃/mmc, lattice parameters a = 365  pm and c = 1182 pm, and four formula units per unit cell. ^[18] The crystal consists of double-hexagonal close packing with the layer sequence ABAC and so is isotypic with α-lanthanum. At pressure >23  GPa, at room temperature, α-Cm becomes β-Cm, which has face-centered cubic symmetry, space group Fm3m and lattice constant a = 493 pm. ^[18] On further compression to 43 GPa, curium becomes an orthorhombic γ-Cm structure similar to α-uranium, with no further transitions observed up to 52 GPa. These three curium phases are also called Cm I, II and III. ^{[19] [20]}

Curium has peculiar magnetic properties. Its neighbor element americium shows no deviation from Curie-Weiss paramagnetism in the entire temperature range, but α-Cm transforms to an antiferromagnetic state upon cooling to 65–52 K, ^{[21] [22]} and β-Cm exhibits a ferrimagnetic transition at ~205 K. Curium pnictides show ferromagnetic transitions upon cooling: ²⁴⁴CmN and ²⁴⁴CmAs at 109 K, ²⁴⁸CmP at 73 K and ²⁴⁸CmSb at 162 K. The lanthanide analog of curium, gadolinium, and its pnictides, also show magnetic transitions upon cooling, but the transition character is somewhat different: Gd and GdN become ferromagnetic, and GdP, GdAs and GdSb show antiferromagnetic ordering. ^[23]

In accordance with magnetic data, electrical resistivity of curium increases with temperature – about twice between 4 and 60 K – and then is nearly constant up to room temperature. There is a significant increase in resistivity over time (~10 µΩ·cm/h) due to self-damage of the crystal lattice by alpha decay. This makes uncertain the true resistivity of curium (~125 µΩ·cm). Curium's resistivity is similar to that of gadolinium, and the actinides plutonium and neptunium, but significantly higher than that of americium, uranium, polonium and thorium. ^{[3] [24]}

Under ultraviolet illumination, curium(III) ions show strong and stable yellow-orange fluorescence with a maximum in the range of 590–640 nm depending on their environment. ^[25] The fluorescence originates from the transitions from the first excited state ⁶D_7/2 and the ground state ⁸S_7/2. Analysis of this fluorescence allows monitoring interactions between Cm(III) ions in organic and inorganic complexes. ^[26]

Chemical

A solution of curium

Curium ion in solution almost always has a +3 oxidation state, the most stable oxidation state for curium. ^[27] A +4 oxidation state is seen mainly in a few solid phases, such as CmO₂ and CmF₄. ^{[28] [29]} Aqueous curium(IV) is only known in the presence of strong oxidizers such as potassium persulfate, and is easily reduced to curium(III) by radiolysis and even by water itself. ^[30] Chemical behavior of curium is different from the actinides thorium and uranium, and is similar to americium and many lanthanides. In aqueous solution, the Cm³⁺ ion is colorless to pale green; ^[31] Cm⁴⁺ ion is pale yellow. ^[32] The optical absorption of Cm³⁺ ion contains three sharp peaks at 375.4, 381.2 and 396.5 nm and their strength can be directly converted into the concentration of the ions. ^[33] The +6 oxidation state has only been reported once in solution in 1978, as the curyl ion (CmO²⁺
₂): this was prepared from beta decay of americium-242 in the americium(V) ion ²⁴²
AmO⁺
₂. ^[2] Failure to get Cm(VI) from oxidation of Cm(III) and Cm(IV) may be due to the high Cm⁴⁺/Cm³⁺ ionization potential and the instability of Cm(V). ^[30]

Curium ions are hard Lewis acids and thus form most stable complexes with hard bases. ^[34] The bonding is mostly ionic, with a small covalent component. ^[35] Curium in its complexes commonly exhibits a 9-fold coordination environment, with a tricapped trigonal prismatic molecular geometry. ^[36]

Isotopes

See also: Isotopes of curium

About 19 radioisotopes and 7 nuclear isomers, ²³³Cm to ²⁵¹Cm, are known; none are stable. The longest half-lives are 15.6 million years (²⁴⁷Cm) and 348,000 years (²⁴⁸Cm). Other long-lived ones are ²⁴⁵Cm (8500 years), ²⁵⁰Cm (8300 years) and ²⁴⁶Cm (4760 years). Curium-250 is unusual: it mostly (~86%) decays by spontaneous fission. The most commonly used isotopes are ²⁴²Cm and ²⁴⁴Cm with the half-lives 162.8 days and 18.1 years, respectively. ^[10]

Thermal neutron cross sections (barns) [37]
	242Cm	243Cm	244Cm	245Cm	246Cm	247Cm
Fission	5	617	1.04	2145	0.14	81.90
Capture	16	130	15.20	369	1.22	57
C/F ratio	3.20	0.21	14.62	0.17	8.71	0.70
LEU spent nuclear fuel 20 years after 53 MWd/kg burnup [38]
3 common isotopes		51	3700	390
Fast-neutron reactor MOX fuel (avg 5 samples, burnup 66–120 GWd/t) [39]
Total curium 3.09×10−3%		27.64%	70.16%	2.166%	0.0376%	0.000928%

Isotope	242Cm	243Cm	244Cm	245Cm	246Cm	247Cm	248Cm	250Cm
Critical mass, kg	25	7.5	33	6.8	39	7	40.4	23.5

All isotopes ranging from ²⁴²Cm to ²⁴⁸Cm, as well as ²⁵⁰Cm, undergo a self-sustaining nuclear chain reaction and thus in principle can be a nuclear fuel in a reactor. As in most transuranic elements, nuclear fission cross section is especially high for the odd-mass curium isotopes ²⁴³Cm, ²⁴⁵Cm and ²⁴⁷Cm. These can be used in thermal-neutron reactors, whereas a mixture of curium isotopes is only suitable for fast breeder reactors since the even-mass isotopes are not fissile in a thermal reactor and accumulate as burn-up increases. ^[40] The mixed-oxide (MOX) fuel, which is to be used in power reactors, should contain little or no curium because neutron activation of ²⁴⁸Cm will create californium. Californium is a strong neutron emitter, and would pollute the back end of the fuel cycle and increase the dose to reactor personnel. Hence, if minor actinides are to be used as fuel in a thermal neutron reactor, the curium should be excluded from the fuel or placed in special fuel rods where it is the only actinide present. ^[41]

Transmutation flow between Pu and Cm in LWR.
Fission percentage is 100 minus shown percentages.
Total rate of transmutation varies greatly by nuclide.
Cm– Cm are long-lived with negligible decay.

