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Dubnium (pronounced /ˈduːbniəm/, DOOB-nee-əm) is a chemical element with the symbol Db and atomic number 105.

This is a radioactive synthetic element whose most stable isotope is 268Db with a half life of 28 hours.[1] This is the longest lived transactinide isotope and is a reflection of the stability of the Z = 108 and N = 162 closed shells and the effect of odd particles in nuclear decay. Chemistry experiments have provided sufficient evidence to confidently place dubnium in group 5 of the Periodic Table.

Discovery profile

Element 105 was first reported by Russian scientists, in 1968-1970 at the Joint Institute for Nuclear Research in Dubna, Russia. The 1968 work was based on the detection of correlated decays of element 105 to known daughter nuclei using the reaction 243Am(22Ne,xn). They reported a 9.40 MeV and a 9.70 MeV alpha-activity and assigned the decays to the isotopes 260105 or 261105.

In 1970 they expanded their work by the application of thermal gradient chromatography and detection by spontaneous fission. They observed a 2.2 s SF activity in a fraction portraying niobium-like characteristics and assigned the activity to 261DbCl5.

In late April 1970 researchers led by Albert Ghiorso working at the University of California, Berkeley published a convincing synthesis of 260Db in the reaction:

24998Cf + 157N → 260105Db + 4 n

The team claimed that 260Db decayed by 9.10 MeV alpha-emission with a half-life of 1.6 seconds to 256Lr. Decay data for 256Lr agreed with the literature values and provided strong support to their claim.

These results by the Berkeley scientists did not confirm the Soviet findings regarding the 9.40 MeV or 9.70 MeV alpha-decay of 260Db.

In 1971, the Russian team repeated their reaction using an improved set-up and were able to confirm the decay data for 260Db using the reaction:

243Am + 22Ne → 260Db + 5 n

In 1976, the Russian team continued their study of the reaction using thermal gradient chromatography and were able to identify the product 260DbBr5.

In 1977, all doubt was dispelled by the L X-ray elemental detection of lawrencium isotopes from the reaction:

249Cf + 15N → 260Db + 4 n

In 1992 the TWG assessed the claims of the two groups and concluded that confidence in the discovery grew from results from both laboratories and the claim of discovery should be shared.[2]
Proposed names

Historically element 105 has been called eka-tantalum, reflecting Mendeleev's placeholder terminology.[citation needed]

The American team proposed that the new element should be named hahnium (Ha), in honor of the late German physicist Otto Hahn. Consequently this was the name that most American and Western European scientists used and appears in many papers published at the time.

The Russian team proposed the name nielsbohrium (Ns) in honor of the Danish nuclear physicist Niels Bohr.

An element naming controversy erupted between the two groups. The International Union of Pure and Applied Chemistry (IUPAC) thus adopted unnilpentium (Unp) as a temporary, systematic element name. Attempting to resolve the issue, in 1994, the IUPAC proposed the name joliotium (Jl), after the French physicist Frédéric Joliot-Curie. The two principal claimants still disagreed about the names of elements 104-106. However in 1997 they resolved the dispute and adopted the current name, dubnium (Db), after the Russian town of Dubna, the location of the Joint Institute for Nuclear Research. It was argued by IUPAC that the Berkeley laboratory had already been recognized several times in the naming of elements (i.e., berkelium, californium, americium) and that the acceptance of the names rutherfordium and seaborgium for elements 104 and 106 should be offset by recognizing the Russian team's contributions to the discovery of elements 104, 105 and 106.[3][4]
Electronic structure

Dubnium is element 105 in the Periodic Table. The two forms of the projected electronic structure are:
Bohr model 2, 8, 18, 32, 32, 11, 2
Quantum mechanical model 1s22s22p63s23p64s23d104p65s24d105p66s24f145d106p67s25f146d3
Extrapolated chemical properties of eka-tantalum/dvi-niobium
Oxidation states

Element 105 is projected to be the second member of the 6d series of transition metals and the heaviest member of group V in the Periodic Table, below vanadium, niobium and tantalum. All the members of the group readily portray their oxidation state of +5 and the state becomes more stable as the group is descended. Thus dubnium is expected to form a stable +5 state. For this group, +4 and +3 states are also known for the heavier members and dubnium may also form these reducing oxidation states.

