Isotopes of hassium
Hassium (Hs) is an artificial element, and thus a standard atomic mass cannot be given. Like all artificial elements, it has no stable isotopes. The first isotope to be synthesized was 265Hs in 1984. There are 12 known isotopes from 263Hs to 277Hs and 1-4 isomers. The longest-lived isotope is 269Hs with a half-life of 9.6 seconds.
Contents
|
[edit] Table
| nuclide symbol |
Z(p) | N(n) | isotopic mass (u) |
half-life | decay mode(s)[n 1] |
daughter isotope(s) |
nuclear spin |
|---|---|---|---|---|---|---|---|
| excitation energy | |||||||
| 263Hs | 108 | 155 | 263.12856(37)# | 1# ms | α | 259Sg | 7/2+# |
| 264Hs | 108 | 156 | 264.12839(5) | 540(300) µs | α (50%) | 260Sg | 0+ |
| SF (50%) | (various) | ||||||
| 265Hs | 108 | 157 | 265.13009(15)# | 2.1(3) ms [2.0(+3-2) ms] |
α | 261Sg | 9/2+# |
| 265mHs | 300(70) keV | 0.780(0.15) ms [0.75(+17-12) ms] |
α | 261Sg | 3/2+# | ||
| 266Hs[n 2] | 108 | 158 | 266.13010(31)# | 2.7(10) ms [2.3(+13-6) ms] |
α | 262Sg | 0+ |
| 267Hs | 108 | 159 | 267.13179(11)# | 52(+13-8) s ms | α | 263Sg | 3/2+# |
| 267mHs[n 3] | α | 263Sg | |||||
| 268Hs | 108 | 160 | 268.13216(44)# | 2# s | α | 264Sg | 0+ |
| 269Hs[n 4] | 108 | 161 | 269.13406(13)# | 9.7(+99-33) s | α | 265Sg | |
| 269mHs[n 3] | α | 265Sg | |||||
| 270Hs | 108 | 162 | 270.13465(31)# | 3.6(+8-14) s | α | 266Sg | 0+ |
| 271Hs | 108 | 163 | 271.13766(36)# | 40# s | α | 267Sg | |
| 273Hs[n 5] | 108 | 165 | 273.14199(89)# | 240 ms | α | 269Sg | (3/2+)# |
| 275Hs[n 6] | 108 | 167 | 275.14595(77)# | 0.15(+27-6) s | α | 271Sg | |
| 277Hs[n 7] | 108 | 169 | 277.14984(78)# | SF | (various) | 3/2+# | |
| 277mHs[n 3][n 7] | 40(30) min | SF | (various) | ||||
- ^ Abbreviations:
SF: Spontaneous fission - ^ Not directly synthesized, occurs as decay product of 270Ds
- ^ a b c Existence of this isomer is unconfirmed
- ^ Not directly synthesized, occurs in decay chain of 277Cn
- ^ Not directly synthesized, occurs in decay chain of 285Uuq
- ^ Not directly synthesized, occurs in decay chain of 287Uuq
- ^ a b Not directly synthesized, occurs in decay chain of 289Uuq
[edit] Notes
- Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
- Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC which use expanded uncertainties.
[edit] Isotopes and nuclear properties
[edit] Nucleosynthesis
[edit] Cold fusion
This section deals with the synthesis of nuclei of hassium 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.
[edit] 136Xe(136Xe,xn)272−xHs
Important future experiments will involve the attempted synthesis of hassium isotopes in this symmetric reaction using the fission fragments. This reaction was carried out at Dubna in 2007 but no atoms were detected, leading to a cross section limit of 1 pb.[1] If confirmed, this would indicate that such symmetric fusion reactions should be modelled as 'hot fusion' reactions rather than 'cold fusion' ones, as first suggested. This would indicate that such reactions will unfortunately have limited use in the synthesis of superheavy elements.
[edit] 198Pt(70Zn,xn)268−xHs
This reaction was performed in May 2002 at the GSI. Unfortunately, the experiment was cut short due to a failure of the zinc-70 beam.
[edit] 208Pb(58Fe,xn)266−xHs (x=1,2)
This reaction was first reported in 1978 by the team at Dubna. In a later experiment in 1984, using the rotating drum technique, they were able to detect a spontaneous fission activity assigned to 260Sg, daughter of 264Hs. [2] In a repeat experiment in the same year, they applied the method of chemical identification of a descendant to provide support to the synthesis of element 108. They were able to detect several alpha decays of 253Es and 253Fm, descendants of 265Hs.