The adjacent table lists the critical masses for curium isotopes for a sphere, without moderator or reflector. With a metal reflector (30 cm of steel), the critical masses of the odd isotopes are about 3–4 kg. When using water (thickness ~20–30 cm) as the reflector, the critical mass can be as small as 59 grams for ²⁴⁵Cm, 155 grams for ²⁴³Cm and 1550 grams for ²⁴⁷Cm. There is significant uncertainty in these critical mass values. While it is usually on the order of 20%, the values for ²⁴²Cm and ²⁴⁶Cm were listed as large as 371 kg and 70.1 kg, respectively, by some research groups. ^{[40] [43]}

Curium is not currently used as nuclear fuel due to its low availability and high price. ^{[44] 245}Cm and ²⁴⁷Cm have very small critical mass and so could be used in tactical nuclear weapons, but none are known to have been made. Curium-243 is not suitable for such, due to its short half-life and strong α emission, which would cause excessive heat. ^[45] Curium-247 would be highly suitable due to its long half-life, which is 647 times longer than plutonium-239 (used in many existing nuclear weapons).

Occurrence

Several isotopes of curium were detected in the fallout from the Ivy Mike nuclear test.

The longest-lived isotope, ²⁴⁷Cm, has half-life 15.6 million years; so any primordial curium, that is, present on Earth when it formed, should have decayed by now. Its past presence as an extinct radionuclide is detectable as an excess of its primordial, long-lived daughter ²³⁵U. ^[46] Traces of curium may occur naturally in uranium minerals due to neutron capture and beta decay, though this has not been confirmed. ^{[47] [48]} Traces of ²⁴⁷Cm are also probably brought to Earth in cosmic rays, but again this has not been confirmed. ^[49]

Curium is made artificially in small amounts for research purposes. It also occurs as one of the waste products in spent nuclear fuel. ^{[50] [51]} Curium is present in nature in some areas used for nuclear weapons testing. ^[52] Analysis of the debris at the test site of the United States' first thermonuclear weapon, Ivy Mike, (1 November 1952, Enewetak Atoll), besides einsteinium, fermium, plutonium and americium also revealed isotopes of berkelium, californium and curium, in particular ²⁴⁵Cm, ²⁴⁶Cm and smaller quantities of ²⁴⁷Cm, ²⁴⁸Cm and ²⁴⁹Cm. ^[53]

Atmospheric curium compounds are poorly soluble in common solvents and mostly adhere to soil particles. Soil analysis revealed about 4,000 times higher concentration of curium at the sandy soil particles than in water present in the soil pores. An even higher ratio of about 18,000 was measured in loam soils. ^[54]

The transuranium elements from americium to fermium, including curium, occurred naturally in the natural nuclear fission reactor at Oklo, but no longer do so. ^[55]

Curium, and other non-primordial actinides, have also been suspected to exist in the spectrum of Przybylski's Star. ^[56]

Synthesis

Isotope preparation

Curium is made in small amounts in nuclear reactors, and by now only kilograms of ²⁴²Cm and ²⁴⁴Cm have been accumulated, and grams or even milligrams for heavier isotopes. Hence the high price of curium, which has been quoted at 160–185 USD per milligram, ^[13] with a more recent estimate at US$2,000/g for ²⁴²Cm and US$170/g for ²⁴⁴Cm. ^[57] In nuclear reactors, curium is formed from ²³⁸U in a series of nuclear reactions. In the first chain, ²³⁸U captures a neutron and converts into ²³⁹U, which via β⁻ decay transforms into ²³⁹Np and ²³⁹Pu.

${\displaystyle {\ce {^{238}_{92}U->[{\ce {(n,\gamma )}}]{^{239}_{92}U}->[\beta ^{-}][23.5\ {\ce {min}}]_{93}^{239}Np->[\beta ^{-}][2.3565\ {\ce {d}}]_{94}^{239}Pu}}}$(the times are half-lives).

(1)

Further neutron capture followed by β⁻-decay gives americium (²⁴¹Am) which further becomes ²⁴²Cm:

${\displaystyle {\ce {^{239}_{94}Pu->[{\ce {2(n,\gamma )}}]_{94}^{241}Pu->[\beta ^{-}][14.35\ {\ce {yr}}]{^{241}_{95}Am}->[{\ce {(n,\gamma )}}]_{95}^{242}Am->[\beta ^{-}][16.02{\ce {h}}]_{96}^{242}Cm}}}$.

(2)

For research purposes, curium is obtained by irradiating not uranium but plutonium, which is available in large amounts from spent nuclear fuel. A much higher neutron flux is used for the irradiation that results in a different reaction chain and formation of ²⁴⁴Cm: ^[7]

${\displaystyle {\ce {^{239}_{94}Pu->[{\ce {4(n,\gamma )}}]_{94}^{243}Pu->[\beta ^{-}][4.956\ {\ce {h}}]_{95}^{243}Am->[({\ce {n}},\gamma )]_{95}^{244}Am->[\beta ^{-}][10.1{\ce {h}}]_{96}^{244}Cm->[\alpha ][18.11\ {\ce {yr}}]_{94}^{240}Pu}}}$

(3)

Curium-244 alpha decays to ²⁴⁰Pu, but it also absorbs neutrons, hence a small amount of heavier curium isotopes. Of those, ²⁴⁷Cm and ²⁴⁸Cm are popular in scientific research due to their long half-lives. But the production rate of ²⁴⁷Cm in thermal neutron reactors is low because it is prone to fission due to thermal neutrons. ^[58] Synthesis of ²⁵⁰Cm by neutron capture is unlikely due to the short half-life of the intermediate ²⁴⁹Cm (64 min), which β⁻ decays to the berkelium isotope ²⁴⁹Bk. ^[58]

${\displaystyle {\ce {^{\mathit {A}}_{96}Cm{}+_{0}^{1}n->_{96}^{{\mathit {A}}+1}Cm{}+\gamma }}\ ({\text{for }}244\leq A\leq 248)}$

(4)

The above cascade of (n,γ) reactions gives a mix of different curium isotopes. Their post-synthesis separation is cumbersome, so a selective synthesis is desired. Curium-248 is favored for research purposes due to its long half-life. The most efficient way to prepare this isotope is by α-decay of the californium isotope ²⁵²Cf, which is available in relatively large amounts due to its long half-life (2.65 years). About 35–50 mg of ²⁴⁸Cm is produced thus, per year. The associated reaction produces ²⁴⁸Cm with isotopic purity of 97%. ^[58]

${\displaystyle {\begin{matrix}{}\\{\ce {^{252}_{98}Cf ->[\alpha][2.645\ {\ce {yr}}] ^{248}_{96}Cm}}\\{}\end{matrix}}}$

(5)

Another isotope, ²⁴⁵Cm, can be obtained for research, from α-decay of ²⁴⁹Cf; the latter isotope is produced in small amounts from β⁻-decay of ²⁴⁹ Bk.