In an extrapolation of the chemistries from niobium and tantalum, dubnium should react with oxygen to form an inert pentoxide, Db2O5. In alkali, the formation of an orthodubnate complex, DbO43−, is expected. Reaction with the halogens should readily form the pentahalides, DbX5. The pentachlorides of niobium and tantalum exist as volatile solids or monomeric trigonal bipyramidal molecules in the vapour phase. Thus, DbCl5 is expected to be a volatile solid. Similarly, the pentafluoride, DbF5, should be even more volatile. Hydrolysis of the halides is known to readily form the oxyhalides, MOX3. Thus the halides DbX5 should react with water to form DbOX3. The reaction with fluoride ion is also well known for the lighter homologues and dubnium is expected to form a range of fluoro-complexes. In particular, reaction of the pentafluoride with HF should form a hexafluorodubnate ion, DbF6–. Excess fluoride should lead to DbF72– and DbOF52–. If eka-tantalum properties are portrayed, higher concentrations of fluoride should ultimately form DbF83– since NbF83– is not known.
Experimental chemistry
Gas phase chemistry

The chemistry of dubnium has been studied for several years using gas thermochromatography. The experiments have studied the relative adsorption characteristics of isotopes of niobium, tantalum and dubnium radioisotopes. The results have indicated the formation of typical group 5 halides and oxyhalides, namely DbCl5, DbBr5, DbOCl3 and DbOBr3. Reports on these early experiments usually refer to dubnium as hahnium.
Summary of compounds and complex ions
Formula Names(s)
DbCl5 dubnium pentachloride ; dubnium(V) chloride
DbBr5 dubnium pentabromide ; dubnium(V) bromide
DbOCl3 dubnium oxychloride ; dubnium(V) trichloride oxide ; dubnyl(V) chloride
DbOBr3 dubnium oxybromide ; dubnium(V) tribromide oxide ; dubnyl(V) bromide
History of synthesis of isotopes by cold fusion

This section deals with the synthesis of nuclei of dubnium by so-called "cold" fusion reactions. These are processes which create compound nuclei at low excitation energy (~10-20 MeV, hence "cold"), leading to a higher probability of survival from fission. The excited nucleus then decays to the ground state via the emission of one or two neutrons only.
209Bi(50Ti,xn)259-xDb (x=1,2,3)

The first attempts to synthesise element 105 using cold fusion reactions were performed in 1976 by the team at FLNR, Dubna using the above reaction. They were able to detect a 5 s spontaneous fission (SF) activity which they assigned to 257105. This assignment was later corrected to 258105. In 1981, the team at GSI studied this reaction using the improved technique of correlation of genetic parent-daughter decays. They were able to positively identify 258Db, the product from the 1n neutron evaporation channel.[5] In 1983, the team at Dubna revisited the reaction using the method of identification of a descendant using chemical separation. They succeeded in measuring alpha decays from known descendants of the decay chain beginning with 258105. This was taken as providing some evidence for the formation of element 105 nuclei. The team at GSI revisited the reaction in 1985 and were able to detect 10 atoms of 257Db.[6] After a significant upgrade of their facilities in 1993, in 2000 the team measured 120 decays of 257Db, 16 decays of 256Db and decay of 258Db in the measurement of the 1n, 2n and 3n excitation functions. The data gathered for 257Db allowed a first spectroscopic study of this isotope and identified an isomer, 257mDb, and a first determination of a decay level structure for 257Db.[7] The reaction was used in spectroscopic studies of isotopes of mendelevium and einsteinium in 2003-2004.[8]
209Bi(49Ti,xn)258-xDb (x=2?)

This reaction was studied by Yuri Oganessian and the team at Dubna in 1983. They observed a 2.6 s SF activity tentatively assigned to 256Db. Later results suggest a possible reassignment to 256Rf, resulting from the ~30% EC branch in 256Db.
209Bi(48Ti,xn)257-xDb (x=1?)

