exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
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width measurements.<br />
This relationship simply illustrates the fact that an<br />
atomic vacancy which has been created in the<br />
entrance channel phase of the collision in the <strong>reaction</strong><br />
partners — <strong>and</strong> transferred to the fused nucleus<br />
after electronic orbital arrangements — disappears<br />
either because it decays through X ray<br />
emission, characteristic of the formed element, or<br />
because a nuclear decay process has occurred,<br />
leading to a new element whose characteristic inner<br />
shell X-ray is different. These competing processes<br />
between nuclear <strong>and</strong> atomic decays will<br />
eventually continue along the decay chain. The<br />
experiment performed at Ganil in November 2009<br />
focused on the compared decay of 103 In <strong>and</strong> 109 In<br />
formed in the <strong>reaction</strong>s 76 Kr+ 27 Al <strong>and</strong> 82 Kr+ 27 Al at<br />
340 MeV.<br />
The second experiment entitled "Super-Heavy Element<br />
Fission Time Measurements Using Inner-<br />
Shell Ionization” is the first step of the SHE stability<br />
measurement program which extends our crystal<br />
blocking experiments. The lifetimes of K- <strong>and</strong> L-<br />
shell vacancies of such atoms, in the 10 -18 s <strong>and</strong><br />
10 -17 s range, respectively, should allow to measure<br />
fission times much longer than the nuclear formation<br />
time. In particular by choosing fissioning<br />
<strong>nuclei</strong> with atomic numbers near or at predicted<br />
closed shells for protons <strong>and</strong>/or neutrons, one<br />
should be able to probe the stability of super-heavy<br />
elements as the high fission barriers expected in<br />
the vicinity of shell closures should lead to fission<br />
times long enough for K <strong>and</strong> L X-ray emission from<br />
the compound nucleus. Moreover, X-ray observation<br />
from super-heavy compound <strong>nuclei</strong> gives access<br />
at the same time to their charge identification<br />
<strong>and</strong> to a quantitative estimate of their fission time,<br />
bringing thus valuable <strong>and</strong> complementary pieces<br />
of information to the crystal-blocking experiments<br />
performed at GANIL. In addition, this method allows<br />
the study of systems for which single crystal<br />
targets are not available.<br />
In a first step, this alternative method for fission<br />
time measurement, independent of any nuclear<br />
model has been applied in December 2009 to the<br />
Z=120 element formed in U induced <strong>reaction</strong>s on<br />
Ni targets. The confirmation of the existence of<br />
long lifetime ( > 10 -18 s) components for such heavy<br />
elements by two independent experimental methods<br />
is of crucial interest as within the present theoretical<br />
approaches it seems quite difficult to reconcile<br />
the very tiny measured residue cross sections<br />
<strong>and</strong> the rather high cross sections associated to<br />
compound <strong>nuclei</strong> surviving against fission longer<br />
than 10 -18 s. In addition , by studying the 238 U +<br />
58 Ni <strong>and</strong> 238 U + 64 Ni systems, the evolution of fission<br />
times with neutron numbers in the proximity of<br />
the neutron shell closure can also be studied, providing<br />
thus very sensitive tests of nuclear shell<br />
models.<br />
The experimental planning<br />
Successful tests have been realized in September<br />
2008, in order to check the background counting<br />
rates registered in the X-ray Germanium detectors<br />
at low energy <strong>and</strong> the feasibility of the lifetime<br />
measurement experiments based on the Atomic<br />
Clock technique. 2009 has been mainly dedicated<br />
to the realization <strong>and</strong> tests of the different parts of<br />
the experimental set-up: the sectorized ionization<br />
chambers constituting the first stage of the<br />
charged fragment telescopes built in Ganil have<br />
been tested in June. Then we tested the sensitivity<br />
of diamond monocristal detectors to radiation damage<br />
with 7.5 A MeV 129Xe beams, in order to<br />
check whether this type of detectors could be used<br />
to detect the elastically scattered projectiles in our<br />
experiments, to deduce the inner shell ionization<br />
probabilities. Finally it appeared that the pulseheight<br />
delivered by these diamond detectors was<br />
quite rapidly affected by the radiation damage,<br />
which led us to use alternatively the elastically<br />
scattered target <strong>nuclei</strong> in st<strong>and</strong>ard detectors located<br />
at large angles.<br />
Furthermore, all the mechanics needed to install<br />
the FluoX detection set up around the Vamos target<br />
have been designed <strong>and</strong> built this year: a set of<br />
supports for the Germanium detectors operated<br />
under vacuum, allowing precise displacements has<br />
been designed in <strong>IPN</strong>O whereas the <strong>reaction</strong><br />
chamber hosting the fragment detectors was<br />
drawn in Ganil. A few days of beam time have<br />
been used in September to check the whole setup,<br />
including the Vamos spectrometer <strong>and</strong> finally<br />
the two scheduled experiments have been successfully<br />
performed in the last months of 2009.<br />
The analysis of these two experiments just started<br />
in January 2010.<br />
References<br />
[1] Morjean M. et al «Fission time measurements: a new probe<br />
into super-heavy element stability», Physical Review Letters,<br />
101, 072701, 2008<br />
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