Yu.Ts.Oganessian et al
EXPERIMENT ON THE SYNTHESIS OF ELEMENT 115
IN THE REACTION
243Am(48Ca,
xn)291-x115
I. INTRODUCTION
Our previous experiments
were designed to synthesize even-Z superheavy elements (114-118) in the 48Ca-induced
reactions with actinide targets 244Pu [1], 248Cm [2] and 249Cf
[3]. The observed fusion-evaporation reaction products underwent two or three
consecutive α-decays
terminated by spontaneous fission (SF).
For the neighboring odd-Z
elements, especially their odd-odd isotopes, the probability of α-decay with respect to SF should
increase due to hindrance for SF. For such odd-Z nuclei one might expect longer
consecutive α-decay
chains terminated by the SF of relatively light descendant nuclides (Z<105).
The decay pattern of these
superheavy nuclei is of interest for nuclear theory. In the course of α-decays, the increased stability of
nuclei caused by the predicted spherical neutron shell N=184 (or perhaps N=172)
should gradually become weaker for descendant isotopes. However, the stability
of these nuclei at the end of the decay chains should increase again due to the
influence of the deformed shell at N=\62.
The observation of nuclei
passing from spherical to deformed shapes in the course of their consecutive α-decays could provide valuable
information about the influence of significant nuclear structure changes on the
decay properties of these nuclei. For these investigations, we chose the
fusion-evaporation reaction 243Am+48Ca, leading to
isotopes of element 115. According to calculations based on the results of
experiments on the synthesis of even-Z nuclei [1-4], the 3/7- and
4/7-evaporation channels leading to isotopes 288115 (N=\73) and 287115
(N=172) should be observed with the highest yields.
II. EXPERIMENT
The experiments were
performed between July J4 and August 10, 2003, at the U400 cyclotron with the
Dubna gas-filled recoil-separator (DGFRS). The average incident beam intensity
was 1.3 pμA). Over
this period, equal beam doses of 4.3∙l018 48Ca projectiles
were delivered to the target at two bombarding energies. In this experiment, we
chose the laboratory energies for the 4SCa ions of 248 MeV and 253
MeV in the middle of the target. The systematic uncertainty in the beam energy
is ~1 MeV. With the beam energy resolution, small variation of the beam energy
during irradiation and energy losses in the target (-3.3 MeV). we expected the
resulting compound nuclei 291115 to have excitation energies between
38.0-42.3 MeV and 42.4-46.5 MeV, respectively [5].
The 32-cm2
rotating target consisted of the enriched isotope 243Am (99.9%) in
the form of AmO2. The target material was deposited onto 1.5-μm Ti foils to a thickness
corresponding to ≈0.36 mg cm-2 of 243Am.
The evaporation residues
(EVRs) recoiling from the target were separated in flight from the 48Ca
beam ions, scattered particles and transfer-reaction products by the DGFRS [6].
The transmission efficiency of the separator for Z=115 nuclei was estimated to
be about 35% [6].
The detection system consisted
of a multiwire proportional counter to measure time-of-flight (TOF) and a
4xl2-cm2 semiconductor focal-plane detector array with 12 vertical
position-sensitive strips to measure the decay of the implanted recoils. This
detector, in turn, was surrounded by eight 4x4-cm2 side detectors
without position sensitivity, forming a box of detectors open from the front
side. The detection efficiency for α-decays of implanted nuclei was 87% of 4π. The detection system was tested by
registering the recoil nuclei and α- and SF-decays of the known isotopes of Jl and
Th, as well as their descendants, produced in the reactions 206Pb(48Ca,
2n) and natYb(48Ca, 3-5n). The energy resolution for
cc-particles absorbed in the focal-plane detector was 60-100 keV, depending on the
strip and the position in the strip. For α's escaping the focal-plane detector at
different angles and registered by side detectors, the energy resolution of the
summed signals was 140-200 keV. The FWHM position resolutions of correlated
decays of nuclei implanted in the focal-plane detector were 0.9-1.9 mm for EVR-α correlations and 0.5-0.9 mm for
EVR-SF correlations. If both the focal-plane and a side detector detected an α-particle, the position resolution
depended on the amplitude of the signal in the focal-plane detector (see, e.g.,
Fig. 4 in [3]), but was generally inferior to that obtained for the full-energy
signal.
