Реклама

      The Synthesis of Superheavy Nuclei in the 48Ca + 244Pu Reaction: 288114

      Yu.Ts. Oganessian, V.K. Utyonkov, Yu.V. Lobanov, F.Sh. Abdullin, A.N. Polyakov, I.V. Shirokovsky, Yu.S. Tsyganov, G.G. Gulbekian, S.L. Bogomolov, B.N. Gikal, A.N. Mezentsev, S. Iliev, V.G. Subbotin, A.M. Sukhov, O.V. Ivanov, G.V. Buklanov, K.Subotic, and M.G. Itkis

      Joint Institute for Nuclear Research, 141980 Dubna, Russian Federation

      K.J. Moody, J.F. Wild, N.J. Stoyer, M.A. Stoyer, and R.W. Lougheed

      University of California, Lawrence Livermore National Laboratory, Livermore, California 94551, USA

      (Received 275 December 1999)

      In the bombardment of a 244Pu target with 48Ca ions, we observed two decay sequences of genetically linked events, each consisting of an implanted heavy atom, two subsequent -decays, and terminated by a spontaneous fission. The measured -energies and corresponding half-lives of the sequential chain members were: E =9.84 MeV (T1/2=1.9 s) and 9.17 MeV (T1/2=9.8 s); for the spontaneous fission (T1/2=7.5 s), the total deposited energy was approximately 230-240 MeV. The decay properties of the synthesized nuclei are consistent with the consecutive -decays originating from the parent even-even nucleus 288114, produced in the 4n-evaporation channel with a cross section of about 1 pb. The observed decay sequences The decay properties of the synthesized nuclei reproduce the decay scenario predicted by the macroscopic-microscopic theory are consistent with the consecutive -decays originating from the parentfor the even-even nuclideeus 288114, produced in the 4n-evaporation channel with a cross section of about 1 pb. Direct comparison of the measured decay properties of the new even-even superheavy nuclei 288114, 284112, and 280110 with theoretical calculations suggests that nuclei in the vicinity of spherical shell closures with Z=114 and N=184 could be even more stable than is predicted by macroscopic-microscopic theory.

      PACS number: 25.70.Gh, 23.60.+e, 25.85.Ca, 27.90.+b

       


      During the last year the first convincing evidence for the discovery synthesis of superheavy nuclei around the theoretically predicted spherical shell closures at Z=114 and N=184 was presented[1-4].

      These reports included the results of our experiment, in which a 244Pu target was bombarded with 5.2x1018 48Ca ions during September-December, 1998, employing the Dubna Gas-filled Recoil Separator. We observed a decay sequence consisting of an implanted heavy atom, three subsequent -decays (E=9.71 MeV, 8.67 MeV and 8.83 MeV), and a spontaneous fission (SF), all correlated in time and position [2]. The most reasonable explanation for this decay chain is consecutive -decays starting from the parent nucleus 289114, produced in the 3n-evaporation channel.

      In March-April, 1999, a 242Pu target was bombarded with 7.5x1018 48Ca ions at the separator VASSILISSA. Two decay chains were assigned to the -decay of the parent nucleus 287114 with T1/2=5.5 s and E=10.29 MeV [3]. Both decay chains were terminated after the first -decays by spontaneous fission of the daughter nucleus 283112, a nuclide previously observed in the 238U+48Ca reaction [1].

      The discovery synthesis of 293118 and its sequential -particle emission to the daughter isotopes with Z=116-106 from the bombardment of 208Pb with 2.3x1018 449-MeV 86Kr ions using the Berkeley separator BGS was announced in April-May, 1999. Three decay chains were observed, each consisting of an implanted atom and six subsequent -decays.

      In June-October, 1999, we continued the bombardment of a 244Pu target with 48Ca ionsprojectiles. Most of the details of the experiment are given in our previous publication [2]. As before, the rotating target consisted of 9 separate targets made of the enriched isotope 244Pu (98.6%) in the form of PuO2, deposited onto 1.5-mm Ti foils to a thickness of ~0.37 mg cm-2. We used a 48Ca bombarding energy of ~236 MeV at the middle of the target. Taking into account the energy loss in the target (~3.4 MeV), the small variation of thickness of individual targets, the beam energy resolution and the variation of the beam energy during the long-term irradiation, the excitation energy of the compound nucleus 292114 was in the range of 31.5-39 MeV [6], which should correspond to the evaporation of 3 or 4 neutrons.

