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NeuLAND - FAIR

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In the following section we discuss the <strong>NeuLAND</strong> performance along some of the physics<br />

examples, as laid out in chapter 2. However, to summarize the overall relative energy<br />

resolution σ(Erel), we display in figure 4.17 σ(Erel) as a function of Erel, exemplarily for<br />

132 Sn decaying into 131 Sn and one neutron at beam energies of 600 AMeV, derived from<br />

phase-space simulations.<br />

Figure 4.17.: The relative energy resolution σ(Erel) for Erel values from 100 to 3000 keV<br />

is shown for 132 Sn decaying into 131 Sn and one neutron at beam energies of<br />

600 AMeV. The values, derived from phase-space simulations, are displayed<br />

for distances between the detector and the target of 15.5 m (squares) and<br />

35 m (circles). The resolution is proportional to the square-root of Erel,<br />

the curves present fit functions with a proportionality to √ Erel.<br />

4.5.4. Physics Cases<br />

Evolution of the Collective Response of Exotic Nuclei<br />

For the investigation of heavy exotic nuclei with respect to their collective response, we<br />

discuss, exemplarily, the case of 136 Sn, excited in inverse kinematics via the Coulomb<br />

interaction. The input distribution of dipole strength takes into account a giant dipole<br />

resonance (GDR) and additional strength at lower energy, resembling the pygmy dipole<br />

resonance (PDR). For the GDR, a peak energy of Em = 15.5 MeV and a resonance<br />

width of Γ = 4 MeV were adopted as resonance parameters from systematics. The<br />

GDR exhausts 100% Thomas-Reiche-Kuhn (TRK) sum rule strength. For the PDR,<br />

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