${\displaystyle {\ce {^{249}_{97}Bk ->[\beta^-][330\ {\ce {d}}] ^{249}_{98}Cf ->[\alpha][351\ {\ce {yr}}] ^{245}_{96}Cm}}}$

(6)

Metal preparation

Chromatographic elution curves revealing the similarity between Tb, Gd, Eu lanthanides and corresponding Bk, Cm, Am actinides.

Most synthesis routines yield a mix of actinide isotopes as oxides, from which a given isotope of curium needs to be separated. An example procedure could be to dissolve spent reactor fuel (e.g. MOX fuel) in nitric acid, and remove the bulk of the uranium and plutonium using a PUREX (Plutonium – URanium EXtraction) type extraction with tributyl phosphate in a hydrocarbon. The lanthanides and the remaining actinides are then separated from the aqueous residue (raffinate) by a diamide-based extraction to give, after stripping, a mixture of trivalent actinides and lanthanides. A curium compound is then selectively extracted using multi-step chromatographic and centrifugation techniques with an appropriate reagent. ^[59] Bis-triazinyl bipyridine complex has been recently proposed as such reagent which is highly selective to curium. ^[60] Separation of curium from the very chemically similar americium can also be done by treating a slurry of their hydroxides in aqueous sodium bicarbonate with ozone at elevated temperature. Both americium and curium are present in solutions mostly in the +3 valence state; americium oxidizes to soluble Am(IV) complexes, but curium stays unchanged and so can be isolated by repeated centrifugation. ^[61]

Metallic curium is obtained by reduction of its compounds. Initially, curium(III) fluoride was used for this purpose. The reaction was done in an environment free of water and oxygen, in an apparatus made of tantalum and tungsten, using elemental barium or lithium as reducing agents. ^{[7] [16] [62] [63] [64]}

${\displaystyle \mathrm {CmF_{3}\ +\ 3\ Li\ \longrightarrow \ Cm\ +\ 3\ LiF} }$

Another possibility is reduction of curium(IV) oxide using a magnesium-zinc alloy in a melt of magnesium chloride and magnesium fluoride. ^[65]

Compounds and reactions

See also: Category:Curium compounds

Oxides

Curium readily reacts with oxygen forming mostly Cm₂O₃ and CmO₂ oxides, ^[52] but the divalent oxide CmO is also known. ^[66] Black CmO₂ can be obtained by burning curium oxalate (Cm
_²(C
_²O
_⁴)
_³), nitrate (Cm(NO
_³)
_³), or hydroxide in pure oxygen. ^{[29] [67]} Upon heating to 600–650 °C in vacuum (about 0.01 Pa), it transforms into the whitish Cm₂O₃: ^{[29] [68]}

${\displaystyle {\ce {4CmO2 ->[\Delta T] 2Cm2O3 + O2}}}$.

Or, Cm₂O₃ can be obtained by reducing CmO₂ with molecular hydrogen: ^[69]

${\displaystyle {\ce {2CmO2 + H2 -> Cm2O3 + H2O}}}$

Also, a number of ternary oxides of the type M(II)CmO₃ are known, where M stands for a divalent metal, such as barium. ^[70]

Thermal oxidation of trace quantities of curium hydride (CmH_2–3) has been reported to give a volatile form of CmO₂ and the volatile trioxide CmO₃, one of two known examples of the very rare +6 state for curium. ^[2] Another observed species was reported to behave similar to a supposed plutonium tetroxide and was tentatively characterized as CmO₄, with curium in the extremely rare +8 state; ^[71] but new experiments seem to indicate that CmO₄ does not exist, and have cast doubt on the existence of PuO₄ as well. ^[72]

Halides

The colorless curium(III) fluoride (CmF₃) can be made by adding fluoride ions into curium(III)-containing solutions. The brown tetravalent curium(IV) fluoride (CmF₄) on the other hand is only obtained by reacting curium(III) fluoride with molecular fluorine: ^[7]

${\displaystyle \mathrm {2\ CmF_{3}\ +\ F_{2}\ \longrightarrow \ 2\ CmF_{4}} }$

A series of ternary fluorides are known of the form A₇Cm₆F₃₁ (A = alkali metal). ^[73]

The colorless curium(III) chloride (CmCl₃) is made by reacting curium hydroxide (Cm(OH)₃) with anhydrous hydrogen chloride gas. It can be further turned into other halides such as curium(III) bromide (colorless to light green) and curium(III) iodide (colorless), by reacting it with the ammonia salt of the corresponding halide at temperatures of ~400–450°C: ^[74]

${\displaystyle \mathrm {CmCl_{3}\ +\ 3\ NH_{4}I\ \longrightarrow \ CmI_{3}\ +\ 3\ NH_{4}Cl} }$

Or, one can heat curium oxide to ~600°C with the corresponding acid (such as hydrobromic for curium bromide). ^{[75] [76]} Vapor phase hydrolysis of curium(III) chloride gives curium oxychloride: ^[77]

${\displaystyle \mathrm {CmCl_{3}\ +\ \ H_{2}O\ \longrightarrow \ CmOCl\ +\ 2\ HCl} }$

Chalcogenides and pnictides

Sulfides, selenides and tellurides of curium have been obtained by treating curium with gaseous sulfur, selenium or tellurium in vacuum at elevated temperature. ^{[78] [79]} Curium pnictides of the type CmX are known for nitrogen, phosphorus, arsenic and antimony. ^[7] They can be prepared by reacting either curium(III) hydride (CmH₃) or metallic curium with these elements at elevated temperature. ^[80]