      However, the data acquisition system allowed to determine the individual target sector which gave origin to each detected recoil atom, as well as 48Ca bombarding energy at this time. Thus a narrower range of excitation energy could be put into correspondence to a particular recoil.

      A typical beam intensity on target was 4x1012 pps. Over a period of 60 days a total of 1.0x1019 projectiles was delivered to the target.

      Evaporation residues (EVR) recoiling from the target were separated in flight from beam particles, scattered ions and various transfer-reaction products by the Dubna Gas-filled Recoil Separator [7], passed through a time-of-flight (TOF) detector, and were implanted in the focal-plane detectors, consisting of twelve 4-cm-highx1-cm-wide position sensitive strips. To detect ’s escaping the focal-plane detector, 8 side detectors of the same type without position sensitivity were arranged in a box surrounding the focal-plane detector. The total -particle detection efficiency was ~87% of 4p. A set of 3 similar “veto” detectors was situated behind the focal-plane detectors in order to eliminate signals from low-ionizing light particles, which could pass through the focal-plane detector (300mm) without being detected in the TOF system. At a beam intensity of 4x1012 pps, the overall counting rate of the detector system was ~15 s-1. We estimate that 40% of the recoiling Z=114 nuclei formed in the 244Pu target would be implanted in the focal-plane detector.

      Alpha-energy calibrations were periodically performed using the peaks from nuclides produced in the test reaction 206Pb+48Ca. The fission-energy calibration was obtained by detecting fission fragments from the SF of 252No. The energy resolution for detection of -particles in the focal-plane detector was ~50 keV; for detection by the side detectors of ’s escaping from the focal-plane detector, the energy resolution was ~190 keV. We determined the position resolution of the signals of correlated decays of nuclei implanted in the detectors: For sequential - decays the FWHM position resolution was 1.1 mm; for correlated EVR- signals, 0.8 mm; and for correlated EVR-SF signals, 0.5 mm.

      According to experimental data obtained in the previous experiments [1-3] and
      Подпись:  
Fig. 1  Time sequences in the observed decay chains. The expected half-lives corresponding to the measured E  values for the given isotopes are shown in parentheses following the measured lifetimes. Positions of the observed decay events are given with respect to the top of the strip.

      ![endif]-->
       predicted decay properties of nuclei, the 2-to-4 neutron evaporation products from the compound nucleus 292114 [8,9] should have -decay chains terminated by spontaneous fission.

      We observed only two fission events during this 244Pu+48Ca bombardment. Both SF events were observed as two coincident signals (two fission fragments) with energies EF1=156+65 MeV and EF2=171+42 MeV. The items in each sum mean energies deposited in the focal-plane and side detectors, respectively. We searched the data backwards in time from these events for preceding particles with E>8 MeV [7,8] and/or EVRs, in the same positions. The latter were defined as the nearest events characterized by the measured energies, TOF signals and estimated resulting mass values, that were consistent with those expected for a complete-fusion EVR, as determined in the calibration reaction. The full decay chains including these two fission events are shown in Fig. 1, with the suggested assignment of decays to specific nuclei.

      Both decay chains are consistent with one another, in all the measured characteristics. The first -particles have similar energies E=9.87 MeV and E=9.80 MeV, and were detected in the focal-plane detector 0.77 s and 4.58 s after the implantation of the recoil nuclei in strips 2 and 8, respectively. The second -particles in corresponding chains, having the energies E=9.21 MeV and E=9.13 MeV, were observed at the same locations after 10.34 s and 18.01 s. Finally, 14.26 s and 7.44 s later, the SF events were observed. All events in the two decay chains appeared within time intervals of 25.4 s and 30.0 s and position intervals of 0.5 mm and 0.4 mm (Fig. 1), respectively.

      To estimate the probability of random origin of the candidate decay chains we used two approaches. By applying a Monte Carlo technique [2,10] we determined the probability per fission of finding such correlated events at any position of the detector array. Following the procedure described in Ref. [11] we calculated probabilities of these decay sequences being caused by the chance correlations of unrelated events at the positions in which the candidate events occurred. The probability that both decay chains consist of random events is less then 10-12.

      By applying a Monte Carlo technique [2,10] we determined to estimate the probability of the candidate decay chains being due to random correlations we determined the probability per fission of finding such correlated events to be Perr=3x10-7. By applying the Geiger-Nuttall relationship, we imposed a lifetime window for each -event. That reduced Perr to 3x10-8. The probability that both decay chains consist of uncorrelated events to beis approximately 3x10-15.