In the official discovery of the element in 1984, the team at GSI studied the reaction using the alpha decay genetic correlation method. They were able to positively identify 3 atoms of 265Hs.[3] After an upgrade of their facilities in 1993, the team repeated the experiment in 1994 and detected 75 atoms of 265Hs and 2 atoms of 264Hs, during the measurement of a partial excitation function for the 1n neutron evaporation channel.[4] The maximum of the 1n channel was measured as 69 pb in a further run in late 1997 in which a further 20 atoms were detected.[5]
The discovery experiment was successfully repeated in 2002 at RIKEN (10 atoms) and in 2003 at GANIL (7 atoms).
The team at RIKEN further studied the reaction in 2008 in order to conduct first spectroscopic studies of the even-even nucleus 264Hs. They were also able to detect a further 29 atoms of 265Hs.
[edit] 207Pb(58Fe,xn)265−xHs (x=1)
The use of a Pb-207 target was first used in 1984 at Dubna. They were able to detect the same SF activity as observed in the Pb-208 run and once again assigned it to260Sg, daughter of 264Hs.[6] The team at GSI first studied the reaction in 1986 using the method of correlation of genetic alpha decays and identified a single atom of 264Hs with a cross section of 3.2 pb.[7] The reaction was repeated in 1994 and the team were able to measure both alpha decay and spontaneous fission for 264Hs.
This reaction was studied in 2008 at RIKEN in order to conduct first spectrscopic studies of the even-even nucleus 264Hs. The team detected 11 atoms of the isotope.
[edit] 208Pb(56Fe,xn)264−xHs (x=1)
This reaction was studied for the first time in 2008 by the team at LBNL. They were able to produce and identify 6 atoms of the new isotope263Hs.[8] A few months later, the RIKEN team also published their results on the same reaction.[9]
[edit] 206Pb(58Fe,xn)264−xHs (x=1)
This reaction was studied for the first time in 2008 by the team at RIKEN. They were able to identify 8 atoms of the new isotope263Hs.[10]
[edit] 209Bi(55Mn,xn)264−xHs
First attempts to synthesise nuclei of hassium were performed using this reaction by the team at Dubna in 1983. Using the rotating drum technique, they were able to detect a spontaneous fission activity assigned to 255Rf, descendant of the 263Hs decay chain. Identical results were measured in a repeat run in 1984.[6] In a subsequent experiment in 1983, they applied the method of chemical identification of a descendant to provide support to the synthesis of hassium. They were able to detect alpha decays from fermium isotopes, assigned as descendants of the decay of 262Hs. This reaction has not been tried since and 262Hs is currently unconfirmed.[6]
[edit] Hot fusion
This section deals with the synthesis of nuclei of hassium 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.
[edit] 226Ra(48Ca,xn)274−xHs (x=4)
This reaction was reportedly first studied in 1978 by the team at the Flerov Laboratory of Nuclear Reactions (FLNR) under the leadership of Yuri Oganessian. However, results are not available in the literature.[6] The reaction was repeated at the FLNR in June 2008 and results show that the 4 atoms of the isotope 270Hs were detected with a yield of 9 pb. The decay data for the recently discovered isotope was confirmed, although the alpha energy was slightly higher.[11] In Jan 2009, the team repeated the experiment and a further 2 atoms of 270Hs were detected.[12]
[edit] 232Th(40Ar,xn)272−xHs
This reaction was first studied at Dubna in 1987. Detection was by spontaneous fission and no activities were found leading to a calculated cross section limit of 2 pb.[6]
[edit] 238U(36S,xn)274−xHs (x=4)
This reaction with the rare and expensive 36S isotope was conducted at the GSI in April–May 2008. Preliminary results show that a single atom of270Hs was detected with a yield of 0.8 pb. The data confirms the decay properties of 270Hs and266Sg.[13]
[edit] 238U(34S,xn)272−xHs (x=4,5)
In March 1994, the team at Dubna led by the late Yuri Lazerev announced the detection of 3 atoms of 267Hs from the 5n neutron evaporation channel. [14]The decay properties were confirmed by the team at GSI in their simultaneous study of darmstadtium.
The reaction was repeated at the GSI in Jan-Feb 2009 in order to search for the new isotope 268Hs. The team, led by Prof. Nishio, detected a single atom of both 268Hs and 267Hs. The new isotope underwent alpha-decay to the previously known isotope 264Sg.