Organocurium compounds and biological aspects

Predicted curocene structure

Organometallic complexes analogous to uranocene are known also for other actinides, such as thorium, protactinium, neptunium, plutonium and americium. Molecular orbital theory predicts a stable "curocene" complex (η⁸-C₈H₈)₂Cm, but it has not been reported experimentally yet. ^{[81] [82]}

Formation of the complexes of the type Cm(n-C
_³H
_⁷-BTP)
_³ (BTP = 2,6-di(1,2,4-triazin-3-yl)pyridine), in solutions containing n-C₃H₇-BTP and Cm³⁺ ions has been confirmed by EXAFS. Some of these BTP-type complexes selectively interact with curium and thus are useful for separating it from lanthanides and another actinides. ^{[25] [83]} Dissolved Cm³⁺ ions bind with many organic compounds, such as hydroxamic acid, ^[84] urea, ^[85] fluorescein ^[86] and adenosine triphosphate. ^[87] Many of these compounds are related to biological activity of various microorganisms. The resulting complexes show strong yellow-orange emission under UV light excitation, which is convenient not only for their detection, but also for studying interactions between the Cm³⁺ ion and the ligands via changes in the half-life (of the order ~0.1 ms) and spectrum of the fluorescence. ^{[26] [84] [85] [86] [87]}

Curium has no biological significance. ^[88] There are a few reports on biosorption of Cm³⁺ by bacteria and archaea, but no evidence for incorporation of curium into them. ^{[89] [90]}

Applications

Radionuclides

The radiation from curium is so strong that the metal glows purple in the dark.

Curium is one of the most radioactive isolable elements. Its two most common isotopes ²⁴²Cm and ²⁴⁴Cm are strong alpha emitters (energy 6 MeV); they have fairly short half-lives, 162.8 days and 18.1 years, and give as much as 120 W/g and 3 W/g of heat, respectively. ^{[13] [91] [92]} Therefore, curium can be used in its common oxide form in radioisotope thermoelectric generators like those in spacecraft. This application has been studied for the ²⁴⁴Cm isotope, while ²⁴²Cm was abandoned due to its prohibitive price, around 2000 USD/g. ²⁴³Cm with a ~30-year half-life and good energy yield of ~1.6 W/g could be a suitable fuel, but it gives significant amounts of harmful gamma and beta rays from radioactive decay products. As an α-emitter, ²⁴⁴Cm needs much less radiation shielding, but it has a high spontaneous fission rate, and thus a lot of neutron and gamma radiation. Compared to a competing thermoelectric generator isotope such as ²³⁸Pu, ²⁴⁴Cm emits 500 times more neutrons, and its higher gamma emission requires a shield that is 20 times thicker—2 inches (51 mm) of lead for a 1 kW source, compared to 0.1 inches (2.5 mm) for ²³⁸Pu. Therefore, this use of curium is currently considered impractical. ^[57]

A more promising use of ²⁴²Cm is for making ²³⁸Pu, a better radioisotope for thermoelectric generators such as in heart pacemakers. The alternate routes to ²³⁸Pu use the (n,γ) reaction of ²³⁷Np, or deuteron bombardment of uranium, though both reactions always produce ²³⁶Pu as an undesired by-product since the latter decays to ²³²U with strong gamma emission. ^[93] Curium is a common starting material for making higher transuranic and superheavy elements. Thus, bombarding ²⁴⁸Cm with neon (²²Ne), magnesium (²⁶Mg), or calcium (⁴⁸Ca) yields isotopes of seaborgium (²⁶⁵Sg), hassium (²⁶⁹Hs and ²⁷⁰Hs), and livermorium (²⁹²Lv, ²⁹³Lv, and possibly ²⁹⁴Lv). ^[94] Californium was discovered when a microgram-sized target of curium-242 was irradiated with 35 MeV alpha particles using the 60-inch (150 cm) cyclotron at Berkeley:

²⁴²
₉₆Cm
+ ⁴
₂He
→ ²⁴⁵
₉₈Cf
+ ¹
₀n

Only about 5,000 atoms of californium were produced in this experiment. ^[95]

The odd-mass curium isotopes ²⁴³Cm, ²⁴⁵Cm, and ²⁴⁷Cm are all highly fissile and can release additional energy in a thermal spectrum nuclear reactor. All curium isotopes are fissionable in fast-neutron reactors. This is one of the motives for minor actinide separation and transmutation in the nuclear fuel cycle, helping to reduce the long-term radiotoxicity of used, or spent nuclear fuel.

Alpha-particle X-ray spectrometer of a Mars exploration rover

X-ray spectrometer

The most practical application of ²⁴⁴Cm—though rather limited in total volume—is as α-particle source in alpha particle X-ray spectrometers (APXS). These instruments were installed on the Sojourner, Mars, Mars 96, Mars Exploration Rovers and Philae comet lander, ^[96] as well as the Mars Science Laboratory to analyze the composition and structure of the rocks on the surface of planet Mars. ^[97] APXS was also used in the Surveyor 5–7 moon probes but with a ²⁴²Cm source. ^{[54] [98] [99]}

An elaborate APXS setup has a sensor head containing six curium sources with a total decay rate of several tens of millicuries (roughly one gigabecquerel). The sources are collimated on a sample, and the energy spectra of the alpha particles and protons scattered from the sample are analyzed (proton analysis is done only in some spectrometers). These spectra contain quantitative information on all major elements in the sample except for hydrogen, helium and lithium. ^[100]

Safety

Due to its radioactivity, curium and its compounds must be handled in appropriate labs under special arrangements. While curium itself mostly emits α-particles which are absorbed by thin layers of common materials, some of its decay products emit significant fractions of beta and gamma rays, which require a more elaborate protection. ^[52] If consumed, curium is excreted within a few days and only 0.05% is absorbed in the blood. From there, ~45% goes to the liver, 45% to the bones, and the remaining 10% is excreted. In bone, curium accumulates on the inside of the interfaces to the bone marrow and does not significantly redistribute with time; its radiation destroys bone marrow and thus stops red blood cell creation. The biological half-life of curium is about 20 years in the liver and 50 years in the bones. ^{[52] [54]} Curium is absorbed in the body much more strongly via inhalation, and the allowed total dose of ²⁴⁴Cm in soluble form is 0.3 μCi. ^[13] Intravenous injection of ²⁴²Cm- and ²⁴⁴Cm-containing solutions to rats increased the incidence of bone tumor, and inhalation promoted lung and liver cancer. ^[52]