This reaction was studied by Yuri Oganessian and the team at Dubna in 1983. They observed a 1.6 s activity with a ~80% alpha branch with a ~20% SF branch. The activity was tentatively assigned to 255Db. Later results suggest a reassignment to 256Db.
208Pb(51V,xn)259-xDb (x=1,2)

The team at Dubna also studied this reaction in 1976 and were again able to detect the 5 s SF activity, first tentatively assigned to 257Db and later to 258Db. In 2006, the team at LBNL reinvestigated this reaction as part of their odd-Z projectile program. They were able to detect 258Db and 257Db in their measurement of the 1n and 2n neutron evaporation channels. [9]

The team at Dubna also studied this reaction in 1976 but this time they were unable to detect the 5 s SF activity, first tentatively assigned to 257Db and later to 258Db. Instead, they were able to measure a 1.5 s SF activity, tentatively assigned to 255Db.
205Tl(54Cr,xn)259-xDb (x=1?)

The team at Dubna also studied this reaction in 1976 and were again able to detect the 5 s SF activity, first tentatively assigned to 257Db and later to 258Db.
History of synthesis of isotopes by hot fusion

This section deals with the synthesis of nuclei of dubnium by so-called "hot" fusion reactions. These are processes which create compound nuclei at high excitation energy (~40-50 MeV, hence "hot"), leading to a reduced probability of survival from fission and quasi-fission. The excited nucleus then decays to the ground state via the emission of 3-5 neutrons.
232Th(31P,xn)263-xDb (x=5)

There are very limited reports that this rare reaction using a P-31 beam was studied in 1989 by Andreyev et al. at the FLNR. One source suggests that no atoms were detected whilst a better source from the Russians themselves indicates that 258Db was synthesised in the 5n channel with a yield of 120 pb.
238U(27Al,xn)265-xDb (x=4,5)

In 2006, as part of their study of the use of uranium targets in superheavy element synthesis, the LBNL team led by Ken Gregorich studied the excitation functions for the 4n and 5n channels in this new reaction.[10]
236U(27Al,xn)263-xDb (x=5,6)

This reaction was first studied by Andreyev et al. at the FLNR, Dubna in 1992. They were able to observe 258Db and 257Db in the 5n and 6n exit channels with yields of 450 pb and 75 pb, respectively.[11]
243Am(22Ne,xn)265-xDb (x=5)

The first attempts to synthesis element 105 were performed in 1968 by the team at the Flerov Laboratory of Nuclear Reactions (FLNR) in Dubna,Russia. They observed two alpha lines which they tentatively assigned to 261105 and 260105. They repeated their experiment in 1970 looking for spontaneous fission. They found a 2.2 s SF activity which they assigned to 261105. In 1970, the Dubna team began work on using gradient thermochromatography in order to detect element 105 in chemical experiments as a volatile chloride. In their first run they detected a volatile SF activity with similar adsorption properties to NbCl5 and unlike HfCl4. This was taken to indicate the formation of nuclei of dvi-niobium as [105]Cl5. In 1971, they repeated the chemistry experiment using higher sensitivity and observed alpha decays from an dvi-niobium component, taken to confirm the formation of 260105. The method was repeated in 1976 using the formation of bromides and obtained almost identical results, indicating the formation of a volatile, dvi-niobium-like [105]Br5.
241Am(22Ne,xn)263-xDb (x=4,5)

In 2000, Chinese scientists at the Institute of Modern Physics (IMP), Lanzhou, announced the discovery of the previously unknown isotope 259Db formed in the 4n neutron evaporation channel. They were also able to confirm the decay properties for 258Db.[12]
248Cm(19F,xn)267-xDb (x=4,5)

This reaction was first studied in 1999 at the Paul Scherrer Institute (PSI) in order to produce 262Db for chemical studies. Just 4 atoms were detected with a cross section of 260 pb.[13] Japanese scientists at JAERI studied the reaction further in 2002 and determined yields for the isotope 262Db during their efforts to study the aqueous chemistry of dubnium.[14]
249Bk(18O,xn)267-xDb (x=4,5)