Fission fragments from 252Jl
implants produced in the 206Pb+48Ca reaction were used
for a fission-energy calibration. The measured fragment energies were not
corrected for the pulse-height defect of the detectors, or for the energy loss
in the detectors' entrance windows, dead layers, and low-pressure pentane gas
filling the detection system. The mean sum energy loss of fission fragments
from the SF-decay of 252Jl was estimated to be about 20 MeV.
To greatly reduce the
background, we switched off the beam after a recoil signal was detected with
preset parameters of implantation energy and TOF expected for Z=115 evaporation
residues, followed by an α-like signal with an energy of 9.6 MeV< Ea <11.0 MeV in
the same strip, within a position window of 1.4-1.9 mm and time interval of up
to 8 s. The beam-off interval was initially set at 2 minutes. If, in this time
interval, an α-particle
with Ea>8.6 MeV was registered, the beam-off interval was
extended to between 12 minutes and 2.5 hours. Thus, all the expected sequential
decays of the daughter nuclides with Z<113 could be observed under very low
background conditions.
III. EXPERIMENTAL RESULTS AND DISCUSSION
The three similar decay
chains observed at 248 MeV are shown in Fig. la. The implantations of recoils in strips 2, 3
and 4 of the focal-plane detector were followed by α-particles with Ea=10.46±0.06
MeV. These sequences switched the ion beam off, and four more α-decays were detected in time
intervals of 29 s, 15 s, and 20 s, respectively, in the absence of a
beam-associated background. The last α-decay in the first chain and second and fourth
α-decays in the
second chain were registered by the side detectors only. The energies deposited
by these α-particles
in the focal-plane detector were not registered. However, with the actual α-counting rates, the probability
that these α-particles
appeared in the detector (Δt~30 s) as random events can be estimated to be approximately 1.5% [7],
so we assign them to the decay of the same implanted nuclei. During the
remainder of the 2.5 h beam-off period following the last position-correlated α-particle, no α-particles with Ea>1.6
MeV were registered by the focal-plane detectors. The SF-decay of the final
nuclei in these chains was detected 28.7 h, 23.5 h and 16.8 h, respectively,
after the last α-decay.
A search was performed to identify α-decays correlated closely in time (<60 s)
and position to each of the three SF-events in Fig. la. No correlations were found.
In the first two decay
chains, the focal-plane and side detectors simultaneously detected fission
fragments with sum energies of 205 MeV and 200 MeV. In the third chain, only
the focal-plane detector registered a fission fragment. All three SF-events
were registered in the corresponding strips and positions where the three EVR-α1-α5 decay chains were observed (see Fig. la). Thus, these SF-events should be
assigned to the spontaneous fission of the descendant nuclei in these observed
chains.
In the course of this
experiment at 248 MeV, we observed only seven spontaneous-fission events. In
addition to the three previously mentioned events, three other SF-events, with
measured energies of 147 MeV, 168 MeV, and 154 MeV, were detected 0.51 ms, 4.1
ms and 2.07 ms after the implantation of corresponding recoil nuclei in strips
12, 10 and 11, respectively. For the second and third event, both the
focal-plane and side detectors registered fission fragments. Based on the
apparent lifetime, we assign these events to the spontaneous fission of the
0.9-ms 244mlAm isomer, a product of transfer reactions with the 24jAm
target. The DGFRS suppresses the yield of such products by a factor of 105.
An additional long-lived SF event with Esum=146 MeV was observed in
strip 2. This SF event corresponds to the background level of long-lived SF Cf
isotopes produced in incomplete fusion reactions in a previous experiment with
a 249Cf target [3] where the same set of detectors was used.