Curium isotopes are inevitably present in spent nuclear fuel (about 20 g/tonne). ^[101] The isotopes ²⁴⁵Cm–²⁴⁸Cm have decay times of thousands of years and must be removed to neutralize the fuel for disposal. ^[102] Such a procedure involves several steps, where curium is first separated and then converted by neutron bombardment in special reactors to short-lived nuclides. This procedure, nuclear transmutation, while well documented for other elements, is still being developed for curium. ^[25]

References

1. Kovács, Attila; Dau, Phuong D.; Marçalo, Joaquim; Gibson, John K. (2018). "Pentavalent Curium, Berkelium, and Californium in Nitrate Complexes: Extending Actinide Chemistry and Oxidation States". Inorg. Chem. American Chemical Society. 57 (15): 9453–9467. doi:10.1021/acs.inorgchem.8b01450. OSTI   1631597. PMID   30040397. S2CID   51717837.
2. Domanov, V. P.; Lobanov, Yu. V. (October 2011). "Formation of volatile curium(VI) trioxide CmO₃". Radiochemistry. SP MAIK Nauka/Interperiodica. 53 (5): 453–6. doi:10.1134/S1066362211050018. S2CID   98052484.
3. Schenkel, R. (1977). "The electrical resistivity of 244Cm metal". Solid State Communications. 23 (6): 389. Bibcode:1977SSCom..23..389S. doi:10.1016/0038-1098(77)90239-3.
4. Kondev, 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.
5. Hall, Nina (2000). The New Chemistry: A Showcase for Modern Chemistry and Its Applications . Cambridge University Press. pp.  8–9. ISBN   978-0-521-45224-3.
6. Seaborg, Glenn T.; James, R. A.; Ghiorso, A. (1949). "The New Element Curium (Atomic Number 96)" (PDF). NNES PPR (National Nuclear Energy Series, Plutonium Project Record). The Transuranium Elements: Research Papers, Paper No. 22.2. 14 B. OSTI   4421946. Archived from the original (PDF) on 12 October 2007.
7. Morss, L. R.; Edelstein, N. M. and Fugere, J. (eds): The Chemistry of the Actinide Elements and transactinides, volume 3, Springer-Verlag, Dordrecht 2006, ISBN   1-4020-3555-1.
8. Pepling, Rachel Sheremeta (2003). "Chemical & Engineering News: It's Elemental: The Periodic Table – Americium" . Retrieved 2008-12-07.
9. Krebs, Robert E. The history and use of our earth's chemical elements: a reference guide, Greenwood Publishing Group, 2006, ISBN   0-313-33438-2 p. 322
10. Audi, Georges; Bersillon, Olivier; Blachot, Jean; Wapstra, Aaldert Hendrik (1997). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 624 (1): 1–124. Bibcode:1997NuPhA.624....1A. doi:10.1016/S0375-9474(97)00482-X. Archived from the original (PDF) on 2008-09-23.
11. Seaborg, G. T. U.S. Patent 3,161,462 "Element", Filing date: 7 February 1949, Issue date: December 1964
12. Greenwood, p. 1252
13. Hammond C. R. "The elements" in Lide, D. R., ed. (2005). CRC Handbook of Chemistry and Physics (86th ed.). Boca Raton (FL): CRC Press. ISBN   0-8493-0486-5.
14. L. B. Werner, I. Perlman: "Isolation of Curium", NNES PPR (National Nuclear Energy Series, Plutonium Project Record), Vol. 14 B, The Transuranium Elements: Research Papers, Paper No. 22.5, McGraw-Hill Book Co., Inc., New York, 1949.
15. "National Academy of Sciences. Isadore Perlman 1915–1991". Nap.edu. Retrieved 2011-03-25.
16. Wallmann, J. C.; Crane, W. W. T.; Cunningham, B. B. (1951). "The Preparation and Some Properties of Curium Metal" (PDF). Journal of the American Chemical Society . 73 (1): 493–494. doi:10.1021/ja01145a537. hdl:2027/mdp.39015086479790.
17. Werner, L. B.; Perlman, I. (1951). "First Isolation of Curium". Journal of the American Chemical Society. 73 (1): 5215–5217. doi:10.1021/ja01155a063. S2CID   95799539.
18. Milman, V.; Winkler, B.; Pickard, C. J. (2003). "Crystal structures of curium compounds: an ab initio study". Journal of Nuclear Materials. 322 (2–3): 165. Bibcode:2003JNuM..322..165M. doi:10.1016/S0022-3115(03)00321-0.
19. Young, D. A. Phase diagrams of the elements, University of California Press, 1991, ISBN   0-520-07483-1, p. 227
20. Haire, R.; Peterson, J.; Benedict, U.; Dufour, C.; Itie, J. (1985). "X-ray diffraction of curium-248 metal under pressures of up to 52 GPa". Journal of the Less Common Metals. 109 (1): 71. doi:10.1016/0022-5088(85)90108-0.
21. Kanellakopulos, B.; Blaise, A.; Fournier, J. M.; Müller, W. (1975). "The magnetic susceptibility of Americium and curium metal". Solid State Communications. 17 (6): 713. Bibcode:1975SSCom..17..713K. doi:10.1016/0038-1098(75)90392-0.
22. Fournier, J.; Blaise, A.; Muller, W.; Spirlet, J.-C. (1977). "Curium: A new magnetic element". Physica B+C. 86–88: 30. Bibcode:1977PhyBC..86...30F. doi:10.1016/0378-4363(77)90214-5.
23. Nave, S. E.; Huray, P. G.; Peterson, J. R. and Damien, D. A. Magnetic susceptibility of curium pnictides, Oak Ridge National Laboratory
24. Schenkel, R. (1977). "The electrical resistivity of 244Cm metal". Solid State Communications. 23 (6): 389. Bibcode:1977SSCom..23..389S. doi:10.1016/0038-1098(77)90239-3.