Following from the discovery of 260Db by Albert Ghiorso in 1970 at the University of California (UC), the same team continued in 1971 with the discovery of the new isotope 262Db. They also observed an unassigned 25 s SF activity, probably associated with the now-known SF branch of 263Db.[15] In 1990, a team led by Kratz at LBNL definitively discovered the new isotope 263Db in the 4n neutron evaporation channel.[16] This reaction has been used by the same team on several occasions in order to attempt to confirm an electron capture (EC) branch in 263Db leading to long-lived 263Rf (see rutherfordium).[17]
249Bk(16O,xn)265-xDb (x=4)

Following from the discovery of 260Db by Albert Ghiorso in 1970 at the University of California (UC), the same team continued in 1971 with the discovery of the new isotope 261Db.[15]
250Cf(15N,xn)265-xDb (x=4)

Following from the discovery of 260Db by Ghiorso in 1970 at LBNL, the same team continued in 1971 with the discovery of the new isotope 261Db.[15]
249Cf(15N,xn)264-xDb (x=4)

In 1970, the team at the Lawrence Berkeley National Laboratory (LBNL) studied this reaction and identified the isotope 260105 in their discovery experiment. They used the modern technique of correlation of genetic parent-daughter decays to confirm their assignment.[18] In 1977, the team at Oak Ridge repeated the experiment and were able to confirm the discovery by the identification of K X-rays from the daughter lawrencium.[19]

In 1988, scientists as the Lawrence Livermore National Laboratory (LLNL) used the asymmetric hot fusion reaction with an einsteinium-254 target to search for the new nuclides 264Db and 263Db. Due to the low sensitivity of the experiment caused by the small Es-254 target,they were unable to detect any evaporation residues (ER).
Synthesis of isotopes as decay products

Isotopes of dubnium have also been identified in the decay of heavier elements. Observations to date are summarised in the table below:
Evaporation Residue Observed Db isotope
294117 270Db
288115 268Db
287115 267Db
282113 266Db
267Bh 263Db
278113 , 266Bh 262Db
265Bh 261Db
272Rg 260Db
266Mt , 262Bh 258Db
261Bh 257Db
260Bh 256Db
Chronology of isotope discovery
Isotope Year discovered discovery reaction
256Db 1983? , 2000 209Bi(50Ti,3n)
257Dbg 1985 209Bi(50Ti,2n)
257Dbm 2000 209Bi(50Ti,2n)
258Db 1976? , 1981 209Bi(50Ti,n)
259Db 2001 241Am(22Ne,4n)
260Db 1970 249Cf(15N,4n)
261Db 1971 249Bk(16O,4n)
262Db 1971 249Bk(18O,5n)
263Db 1971? , 1990 249Bk(18O,4n)
264Db unknown
265Db unknown
266Db 2006 237Np(48Ca,3n)
267Db 2003 243Am(48CaCa,4n)
268Db 2003 243Am(48Ca,3n)
269Db unknown
270Db 2009 249Bk(48Ca,3n)
Isomerism in dubnium nuclides

Recent data on the decay of 272Rg has revealed that some decay chains continue through 260Db with extraordinary longer life-times than expected. These decays have been linked to an isomeric level decaying by alpha decay with a half-life of ~19 s. Further research is required to allow a definite assignment.

Evidence for an isomeric state in 258Db has been gathered from the study of the decay of 266Mt and 262Bh. It has been noted that those decays assigned to an electron capture (EC) branch has a significantly different half-life to those decaying by alpha emission. This has been taken to suggest the existence of an isomeric state decaying by EC with a half-life of ~20 s. Further experiments are required to confirm this assignment.