[edit] 248Cm(26Mg,xn)274−xHs (x=3,4,5)
Most recently, a GSI-PSI collaboration has studied the nuclear reaction of curium-248 with magnesium-26 ions. Between May 2001 and August 2005, the team has studied the excitation function of the 3n, 4n, and 5n evaporation channels leading to 269Hs, 270Hs, and271Hs.[15][dead link][16][dead link] The synthesis of the important isotope270Hs was published in December 2006 by the team of scientists from the Technical University of Munich.[17] It was reported that this isotope decayed by emission of an alpha-particle with an energy of 8.83 MeV and a projected half-life of ~22 s, assuming a 0+ to 0+ ground state decay to 266Sg using the Viola-Seaborg equation.
[edit] 248Cm(25Mg,xn)273−xHs
This new reaction was studied at the GSI in July–August 2006 in a search for the new isotope 268Hs. They were unable to detect any atoms from neutron evaporation and calculated a cross section limit of 1 pb.
[edit] 249Cf(22Ne,xn)271−xHs
The team at Dubna studied this reaction in 1983 using detection by spontaneous fission (SF). Several short SF activities were found indicating the formation of nuclei of hassium. [6]
[edit] Chronology of isotope discovery
| Isotope | Year discovered | Discovery reaction |
|---|---|---|
| 263Hs | 2008 | 208Pb(56Fe,n) |
| 264Hs | 1986 | 207Pb(58Fe,n) |
| 265Hs | 1984 | 208Pb(58Fe,n) |
| 266Hs | 2000 | 207Pb(64Ni,n) [18] |
| 267Hs | 1995 | 238U(34S,5n) |
| 268Hs | 2009 | 238U(34S,4n) |
| 269Hs | 1996 | 208Pb(70Zn,n) [19] |
| 270Hs | 2004 | 248Cm(26Mg,4n) |
| 271Hs | 2004 | 248Cm(26Mg,3n)[citation needed] |
| 272Hs | unknown | |
| 273Hs | 2010 | 242Pu(48Ca,5n) |
| 274Hs | unknown | |
| 275Hs | 2003 | 242Pu(48Ca,3n) [20] |
| 276Hs | unknown | |
| 277aHs | 2009 | 244Pu(48Ca,3n) |
| 277bHs? | 1999 | 244Pu(48Ca,3n) [20] |
[edit] Unconfirmed isotopes
[edit] 277bHs
An isotope assigned to 277Hs has been observed on one occasion decaying by SF with a long half-life of ~11 minutes.[21] The isotope is not observed in the decay of the most common isotope of281Ds but is observed in the decay from a rare, as yet unconfirmed isomeric level, namely 281bDs . The half-life is very long for the ground state and it is possible that it belongs to an isomeric level in 277Hs. Furthermore, in 2009, the team at the GSI observed a small alpha decay branch for281aDs producing an isotope of 277Hs decaying by SF in a short lifetime. The measured half-life is close to the expected value for ground state isomer, 277aHs. Further research is required to confirm the production of the isomer.
[edit] Retracted isotopes
[edit] 273Hs
The claimed synthesis of element 118 by LBNL in 1999 involved the intermediate 273Hs. This isotope was claimed to decay by 9.78 and 9.47 MeV alpha emission with a half-life of 1.2 s. The claim to discovery of 293118 was retracted in 2001. This isotope was finally created in 2010 and the data confirmed the fabrication of previous data.
[edit] 270Hs: prospects for a deformed doubly magic nucleus
According to macroscopic-microscopic (MM) theory, Z=108 is a deformed proton magic number, in combination with the neutron shell at N=162. This means that such nuclei are permanently deformed in their ground state but have high, narrow fission barriers to further deformation and hence relatively long SF partial half-lives. The SF half-lives in this region are typically reduced by a factor of 109 in comparison with those in the vicinity of the spherical doubly magic nucleus298114, caused by an increase in the probability of barrier penetration by quantum tunnelling, due to the narrower fission barrier. In addition, N=162 has been calculated as a deformed neutron magic number and hence the nucleus 270Hs has promise as a deformed doubly magic nucleus. Experimental data from the decay of Z=110 isotopes 271Ds and 273Ds, provides strong evidence for the magic nature of the N=162 sub-shell. The recent synthesis of 269Hs, 270Hs, and 271Hs also fully support the assignment of N=162 as a magic closed shell. In particular, the low decay energy for 270Hs is in complete agreement with calculations.[22]
[edit] Evidence for the Z=108 deformed proton shell
Evidence for the magicity of the Z=108 proton shell can be deemed from two sources:
- the variation in the partial spontaneous fission half-lives for isotones
- the large gap in Qα for isotonic pairs between Z=108 and Z=110.