25. Denecke, Melissa A.; Rossberg, André; Panak, Petra J.; Weigl, Michael; Schimmelpfennig, Bernd; Geist, Andreas (2005). "Characterization and Comparison of Cm(III) and Eu(III) Complexed with 2,6-Di(5,6-dipropyl-1,2,4-triazin-3-yl)pyridine Using EXAFS, TRFLS, and Quantum-Chemical Methods". Inorganic Chemistry. 44 (23): 8418–8425. doi:10.1021/ic0511726. PMID   16270980.
26. Bünzli, J.-C. G. and Choppin, G. R. Lanthanide probes in life, chemical, and earth sciences: theory and practice, Elsevier, Amsterdam, 1989 ISBN   0-444-88199-9
27. Penneman, p. 24
28. Keenan, Thomas K. (1961). "First Observation of Aqueous Tetravalent Curium". Journal of the American Chemical Society. 83 (17): 3719. doi:10.1021/ja01478a039.
29. Asprey, L. B.; Ellinger, F. H.; Fried, S.; Zachariasen, W. H. (1955). "Evidence for Quadrivalent Curium: X-Ray Data on Curium Oxides1". Journal of the American Chemical Society. 77 (6): 1707. doi:10.1021/ja01611a108.
30. Gregg J., Lumetta; Thompson, Major C.; Penneman, Robert A.; Eller, P. Gary (2006). "Curium". In Morss, Lester R.; Edelstein, Norman M.; Fuger, Jean (eds.). The Chemistry of the Actinide and Transactinide Elements (PDF). Vol. 3 (3rd ed.). Dordrecht, the Netherlands: Springer. pp. 1397–1443. doi:10.1007/1-4020-3598-5_9. ISBN   978-1-4020-3555-5. Archived from the original (PDF) on 2018-01-17. Retrieved 2013-10-18.
31. Greenwood, p. 1265
32. Holleman, p. 1956
33. Penneman, pp. 25–26
34. Jensen, Mark P.; Bond, Andrew H. (2002). "Comparison of Covalency in the Complexes of Trivalent Actinide and Lanthanide Cations". Journal of the American Chemical Society. 124 (33): 9870–9877. doi:10.1021/ja0178620. PMID   12175247.
35. Seaborg, Glenn T. (1993). "Overview of the Actinide and Lanthanide (the f) Elements". Radiochimica Acta. 61 (3–4): 115–122. doi:10.1524/ract.1993.61.34.115. S2CID   99634366.
36. Greenwood, p. 1267
37. Pfennig, G.; Klewe-Nebenius, H. and Seelmann Eggebert, W. (Eds.): Karlsruhe nuclide, 6th Ed. 1998
38. Kang, Jungmin; Von Hippel, Frank (2005). "Limited Proliferation-Resistance Benefits from Recycling Unseparated Transuranics and Lanthanides from Light-Water Reactor Spent Fuel" (PDF). Science and Global Security. 13 (3): 169. Bibcode:2005S&GS...13..169K. doi:10.1080/08929880500357682. S2CID   123552796. Archived (PDF) from the original on 2011-11-28.
39. Osaka, M.; et al. (2001). "Analysis of Curium Isotopes in Mixed Oxide Fuel Irradiated in Fast Reactor". Journal of Nuclear Science and Technology. 38 (10): 912–914. doi: 10.3327/jnst.38.912 .
40. Institut de Radioprotection et de Sûreté Nucléaire: "Evaluation of nuclear criticality safety. data and limits for actinides in transport" Archived May 19, 2011, at the Wayback Machine , p. 16
41. National Research Council (U.S.). Committee on Separations Technology and Transmutation Systems (1996). Nuclear wastes: technologies for separations and transmutation. National Academies Press. pp. 231–. ISBN   978-0-309-05226-9 . Retrieved 19 April 2011.
42. Sasahara, Akihiro; Matsumura, Tetsuo; Nicolaou, Giorgos; Papaioannou, Dimitri (2004). "Neutron and Gamma Ray Source Evaluation of LWR High Burn-up UO2 and MOX Spent Fuels" (PDF). Journal of Nuclear Science and Technology. 41 (4): 448–456. doi: 10.3327/jnst.41.448 . Archived (PDF) from the original on 2015-09-03.
43. Okundo, H. & Kawasaki, H. (2002). "Critical and Subcritical Mass Calculations of Curium-243 to −247 Based on JENDL-3.2 for Revision of ANSI/ANS-8.15". Journal of Nuclear Science and Technology. 39 (10): 1072–1085. doi: 10.3327/jnst.39.1072 .
44. § 2 Begriffsbestimmungen (Atomic Energy Act) (in German)
45. Jukka Lehto; Xiaolin Hou (2 February 2011). Chemistry and Analysis of Radionuclides: Laboratory Techniques and Methodology. Wiley-VCH. pp. 303–. ISBN   978-3-527-32658-7 . Retrieved 19 April 2011.
46. "Cosmochemists find evidence for unstable heavy element at solar system formation". phys.org. University of Chicago. 2016. Retrieved 6 June 2022.
47. Earth, Live Science Staff 2013-09-24T21:44:13Z Planet (24 September 2013). "Facts About Curium". livescience.com. Retrieved 2019-08-10.
48. "Curium - Element information, properties and uses | Periodic Table". www.rsc.org. Retrieved 2019-08-10.
49. Thornton, Brett F.; Burdette, Shawn C. (2019). "Neutron stardust and the elements of Earth". Nature Chemistry. 11 (1): 4–10. Bibcode:2019NatCh..11....4T. doi:10.1038/s41557-018-0190-9. PMID   30552435. S2CID   54632815 . Retrieved 19 February 2022.
50. Chaplin J, Warwick P, Cundy A, Bochud F, Froidevaux P (25 August 2021). "Novel DGT Configurations for the Assessment of Bioavailable Plutonium, Americium, and Uranium in Marine and Freshwater Environments". Analytical Chemistry. 93 (35): 11937–11945. doi: 10.1021/acs.analchem.1c01342 . PMID   34432435. S2CID   237307309.
51. Chaplin J, Christl M, Straub M, Bochud F, Froidevaux P (2 June 2022). "Passive Sampling Tool for Actinides in Spent Nuclear Fuel Pools". ACS Omega. 7 (23): 20053−20058. doi:10.1021/acsomega.2c01884. hdl:20.500.11850/554631. PMC   9202248 . PMID   35722008.
52. Curium (in German)
