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
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
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.
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.