At 253 MeV, the
aforementioned EVR-α1-α5 -SF decay chains were not observed. However, a
different decay chain, consisting of lour α-decays and a spontaneous fission, was
registered (see Fig. lb). The beam was switched off after the detection
of an EVR signal followed in 46.6 ms by an α-particle with Ea=10.50MeV in the
same position in strip 7. Three other a decays were detected in a time interval
of about 0.4 s in the absence of beam-associated background. After 106 minutes,
the terminal SF-event was detected in-beam with a sum energy of 206 MeV in the
same position in strip 7 (see Fig. lb). In addition to this SF event with Esl,m=206
MeV, the decays of three other long-lived background SF nuclei, with measured
fission-fragment energies of 168 MeV, 154 MeV, and 151 MeV, were also observed
in strips 4, 3 and 1, respectively.
The radioactive properties
of nuclei in this decay chain differ from those of the nuclei observed at the
lower bombarding energy. The total decay time of this chain is about 10 times
shorter and the α-decays
are distinguished by higher α-particle energies and shorter lifetimes. Its production also required
increasing the beam energy by about 5 MeV, so this decay chain must originate
from another parent nucleus.
It is most reasonable that
the different decay chains originate from neighboring parent isotopes of
element 115, produced in the complete fusion reaction 243Arn+48Ca
followed by evaporation of three and four neutrons from the compound nucleus 291115.
Indeed, at the excitation energy E =40 MeV, close to the expected maximum for
the 3/7-evaporation channel, we observed longer decay chains of the odd-odd
isotope 288115.
Increasing the beam energy
by 5 MeV results in reducing the 288115-isotope yield and, at the
same time, increasing the yield of the 4“-evaporation channel leading to the
even-odd isotope 287115. Corresponding cross sections for the 3n-
and 4n-evaporation channels at the two projectile energies were measured to be
2.7 pb for 3n-channel and 0.9 pb for 4n-channel. Note that these values are in
agreement with results of recent experiments [4] where excitation functions for
the reaction 244Pu(48Ca,xn) have been measured.
The decay properties of the
product nuclei are presented in Table 1. In the decay chains shown in Fig. la, we assigned SF-events to the
isotope 268Db following five consecutive a-decays. It is also
possible that this isotope undergoes a-decay or electron capture (EC). In the
case of the a-decay of 268Ns with Ta>2.5 h
(after the beam-off period), one would more reasonably expect SF or EC of 264Rf,
because the a-decay of 264Rf seems improbable due to the low
expected a-decay energy (ga=6.84 MeV [8], ra>100 d). The
electron capture of 268Ns or 264Rf leads to the even-even
isotopes 268Ku or 264Jl, for which rapid spontaneous
fission can be expected (e.g., T1/2=1.4 s is predicted for 268Ku
[9]). Since both fission fragments of these terminal nuclei can have the Z=50
and N=82 closed shell configurations, one would expect their SF-decays to
result in narrowly symmetric mass distributions with rather high total kinetic
energies, TKE=230-240 MeV (see, e.g., Ref. [10]). Indeed, the sum fission
fragment energies observed for the terminal nuclei are close to this value. Note,
the likelihood that EC-decay occurs earlier in the observed decay chains is
small because of the short Ta for the observed a-decays of
elements 115, 113, Rg, Mt, and 107.
In the single decay chain
originating from 287115 (see Fig. lb. and Table 1), we propose that we have missed the a-decay
of 271Bh. This assumption follows from the a-decay properties of
nuclei located around N=\62 as predicted by macroscopic-microscopic
theory [8], The expected Ta value for 271107
should be -10 s (go=9.07 MeV [8], Ta~5 s for an
allowed transition), which is much shorter than the interval between the last
observed a-particle and the terminating SF-event, but is much longer than the
intervals between the observed correlated a-particles. A search was performed
to identify a-particles with Ea>7.0 MeV correlated in position to
the observed a-decays. No correlated a-particles were observed within an hour after
the last a-decay. In these experiments, we registered 19 a-particles using a
detector with 87% efficiency, so the loss of one a-particle seems rather
probable. The experimental decay scheme for 287115 is also supported
by the agreement of the observed decay properties of the other nuclides in the
decay chain with the expectations of theory (see Fig. 2). This means that the SF occurs
directly in the decay of Ns since the calculated a-decay and EC-energies for
this isotope are rather low (ga=7.41 MeV [8], E>EC=1
MeV [5]) and their expected partial half-lives significantly exceed the
observed time interval of 106 min.