53. Fields, P. R.; Studier, M. H.; Diamond, H.; et al. (1956). "Transplutonium Elements in Thermonuclear Test Debris". Physical Review. 102 (1): 180–182. Bibcode:1956PhRv..102..180F. doi:10.1103/PhysRev.102.180.
54. Human Health Fact Sheet on Curium Archived 2006-02-18 at the Wayback Machine , Los Alamos National Laboratory
55. Emsley, John (2011). Nature's Building Blocks: An A-Z Guide to the Elements (New ed.). New York, NY: Oxford University Press. ISBN   978-0-19-960563-7.
56. Gopka, V. F.; Yushchenko, A. V.; Yushchenko, V. A.; Panov, I. V.; Kim, Ch. (15 May 2008). "Identification of absorption lines of short half-life actinides in the spectrum of Przybylski's star (HD 101065)". Kinematics and Physics of Celestial Bodies. 24 (2): 89–98. Bibcode:2008KPCB...24...89G. doi:10.3103/S0884591308020049. S2CID   120526363.
57. Basic elements of static RTGs Archived 2013-02-15 at the Wayback Machine , G.L. Kulcinski, NEEP 602 Course Notes (Spring 2000), Nuclear Power in Space, University of Wisconsin Fusion Technology Institute (see last page)
58. Lumetta, Gregg J.; Thompson, Major C.; Penneman, Robert A.; Eller, P. Gary (2006). "Curium" (PDF). In Morss; Edelstein, Norman M.; Fuger, Jean (eds.). The Chemistry of the Actinide and Transactinide Elements (3rd ed.). Dordrecht, The Netherlands: Springer Science+Business Media. p. 1401. ISBN   978-1-4020-3555-5. Archived from the original (PDF) on 2010-07-17.
59. Penneman, pp. 34–48
60. Magnusson D; Christiansen B; Foreman MRS; Geist A; Glatz JP; Malmbeck R; Modolo G; Serrano-Purroy D & Sorel C (2009). "Demonstration of a SANEX Process in Centrifugal Contactors using the CyMe4-BTBP Molecule on a Genuine Fuel Solution". Solvent Extraction and Ion Exchange. 27 (2): 97. doi:10.1080/07366290802672204. S2CID   94720457.
61. Penneman, p. 25
62. Cunningham, B. B.; Wallmann, J. C. (1964). "Crystal structure and melting point of curium metal". Journal of Inorganic and Nuclear Chemistry. 26 (2): 271. doi:10.1016/0022-1902(64)80069-5. OSTI   4667421.
63. Stevenson, J.; Peterson, J. (1979). "Preparation and structural studies of elemental curium-248 and the nitrides of curium-248 and berkelium-249". Journal of the Less Common Metals. 66 (2): 201. doi:10.1016/0022-5088(79)90229-7.
64. Gmelin Handbook of Inorganic Chemistry, System No. 71, Volume 7 a, transuranics, Part B 1, pp. 67–68.
65. Eubanks, I.; Thompson, M. C. (1969). "Preparation of curium metal". Inorganic and Nuclear Chemistry Letters. 5 (3): 187. doi:10.1016/0020-1650(69)80221-7.
66. Holleman, p. 1972
67. Greenwood, p. 1268
68. Noe, M.; Fuger, J. (1971). "Self-radiation effects on the lattice parameter of 244CmO2". Inorganic and Nuclear Chemistry Letters. 7 (5): 421. doi:10.1016/0020-1650(71)80177-0.
69. Haug, H. (1967). "Curium sesquioxide Cm2O3". Journal of Inorganic and Nuclear Chemistry. 29 (11): 2753. doi:10.1016/0022-1902(67)80014-9.
70. Fuger, J.; Haire, R.; Peterson, J. (1993). "Molar enthalpies of formation of BaCmO3 and BaCfO3". Journal of Alloys and Compounds. 200 (1–2): 181. doi:10.1016/0925-8388(93)90491-5.
71. Domanov, V. P. (January 2013). "Possibility of generation of octavalent curium in the gas phase in the form of volatile tetraoxide CmO₄". Radiochemistry. 55 (1): 46–51. doi:10.1134/S1066362213010098. S2CID   98076989.
72. Zaitsevskii, Andréi; Schwarz, W. H. Eugen (April 2014). "Structures and stability of AnO4 isomers, An = Pu, Am, and Cm: a relativistic density functional study". Physical Chemistry Chemical Physics. 2014 (16): 8997–9001. Bibcode:2014PCCP...16.8997Z. doi:10.1039/c4cp00235k. PMID   24695756.
73. Keenan, T. (1967). "Lattice constants of K7Cm6F31 trends in the 1:1 and 7:6 alkali metal-actinide(IV) series". Inorganic and Nuclear Chemistry Letters. 3 (10): 391. doi:10.1016/0020-1650(67)80092-8.
74. Asprey, L. B.; Keenan, T. K.; Kruse, F. H. (1965). "Crystal Structures of the Trifluorides, Trichlorides, Tribromides, and Triiodides of Americium and Curium". Inorganic Chemistry. 4 (7): 985. doi:10.1021/ic50029a013. S2CID   96551460.
75. Burns, J.; Peterson, J. R.; Stevenson, J. N. (1975). "Crystallographic studies of some transuranic trihalides: 239PuCl3, 244CmBr3, 249BkBr3 and 249CfBr3". Journal of Inorganic and Nuclear Chemistry. 37 (3): 743. doi:10.1016/0022-1902(75)80532-X.
76. Wallmann, J.; Fuger, J.; Peterson, J. R.; Green, J. L. (1967). "Crystal structure and lattice parameters of curium trichloride". Journal of Inorganic and Nuclear Chemistry. 29 (11): 2745. doi:10.1016/0022-1902(67)80013-7. S2CID   97334114.
77. Weigel, F.; Wishnevsky, V.; Hauske, H. (1977). "The vapor phase hydrolysis of PuCl3 and CmCl3: heats of formation of PuOC1 and CmOCl". Journal of the Less Common Metals. 56 (1): 113. doi:10.1016/0022-5088(77)90224-7.
78. Troc, R. Actinide Monochalcogenides, Volume 27, Springer, 2009 ISBN   3-540-29177-6, p. 4
79. Damien, D.; Charvillat, J. P.; Müller, W. (1975). "Preparation and lattice parameters of curium sulfides and selenides". Inorganic and Nuclear Chemistry Letters. 11 (7–8): 451. doi:10.1016/0020-1650(75)80017-1.