      Following the procedure described in Ref. [11], the calculated probabilities Perr of these decay sequences being caused by the chance correlations of randomunrelated events in strips 2 and 8 at the positions in which the candidate events occurred, awere calculated to be 7x10-7 and 8x10-7, respectively, in agreement with the results of the Monte Carlo analysis.

      We observed two three-member decay sequences. If we assume that they actually consisted of four decays (i.e., the spontaneous fission was due to element 108), the probability of missing one -event in both decay chains would be less than 3%.

      The 48Ca beam energy in the middle of the target corresponded to the excitation energy of 36-37-MeV of the compound nuclei, in both cases, suitable expected for evaporation of 4 neutrons from the 292114 compound nucleus. We should also note that Tthe observed decay chains, including two alpha-decays and terminated by SF, match the predicted decay scenario predicted for the even-even nuclide 288114dependence of Q on T for heavy even-Z nuclei with Z³110 [8,9]. For all the chain members, the basic rule of -decay, which defines the relation between Q andT1/2 vs. TE values of the detected sequential decays correspond to the decays of the even-even nuclides with Z=114 and 112, is fulfilled. To illustrate this, Fig. 1 presents the expected half-lives, corresponding to the measured -particle energies for the genetically related nuclides with the specified atomic numbers. For the calculation of half-lives, the formula by Viola and Seaborg has been used, with parameters fitted to the T values of 58 even-even nuclei with Z>82 and N>126, for which both T and Q were measured [8,9]. On the other hand, substituting experimental T1/2 and E values in this formula results in atomic numbers of 114.4 and 110.2 for the mother and daughter nuclides, respectively. The total deposited energies of the two fission events are 230-240 MeV, correcting for pulse-height defect. Despite the relatively wide distributions of the total kinetic energies released in spontaneous fission, these deposited energies also indicate the spontaneous fission of rather heavy granddaughter nucleus with Z 106 [12].

      From the above considerationsThus, we can conclude thatthe most reasonable explanation of  the detectedregistered decay chains is by the consecutive -decays startingoriginate from the parent even-even nuclide 288114, produced in the 244Pu+48Ca reaction via 4n-evaporation channel. On the basis of two detected events, the cross section of this reaction is about 1 pb.

      Подпись:  
Fig. 2 Alpha-decay energy vs. neutron number for isotopes of even-Z elements with Z³100 (solid circles) [14-17>. Open circles show data from Ref. [4], triangle from Ref. [3], solid squares - from Ref. [2], and diamonds - data of the present work. Open circles connected with solid lines show theoreti-cal Q  values [8,9] for even-even Z=106-114 isotopes.

      The new decay sequences evidently originate from a different parent nucleus than a single chain that was observed previously in the reaction 244Pu+48Ca and attributed to the decay of 289114 [2]. The new alpha-decaying nuclides are characterized by higher decay energies than the corresponding members of the chain observed in [2], while SF terminates the decay sequence at an earlier stage. Thus, comparison of the decay properties supports assignment of a previously observed longer sequence to the decay of a heavier odd nuclide 289114 [2].

      Both series of experiments with the 244Pu+48Ca reaction were performed under essentially the same experimental conditions with a resulting integral beam dose of 1.5x1019 ions. From the experimental dependencies of the cross sections of symmetric fission induced by 48Ca ions on the 238U and 244Pu targets and recent calculations [13], Eevaporation of 3 or 4 neutrons from the compound nucleus 292114 could be expected, with close probabilities, aint the investigated excitation energy range of of 31.5-39 MeVV. In this respect, Recent semiempirical calculations [13] predict the cross section maxima for emission of 3 and 4 neutrons from the compound nucleus 292114 at the excitation energy of 30 MeV and 38 MeV, respectively. tThe observation of the two neighbouring isotopes of element 114 in the present difference in results of two experiments is thus understandable, keeping in mind the low number of events and the narrow widths expected for the excitation functions. Further, we plan to continue our experiment using ~5 MeV lower projectile energy to search for additional decays of 289114.

      The radioactive properties of the new observed nuclides are in qualitative agreement with predictions of the macroscopic-microscopic nuclear theory [8,9]. The experimental data exactly reproduced the predicted for 288114 decay scenario, i.e., two consecutive -decays terminated by spontaneous fission. Moreover, the radioactive properties of new nuclides agree with those that could be expected from the decay properties of previously synthesized neighbouring odd isotopes 287,289114 [2,3] and 285112 [2].

      The properties of the observed even-even nuclei can be directly compared with calculations [8,9]. Alpha-decay energies of known isotopes of even-Z elements with Z 100 together with theoretical Q values [8,9] for even-even isotopes with Z=106-114 are shown in Fig. 2.