A study of the formation and decay of 257Db has proved the existence of an isomeric state. Initially, 257Db was taken to decay by alpha emission with energies 9.16,9.07 and 8.97 MeV. A measurement of the correlations of these decays with those of 253Lr have shown that the 9.16 MeV decay belongs to a separate isomer. Analysis of the data in conjunction with theory have assigned this activity to a meta stable state, 257mDb. The ground state decays by alpha emission with energies 9.07 and 8.97 MeV. Spontaneous fission of 257m,gDb was not confirmed in recent experiments.
Spectroscopic decay level schemes for dubnium isotopes
This is the currently suggested decay level scheme for 257Dbg,m from the study performed in 2001 by Hessberger et al. at GSI
Retracted isotopes

In 1983, scientists at Dubna carried out a series of supportive experiments in their quest for the discovery of element 107. In two such experiments, they claimed they had detected a ~1.5 s spontaneous fission activity from the reactions 207Pb(51V,xn) and 209Bi(48Ti,xn). The activity was assigned to 255Db. Later research suggested that the assignment should be changed to 256Db. As such, the isotope 255Db is currently not recognised on the chart of radionuclides and further research is required to confirm this isotope.
Chemical yields of isotopes
Cold fusion

The table below provides cross-sections and excitation energies for cold fusion reactions producing dubnium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
Projectile Target CN 1n 2n 3n
51V 208Pb 259Db 1.54 nb , 15.6 MeV 1.8 nb , 23.7 MeV
50Ti 209Bi 259Db 4.64 nb , 16.4 MeV 2.4 nb , 22.3 MeV 200 pb , 31.0 MeV
Hot fusion

The table below provides cross-sections and excitation energies for hot fusion reactions producing dubnium isotopes directly. Data in bold represents maxima derived from excitation function measurements. + represents an observed exit channel.
Projectile Target CN 3n 4n 5n
27Al 238U 265Db + +
22Ne 241Am 263Db 1.6 nb 3.6 nb
22Ne 243Am 265Db + +
19F 248Cm 267Db 1.0 nb
18O 249Bk 267Db 10.0 nb 6.0 nb

