A fusion reaction occurs when two
nuclei come together with sufficient kinetic energy to overcome their mutual
electrostatic repulsion (Coulomb barrier) and form a compound nucleus.
Depending upon the available kinetic energy, the collision partners will fuse
either by passing over or by quantum mechanical tunneling through the Coulomb
barrier. Fusion is one of the ways of producing elements and energy during
nucleosynthesis in the stars, whereas on earth
it is the only
way to produce new very short
lived elements to extend the periodic table. Further, the fusion between two
heavy nuclei at energies around the Coulomb barrier serves as an illustration
of various quantum mechanical aspects. Measurements both here and at other
laboratories showed that the fusion of two nuclei is a multidimensional
tunneling problem which not only depends on the radial separation but is also
very strongly governed by their internal structure. Fusion below the barrier
energy provides an excellent illustration of the connection between various
internal degrees of freedom (direct reactions channels) and the translational
degrees of freedom of the two colliding nuclei (elastic scattering). The
probability of the nuclei to fuse (compound nucleus formation) can be obtained
from measurement of various decay products of the compound nucleus. These could
be measurements of characteristic gamma rays originating from the decay of
evaporation residues, number of fission fragments or direct measurements of the
evaporation residues using a recoil mass separator.
Apart from showing the effect
of the internal properties of the interacting nuclei on the fusion process, a
new method to obtain the angular momentum of the fused nuclei and its
connection with the fusion excitation function have been suggested from
experiments done here. Recent availability of unstable beams, also known as
Radioactive ion beams (beams of short lived nuclei having low binding energy
and a larger extended matter distribution as compared to stable nuclei), at
various facilities around the world have prompted the investigation of
influence of their properties on the reaction process. A precursor to such
studies is the study of stable but weakly bound nuclei. Experiments have been performed to understand
if fusion with weakly bound nuclei behaves differently from normal nuclei
Reactions in which the
interaction between projectile and target happens through a specific degree of
freedom (either a single nucleon or a collective coordinate) causing a change
in that degree of freedom are called direct reactions. Here the two colliding
nuclei essentially maintain their identity after the interaction. By studying
the energy and angular distributions of the nuclei scattered after the
reactions information about the interaction potential (elastic scattering), the
internal states, which correspond to a particular state of motion of the
constituent nucleons (inelastic scattering) and correlations of nucleons like
paring are obtained. Further, these studies provide an insight into how the
states of nuclei can be visualized in terms of various internal
configurations (transfer reactions).
Studies in our lab have focused on understanding the energy dependence of the
interaction potential, breakup of weakly bound nuclei, mechanism of transfer
for a pair of nucleons to see whether they are transferred sequentially or as a
pair, clustering in nuclei and the deviation of one and two nucleon transfer at
large relative distance between the interacting nuclei from theoretical models.
Heavy – ion resonances
a
In the case of
some nuclei, the variation of the cross section for a given process, like
elastic or inelastic scattering, as a function of the projectile energy shows
fluctuations in the form of high and narrow
peaks. A characteristic feature of these resonances, unlike the fluctuations,
is that it shows up simultaneously in various outgoing channels and at all
angles. These fluctuations can be understood in terms of the formation of long
lived, positive energy states of the projectile and target, known as ‘molecular
configurations’. It is very difficult to
identify these states (because of their larger widths) unless they have
a very special structure. Studies here have
focused on investigation of such
states at high energies in light ystems consisting of “4N” nuclei like 16O+12C,
12C+12C. The detailed study of excitation functions of
various outgoing reaction channels for a given incoming channel has helped in
determining their structure. Using the outgoing particle correlations some of
these structures have been interpreted as a linear chain of 6 a particles and others have been shown to
be highly deformed.
