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Perspectives of Nuclear Physics in Europe - European Science ...

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Figure 5. Gamma-ray spectrum <strong>of</strong> the Pygmy Dipole Resonance (PDR) <strong>in</strong> 68 Ni, measured with the RISING array at GSI (left) and a compilation<br />

<strong>of</strong> <strong>in</strong>tegrated low-ly<strong>in</strong>g dipole strength <strong>in</strong> stable and neutron-rich nuclei from S-DALINAC and GSI, respectively, shown as a function <strong>of</strong><br />

asymmetry.<br />

Coulomb projectile break-up at a few hundred MeV/u<br />

are used for these studies. Detailed complementary<br />

studies <strong>of</strong> this new excitation mode known as the Pigmy<br />

Dipole Resonance (PDR), can be done <strong>in</strong> stable nuclei<br />

by employ<strong>in</strong>g electromagnetic and hadronic probes. The<br />

right part <strong>of</strong> Figure 5 shows a compilation <strong>of</strong> observed<br />

low-ly<strong>in</strong>g dipole strength as a function <strong>of</strong> neutron-proton<br />

asymmetry α.<br />

Counts/MeV<br />

It is important to understand the nature <strong>of</strong> the low- and<br />

high-energy components <strong>of</strong> the dipole strength <strong>in</strong> general.<br />

Therefore, studies <strong>of</strong> its evolution as a function <strong>of</strong><br />

larger neutron-proton asymmetry, deformation and temperature<br />

are called for. A very <strong>in</strong>terest<strong>in</strong>g aspect is the<br />

relation <strong>of</strong> the dipole strength to the density-dependence<br />

<strong>of</strong> the symmetry energy and the neutron-sk<strong>in</strong> thickness.<br />

The equation <strong>of</strong> state (EOS) for asymmetric nuclear matter<br />

is particularly important for the understand<strong>in</strong>g and<br />

description <strong>of</strong> neutron-star properties.<br />

The measurement <strong>of</strong> giant resonances <strong>of</strong> other<br />

multipolarities as well as magnetic excitation modes <strong>in</strong><br />

unstable nuclei require new experimental techniques,<br />

such as those based on light-ion scatter<strong>in</strong>g <strong>in</strong> <strong>in</strong>verse<br />

k<strong>in</strong>ematics. A pilot measurement for the giant monopole<br />

excitation, provid<strong>in</strong>g <strong>in</strong>formation on the nuclear compressibility,<br />

was made for the unstable 56 Ni nucleus<br />

(Figure 6) us<strong>in</strong>g <strong>in</strong>verse k<strong>in</strong>ematics and the active target<br />

MAYA (Figure 12). The key <strong>in</strong>strumentation to enable<br />

major experimental steps towards the understand<strong>in</strong>g<br />

Figure 6. Giant quadrupole resonance (16.5 MeV) and giant<br />

monopole resonance (19.5 MeV) <strong>in</strong> 56 Ni <strong>in</strong>duced by the 56 Ni(d,d’)<br />

reaction at 50 MeV/u <strong>in</strong> the MAYA active target at GANIL .<br />

<strong>of</strong> giant resonances <strong>in</strong> exotic nuclei will be available at<br />

FAIR with R 3 B and the storage-r<strong>in</strong>g experiments EXL<br />

and ELISe employ<strong>in</strong>g hadron and electron scatter<strong>in</strong>g,<br />

respectively.<br />

<strong>Perspectives</strong> <strong>of</strong> <strong>Nuclear</strong> <strong>Physics</strong> <strong>in</strong> <strong>Europe</strong> – NuPECC Long Range Plan 2010 | 117

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