1. ^ Physical experiments determined a half-life of ~16 h whilst chemical experiments provided a value of ~32 h. The half-life is often taken as ~28 h due to the higher number of atoms detected by chemical means
2. ^ Barber, R. C.; Greenwood, N. N.; Hrynkiewicz, A. Z.; Jeannin, Y. P.; Lefort, M.; Sakai, M.; Ulehla, I.; Wapstra, A. P. et al. (1993). "Discovery of the transfermium elements. Part II: Introduction to discovery profiles. Part III: Discovery profiles of the transfermium elements (Note: for Part I see Pure Appl. Chem., Vol. 63, No. 6, pp. 879-886, 1991)". Pure and Applied Chemistry 65: 1757. doi:10.1351/pac199365081757.
3. ^ "Names and symbols of transfermium elements (IUPAC Recommendations 1994)". Pure and Applied Chemistry 66: 2419. 1994. doi:10.1351/pac199466122419.
4. ^ "Names and symbols of transfermium elements (IUPAC Recommendations 1997)". Pure and Applied Chemistry 69: 2471. 1997. doi:10.1351/pac199769122471.
5. ^ Munzenberg; Hofmann, S.; He�berger, F. P.; Reisdorf, W.; Schmidt, K. H.; Schneider, J. H. R.; Armbruster, P.; Sahm, C. C. et al. (1981). "Identification of element 107 by α correlation chains". Z. Phys. A. 300: 1. doi:10.1007/BF01412623.
6. ^ Hessberger; M�nzenberg, G.; Hofmann, S.; Agarwal, Y. K.; Poppensieker, K.; Reisdorf, W.; Schmidt, K. -H.; Schneider, J. R. H. et al. (1985). "The new isotopes 258105,257105,254Lr and 253Lr"". Z. Phys A. 322: 4. doi:10.1007/BF01415134.
7. ^ F. P. Hessberger; Hofmann, S.; Ackermann, D.; Ninov, V.; Leino, M.; Münzenberg, G.; Saro, S.; Lavrentev, A. et al. (2001). "Decay properties of neutron-deficient isotopes 256,257Db, 255Rf, 252,253Lr". Eur. Phys. J. A 12: 57–67. doi:10.1007/s100500170039. http://www.edpsciences.org/articles/epja/abs/2001/09/epja1103/epja1103.html.
8. ^ F. P. Hessberger (2005). Eur. Phys. J. A 26: 2. doi:Energy+systematics+of+low-lying+Nilsson+levels+in+odd-mass+einsteinium+isotopes (inactive 2009-11-14). http://www.springerlink.com/content/7n66l7650112m776/.
9. ^ Gates (2005). "Measurement of the 208Pb(51V, xn)259-xDb Excitation Function". LBNL Annual Report. http://rnc.lbl.gov/nsd/annualreport2005/contributions/Gates1_LE.pdf.
10. ^ "238U studies". http://rnc.lbl.gov/nsd/annualreport2005/contributions/Gregorich_LE.pdf. Retrieved 2009-05-05.
11. ^ A. N. Andreyev; Bogdanov, D. D.; Chepigin, V. I.; Kabachenko, A. P.; Malyshev, O. N.; Oganessian, Yu. Ts.; Sagajdak, R. N.; Ter-Akopian, G. M. et al. (1992). "Investigation of the fusion reaction 27Al + 236U → 263105 at excitation energies of 57 MeV and 65 MeV". Z. Phys. A. 344: 2. doi:10.1007/BF01291709.
12. ^ Z. G. Gan; Qin, Z.; Fan, H.M.; Lei, X.G.; Xu, Y.B.; He, J.J.; Liu, H.Y.; Wu, X.L. et al. (2001). "A new alpha-particle-emitting isotope 259Db". Eur. Phys. J. A 10: 1. doi:10.1007/s100500170140.
13. ^ R. Dressler; Eichler, B.; Jost, D. T.; Piguet, D.; Türler, A.; Schädel, M.; Taut, S.; Yakushev, A. B. (1999). "Production of 262Db (Z=105) in the reaction 248Cm(19F,  5n)". Phys. Rev. C 59: 3433–3436. doi:10.1103/PhysRevC.59.3433.
14. ^ Y. Nagame (2002). "Production Cross Sections of 261Rf and 262Db in Bombardments of 248Cm with 18O and 19F Ions". J. Nucl. Radiochem. Sci 3: 85–88. http://sciencelinks.jp/j-east/article/200219/000020021902A0652005.php.
15. ^ a b c A. Ghiorso; Nurmia, Matti; Eskola, Kari; Eskola, Pirkko (1971). "Two New Alpha-Particle Emitting Isotopes of Element 105, 261Ha and 262Ha". Phys. Rev. C 4: 1850–1855. doi:10.1103/PhysRevC.4.1850.
16. ^ J. V. Kratz; Gober, M. K.; Zimmermann, H. P.; Gregorich, K. E.; Türler, A.; Hannink, N. J.; Czerwinski, K. R.; Kadkhodayan, B. et al. (1992). "New nuclide 263Ha". Phys. Rev. C 45: 1064–1069. doi:10.1103/PhysRevC.45.1064.
17. ^ "EC of 263Db". http://www.ulrich-rieth.de/publikationen/RCA0301_059.PDF. Retrieved 2009-05-05.
18. ^ A. Ghiorso; Nurmia, Matti; Eskola, Kari; Harris, James; Eskola, Pirkko (1970). "New Element Hahnium, Atomic Number 105". Phys. Rev. Lett. 24: 1498–1503. doi:10.1103/PhysRevLett.24.1498.
19. ^ C. E. Bemis; Dittner, P. F.; Silva, R. J.; Hahn, R. L.; Tarrant, J. R.; Hunt, L. D.; Hensley, D. C. (1977). "Production, L x-ray identification, and decay of the nuclide 260105". Phys. Rev. C 16: 1146–1158. doi:10.1103/PhysRevC.16.1146.

External links

* WebElements.com - Dubnium

Periodic table
H   He
Li Be   B C N O F Ne
Na Mg   Al Si P S Cl Ar
K Ca Sc   Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr
Rb Sr Y   Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe
Cs Ba La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn
Fr Ra Ac Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr Rf Db Sg Bh Hs Mt Ds Rg Cn Uut Uuq Uup Uuh Uus Uuo
Alkali metals Alkaline earth metals Lanthanoids Actinoids Transition metals Other metals Metalloids Other nonmetals Halogens Noble gases

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