      Comparison of the measured decay properties of the new even-even superheavy nuclei 288114 (E=9.84±0.05 MeV, T1/2=1.9 s), 284112 (E=9.17±0.05 MeV, T1/2=9.8 s), and 280110 (T1/2=7.5 s) with theoretical calculations [8,9] indicates that nuclei in the vicinity of spherical shell closures with Z=114 and N=184 could be even more stable than is predicted by theory. It can be seen in Fig. 2 that alpha-decay energies of the heaviest new even-even nuclides with Z=112 and 114 are 0.4-0.5 MeV less than predicted values. The heaviest even-odd nuclides follow this trend, as well. Such a decrease in Q values leads to an increase of partial -decay lifetimes by an order of magnitude. Calculations are far less definite, regarding spontaneous fission; however, we note that the observed spontaneous fission half-life of 280110 exceeds the predicted value [8] by more than two orders of magnitude.

      We would like to express our gratitude to I.V. Kalagin and the personnel of the U400 cyclotron and the associates of the ion-source group for obtaining an intense 48Ca beam. We are grateful to the JINR Directorate, in particular to Profs. Ts. Vylov and, V.G. Kadyshevsky and A.N. Sisakian for the help and support we got during all stages of performing the experiment. We express our thanks to Dr. V.B. Zlokazov for mathematical analysis of data, Drs. V.Ya. Lebedev and S.N. Dmitriev for developing methods for preparation of the metal Ca samples for the ECR-ion source, and also to V.I. Krashonkin, V.I. Tomin, A.M. Zubareva, and A.N. Shamanin, for their help in preparing and carrying out the experiment.

      The Livermore authors thank their Russian hosts for their hospitality during the experiment.

      This work has been performed with the support of INTAS under grant No. 96-662. Much of support was provided through a special investment of the Russian Ministry of Atomic Energy. The 244Pu target material was provided by the U.S. DOE through ORNL. Much of the support for the LLNL authors was provided through the U.S. DOE under Contract No. W-7405-Eng-48. These studies were performed in the framework of the Russian Federation/U.S. Joint Coordinating Committee for Research on Fundamental Properties of Matter.

       

       

      [1] Yu.Ts. Oganessian et al., Eur. Phys. J. A 5, 63 (1999).

      [2] Yu.Ts. Oganessian et al., Phys. Rev. Lett. 83, 3154 (1999).

      [3] Yu.Ts. Oganessian et al., Nature 400, 242 (1999).

      [4] V. Ninov et al., Phys. Rev. Lett. 83, 3154 (1999).

      [5] S. Hofmann et al., private communication.

      [6] W. D. Myers and W. J. Swiatecki, Nucl. Phys. A 601, 141 (1996).

      [7] Yu.Ts. Oganessian et al., in Proceedings of the Fourth International Conference on Dynamical Aspects of Nuclear Fission, Casta-Papernicka, Slovak Republic, 1998 (to be published).

      [8] R. Smolanczuk, J. Skalski, and A. Sobiczewski, in Proceedings of the International Workshop XXIV on Gross Properties of Nuclei and Nuclear Excitations "Extremes of Nuclear Structure", Hirschegg, 1996 (GSI, Darmstadt, 1996), p.35.

      [9] R. Smolanczuk, Phys. Rev. C 56, 812 (1997).

      [10] N. Stoyer et al., (to be published in Nucl. Inst. Methods A).

      [11] V.B. Zlokazov, JINR Report No. E7-99-273, 1999; Eur. Phys. J. A (submitted).

      [12] M.G. Itkis

      [13] R.N. Sagaidak, in Proceedings of the International Conference on Nuclear Physics "Nuclear Shells - 50 Years", Dubna, 1999 (to be published).

      [14] S. Hofmann et al., Z. Phys. A 350, 277 (1995); Nachrichten GSI 02-95, 4 (1995); Z. Phys. A 350, 281 (1995); Z. Phys. A 354, 229 (1996).

      [15] Yu. A. Lazarev et al., Phys. Rev. Lett. 73, 624 (1994); Phys. Rev. Lett. 75, 1903 (1995); Phys. Rev. C 54, 620 (1996).

      [16] A. Ghiorso A. et al., Phys. Rev. C 51, R2293 (1995).

      [17] R.B. Firestone, V.S. Shirley (editor): Table of Isotopes eighth edition, John Wiley & sons, inc. New York, Chichester, Brisbane, Toronto, Singapore, 1996.

      Hosted by uCoz