80. Lumetta, G. J.; Thompson, M. C.; Penneman, R. A.; Eller, P. G. Curium Archived 2010-07-17 at the Wayback Machine , Chapter Nine in Radioanalytical Chemistry, Springer, 2004, pp. 1420–1421. ISBN   0387341226, ISBN   978-0387 341224
81. Elschenbroich, Ch. Organometallic Chemistry, 6th edition, Wiesbaden 2008, ISBN   978-3-8351-0167-8, p. 589
82. Kerridge, Andrew; Kaltsoyannis, Nikolas (2009). "Are the Ground States of the Later Actinocenes Multiconfigurational? All-Electron Spin−Orbit Coupled CASPT2 Calculations on An(η8-C8H8)2(An = Th, U, Pu, Cm)". The Journal of Physical Chemistry A. 113 (30): 8737–8745. Bibcode:2009JPCA..113.8737K. doi:10.1021/jp903912q. PMID   19719318.
83. Girnt, Denise; Roesky, Peter W.; Geist, Andreas; Ruff, Christian M.; Panak, Petra J.; Denecke, Melissa A. (2010). "6-(3,5-Dimethyl-1H-pyrazol-1-yl)-2,2′-bipyridine as Ligand for Actinide(III)/Lanthanide(III) Separation". Inorganic Chemistry. 49 (20): 9627–9635. doi:10.1021/ic101309j. PMID   20849125. S2CID   978265.
84. Glorius, M.; Moll, H.; Bernhard, G. (2008). "Complexation of curium(III) with hydroxamic acids investigated by time-resolved laser-induced fluorescence spectroscopy". Polyhedron. 27 (9–10): 2113. doi:10.1016/j.poly.2008.04.002.
85. Heller, Anne; Barkleit, Astrid; Bernhard, Gert; Ackermann, Jörg-Uwe (2009). "Complexation study of europium(III) and curium(III) with urea in aqueous solution investigated by time-resolved laser-induced fluorescence spectroscopy". Inorganica Chimica Acta. 362 (4): 1215. doi:10.1016/j.ica.2008.06.016.
86. Moll, Henry; Johnsson, Anna; Schäfer, Mathias; Pedersen, Karsten; Budzikiewicz, Herbert; Bernhard, Gert (2007). "Curium(III) complexation with pyoverdins secreted by a groundwater strain of Pseudomonas fluorescens". BioMetals. 21 (2): 219–228. doi:10.1007/s10534-007-9111-x. PMID   17653625. S2CID   24565144.
87. Moll, Henry; Geipel, Gerhard; Bernhard, Gert (2005). "Complexation of curium(III) by adenosine 5′-triphosphate (ATP): A time-resolved laser-induced fluorescence spectroscopy (TRLFS) study". Inorganica Chimica Acta. 358 (7): 2275. doi:10.1016/j.ica.2004.12.055.
88. "Biochemical Periodic Table – Curium". UMBBD. 2007-06-08. Retrieved 2011-03-25.
89. Moll, H.; Stumpf, T.; Merroun, M.; Rossberg, A.; Selenska-Pobell, S.; Bernhard, G. (2004). "Time-resolved laser fluorescence spectroscopy study on the interaction of curium(III) with Desulfovibrio äspöensis DSM 10631T". Environmental Science & Technology. 38 (5): 1455–1459. Bibcode:2004EnST...38.1455M. doi:10.1021/es0301166. PMID   15046347.
90. Ozaki, T.; et al. (2002). "Association of Eu(III) and Cm(III) with Bacillus subtilis and Halobacterium salinarium". Journal of Nuclear Science and Technology. Suppl. 3: 950–953. Bibcode:2002JNST...39S.950O. doi:10.1080/00223131.2002.10875626. S2CID   98319565. Archived from the original on 2009-02-25.
91. Binder, Harry H.: Lexikon der chemischen Elemente, S. Hirzel Verlag, Stuttgart 1999, ISBN   3-7776-0736-3, pp. 174–178.
92. Gmelin Handbook of Inorganic Chemistry, System No. 71, Volume 7a, transuranics, Part A2, p. 289
93. Kronenberg, Andreas, Plutonium-Batterien Archived 2013-12-26 at the Wayback Machine (in German) "Archived copy". Archived from the original on February 21, 2011. Retrieved April 28, 2011.
94. Holleman, pp. 1980–1981.
95. Seaborg, Glenn T. (1996). Adloff, J. P. (ed.). One Hundred Years after the Discovery of Radioactivity. Oldenbourg Wissenschaftsverlag. p. 82. ISBN   978-3-486-64252-0.
96. "Der Rosetta Lander Philae". Bernd-leitenberger.de. 2003-07-01. Retrieved 2011-03-25.
97. Rieder, R.; Wanke, H.; Economou, T. (September 1996). "An Alpha Proton X-Ray Spectrometer for Mars-96 and Mars Pathfinder". Bulletin of the American Astronomical Society. 28: 1062. Bibcode:1996DPS....28.0221R.
98. Leitenberger, Bernd Die Surveyor Raumsonden (in German)
99. Nicks, Oran (1985). "Ch. 9. Essentials for Surveyor". SP-480 Far Travelers: The Exploring Machines. NASA.
100. Alpha Particle X-Ray Spectrometer (APXS), Cornell University
101. Hoffmann, K. Kann man Gold machen? Gauner, Gaukler und Gelehrte. Aus der Geschichte der chemischen Elemente (Can you make gold? Crooks, clowns and scholars. From the history of the chemical elements), Urania-Verlag, Leipzig, Jena, Berlin 1979, no ISBN, p. 233
102. Baetslé, L. H. Application of Partitioning/Transmutation of Radioactive Materials in Radioactive Waste Management Archived 2005-04-26 at the Wayback Machine , Nuclear Research Centre of Belgium Sck/Cen, Mol, Belgium, September 2001.

Bibliography

• Greenwood, Norman N.; Earnshaw, Alan (1997). Chemistry of the Elements (2nd ed.). Butterworth-Heinemann. ISBN   978-0-08-037941-8.
• Holleman, Arnold F. and Wiberg, Nils Lehrbuch der Anorganischen Chemie, 102 Edition, de Gruyter, Berlin 2007, ISBN   978-3-11-017770-1.
• Penneman, R. A. and Keenan T. K. The radiochemistry of americium and curium, University of California, Los Alamos, California, 1960

External links

• Curium at The Periodic Table of Videos (University of Nottingham)
• NLM Hazardous Substances Databank – Curium, Radioactive