For the measured α-decay energies of the
newly-produced isotopes, one can estimate half-lives for allowed transitions
and compare them with experimental values under the Geiger-Nuttall treatment
using the formula by Viola and Seaborg. Parameters are obtained from fits to
the Ta vs. Qa values of 65 known even-even nuclei with
Z>82 and N>126. The ratios between experimental rexp and
calculated rcalc half-lives define the hindrance factors caused by
odd numbers of protons and/or neutrons in the newly synthesized nuclei. The
measured Texp values closely reproduce the calculated ones for the
first two nuclei of these chains; thus the element 115 and element 113 isotopes
have rather low hindrance factors, if any, for α-decay. For the isotopes of elements Rg, Mt and
107, the difference between measured and calculated Ta values
results in hindrance factors of 3-10. These match the hindrance factors that
can be extracted for the deformed odd-odd nuclei 272Rg and
descendants produced in experiments at GSI [11] and RIKEN [12]. One can suppose
that in this region of nuclei, a noticeable transition from spherical to
deformed shapes occurs at Z= 109-111, resulting in the complication of the
level structures of these nuclei and in an increased probability of α-transitions going through excited
states. Another sign of such a shape transition might be the significant
increase in the difference of α-decay energies of the neighboring isotopes observed as the decay chains
reach Z=lll, see Fig. 2. This assumption is in agreement with
macroscopic-microscopic calculations [8]. The deformation parameter β2 was calculated to be 0.072 and 0.138 for 288115
and 284113, respectively. As the decay chain recedes from the shell
closure at Z= 114, the deformation parameter β2 increases to 0.200, 0.211 and 0.247 for 280l
11,276Mt and 272107, respectively.
The α-decay energies of these synthesized
isotopes are plotted in Fig. 2, in which the α-decay energies of known odd-Z isotopes with
Z>103 together with theoretical Qa values [8] for nuclides with
Z=103-115 are also shown. The α-decay energies of newly produced isotopes of Mt and 107 coincide well
with theoretical values [8]. For the isotopes 279,280 Rg and 283,284113
the difference between theoretical and experimental Qa values amount
to 0.6-0.9 MeV. Some part of this deficient energy can be explained by possible
γ-ray emission
from excited levels populated during α-decay. Thus, low-lying level structure
calculations for these nuclei are desirable for a more quantitative comparison
with theory.
As a whole, the results of
the present work demonstrate that in 48Cα-induced reactions one can produce
and study new nuclei over a wide range of Z and N. These investigations should
result in significant new information on the influence of nuclear structure on
the decay properties of superheavy nuclei.
Due to the hindrance to
spontaneous fission caused by the odd proton, these odd-Z nuclei can undergo
consecutive α-decays
leading to the lighter transactinide elements that have a large neutron excess.
The number of neutrons in such nuclides can be varied downward by using other
target nuclei, e.g., 241Am, 237Np or 231Pa. Therefore,
the investigation of the region of nuclei located near deformed shell closures
Z=108 and N=162 that has been explored from the N<162 side in the cold
fusion reactions [11,12] can be approached from the high-N side using 48Ca-induced
reactions. Note also that the rather long lifetimes of Ns isotopes permit us to
investigate, in more detail, the chemical properties of this element,
previously studied only in on-line experiments with the short-lived isotopes 261,262,263Ns
(Tα=1.8
s, 34 s and 27 s) (see, e.g., [16] and Refs. therein).
ACKNOWLEDGMENTS
We are grateful to the JINR
Directorate, in particular to Profs. V.G. Kadyshevsky, Ts. Vylov and A.N.
Sissakian for the help and support we received during all stages of the
experiment. We would like to express our gratitude to the personnel of the U400
cyclotron and the associates of the ion-source group for obtaining an intense 48Ca
beam. This work has been performed with the support of the Russian Ministry of
Atomic Energy and grants of RFBR No. 01-02-16486 and 03-02-06236. The 243Am
target material was provided by RIAR, Dimitrovgrad, and 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.
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