For SF, it is necessary to measure the half-lives for the isotonic nuclei 268Sg, 270Hs and 272Ds. Since the seaborgium anddarmstadtium isotopes are not known at this time, and fission of 270Hs has not been measured, this method can be used to date to confirm the stabilizing nature of the Z=108 shell. However, good evidence for the magicity of the Z=108 can be deemed from the large differences in the alpha decay energies measured for 270Hs,271Ds and 273Ds. More conclusive evidence would come from the determination of the decay energy for the nucleus 272Ds.
[edit] Nuclear isomerism
[edit] 269Hs
The direct synthesis of 269Hs has resulted in three alpha lines at 9.21, 9.10, and 8.94 MeV. In the decay of 277112, only 9.21 MeV269Hs alpha decays have been observed indicating that this decay occurs from an isomeric level. Further research is required to confirm this.
[edit] 267Hs
The decay of 267Hs is known to occur by alpha decay with three alpha lines at 9.88, 9.83, and 9.75 MeV and a half-life of 52 ms. In the recent syntheses of271m,gDs additional activities have been observed. A .94ms activity decaying by 9.83 MeV alpha emission has been observed in addition to longer lived ~.8 s and ~6.0 s activities. Each of these is currently not assigned and confirmed and further research is required to positively identify them.
[edit] 265Hs
The synthesis of 265Hs has also provided evidence for two levels. The ground state decays by 10.30 MeV alpha emission with a half-life of 2.0 ms. The isomeric state is placed at 300 keV above the ground state and decays by 10.57 MeV alpha emission with a half-life of .75 ms.
[edit] Physical production yields
The tables below provides cross-sections and excitation energies for nuclear reactions that produce isotopes of hassium directly. Data in bold represent maxima derived from excitation function measurements. + represents an observed exit channel.
[edit] Cold fusion
| Projectile | Target | CN | 1n | 2n | 3n |
|---|---|---|---|---|---|
| 58Fe | 208Pb | 266Hs | 69 pb, 13.9 MeV | 4.5 pb | |
| 58Fe | 207Pb | 265Hs | 3.2 pb |
[edit] Hot fusion
| Projectile | Target | CN | 3n | 4n | 5n |
|---|---|---|---|---|---|
| 48Ca | 226Ra | 274Hs | 9.0 pb | ||
| 36S | 238U | 274Hs | 0.8 pb | ||
| 34S | 238U | 272Hs | 2.5 pb, 50.0 MeV | ||
| 26Mg | 248Cm | 274Hs | 2.5 pb | 3.0 pb | 7.0 pb |
[edit] Theoretical calculations
[edit] Evaporation residue cross sections
The below table contains various targets-projectile combinations for which calculations have provided estimates for cross section yields from various neutron evaporation channels. The channel with the highest expected yield is given.
DNS = Di-nuclear system ; σ = cross section
| Target | Projectile | CN | Channel (product) | σ max | Model | Ref |
|---|---|---|---|---|---|---|
| 136Xe | 136Xe | 272Hs | 1-4n (271-268Hs) | 10−6 pb | DNS | [23] |
| 238U | 34S | 272Hs | 4n (268Hs) | 10 pb | DNS | [23] |
[edit] References
- ^ Flerov Lab
- ^ Oganessian, Yu Ts; Demin, A. G.; Hussonnois, M.; Tretyakova, S. P.; Kharitonov, Yu P.; Utyonkov, V. K.; Shirokovsky, I. V.; Constantinescu, O. et al (1984). "On the stability of the nuclei of element 108 withA=263–265". Zeitschrift für Physik A 319 (2): 215. Bibcode 1984ZPhyA.319..215O. doi:10.1007/BF01415635.
- ^ Münzenberg, G.; Armbruster, P.; Folger, H.; He�berger, P. F.; Hofmann, S.; Keller, J.; Poppensieker, K.; Reisdorf, W. et al (1984). "The identification of element 108". Zeitschrift für Physik A 317 (2): 235. Bibcode 1984ZPhyA.317..235M. doi:10.1007/BF01421260.
- ^ Hofmann, S (1998). "New elements - approaching". Reports on Progress in Physics 61 (6): 639. Bibcode 1998RPPh...61..639H. doi:10.1088/0034-4885/61/6/002.
- ^ Hofmann, S.; Heßberger, F.P.; Ninov, V.; Armbruster, P.; Münzenberg, G.; Stodel, C.; Popeko, A.G.; Yeremin, A.V. et al (1997). "Excitation function for the production of 265 108 and 266 109". Zeitschrift für Physik A 358 (4): 377. Bibcode 1997ZPhyA.358..377H. doi:10.1007/s002180050343.
- ^ Cite error: Invalid
<ref>tag; no text was provided for refs named93TWG; see Help:Cite errors/Cite error references no text - ^ Münzenberg, G.; Armbruster, P.; Berthes, G.; Folger, H.; He�erger, F. P.; Hofmann, S.; Poppensieker, K.; Reisdorf, W. et al (1986). "Evidence for264108, the heaviest known even-even isotope". Zeitschrift für Physik A 324 (4): 489. Bibcode 1986ZPhyA.324..489M. doi:10.1007/BF01290935.
- ^ Dragojević, I.; Gregorich, K.; Düllmann, Ch.; Dvorak, J.; Ellison, P.; Gates, J.; Nelson, S.; Stavsetra, L. et al (2009). "New Isotope 263108". Physical Review C 79: 011602. Bibcode 2009PhRvC..79a1602D. doi:10.1103/PhysRevC.79.011602.
- ^ Kaji, Daiya; Morimoto, Kouji; Sato, Nozomi; Ichikawa, Takatoshi; Ideguchi, Eiji; Ozeki, Kazutaka; Haba, Hiromitsu; Koura, Hiroyuki et al (2009). "Production and Decay Properties of 263108". Journal of the Physical Society of Japan 78 (3): 035003. Bibcode 2009JPSJ...78c5003K. doi:10.1143/JPSJ.78.035003.
- ^ Mendeleev Symposium. Morita
- ^ Flerov Lab.
- ^ Results of 226Ra+48Ca Experiment, Yu. Tsyganov et al., April 7, 2009
- ^ Observation of 270Hs in the complete fusion reaction 36S+238U* R. Graeger et al., GSI Report 2008
- ^ Lazarev, Yu. A.; Lobanov, YV; Oganessian, YT; Tsyganov, YS; Utyonkov, VK; Abdullin, FS; Iliev, S; Polyakov, AN et al (1995). "New Nuclide 267108 Produced by the 238U + 34S Reaction". Physical Review Letters 75 (10): 1903. Bibcode 1995PhRvL..75.1903L. doi:10.1103/PhysRevLett.75.1903. PMID 10059158.
- ^ "Decay properties of 269Hs and evidence for the new nuclide 270Hs", Turler et al., GSI Annual Report 2001. Retrieved on 2008-03-01
- ^ 269-271Hs
- ^ "Doubly magic 270Hs", Turler et al., GSI report, 2006. Retrieved on 2008-03-01
- ^ see darmstadtium
- ^ see copernicium
- ^ a b see ununquadium
- ^ http://www.springerlink.com/content/f80mt423204570p8/fulltext.pdf
- ^ Robert Smolanczuk (1997). "Properties of the hypothetical spherical superheavy nuclei". Physical Review C 56 (2): 812–824. Bibcode 1997PhRvC..56..812S. doi:10.1103/PhysRevC.56.812.
- ^ a b of entrance channels on formation of superheavy nuclei in massive fusion reactions, Zhao-Qing Feng, Jun-Qing Li, Gen-Ming Jin, April 2009
- National Nuclear Data Center, Brookhaven National Laboratory
- Isotope masses from:
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties". Nuclear Physics A 729: 3–128. Bibcode 2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001. http://www.nndc.bnl.gov/amdc/nubase/Nubase2003.pdf.
- Isotopic compositions and standard atomic masses from:
- J. R. de Laeter, J. K. Böhlke, P. De Bièvre, H. Hidaka, H. S. Peiser, K. J. R. Rosman and P. D. P. Taylor (2003). "Atomic weights of the elements. Review 2000 (IUPAC Technical Report)". Pure and Applied Chemistry 75 (6): 683–800. doi:10.1351/pac200375060683. http://www.iupac.org/publications/pac/75/6/0683/pdf/.
- M. E. Wieser (2006). "Atomic weights of the elements 2005 (IUPAC Technical Report)". Pure and Applied Chemistry 78 (11): 2051–2066. doi:10.1351/pac200678112051. http://iupac.org/publications/pac/78/11/2051/pdf/. Lay summary.
- Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
- G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties". Nuclear Physics A 729: 3–128. Bibcode 2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001. http://www.nndc.bnl.gov/amdc/nubase/Nubase2003.pdf.
- National Nuclear Data Center. "NuDat 2.1 database". Brookhaven National Laboratory. http://www.nndc.bnl.gov/nudat2/. Retrieved September 2005.
- N. E. Holden (2004). "Table of the Isotopes". In D. R. Lide. CRC Handbook of Chemistry and Physics (85th ed.). CRC Press. Section 11. ISBN 978-0849304859.
| Isotopes of bohrium | Isotopes of hassium | Isotopes of meitnerium |
| Index to isotope pages · Table of nuclides | ||