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This work explores the relationship between the Giant Monopole Resonance (GMR) and the incompressibility of nuclear matter, K∞, by analyzing various effective interactions and GMR strength distributions using an RPA framework. We compare our calculations with experimental data on the EGMR and EISGDR to confirm consistency across non-relativistic and relativistic models. Furthermore, we discuss the significance of "soft" GMR and present first experimental results using deuteron and helium targets at GANIL, employing advanced detection methods to enhance understanding of neutron-rich nuclei.
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From EGMR and EISGDR to K∞ However, the available GMR data can lead to a wide range of values for K∞ (100--500 MeV!) • So, "microscopic approach": • Select "suitable" effective interactions. • Calculate the GMR strength distributions in an RPA approach • Compare with the experimental EGMR and EISGDR K∞
This number is consistent with both GMR and ISGDR Data and with non-relativistic and relativistic calculations
Towards very neutron-rich nuclei • Kt • Kcore and Kskin “soft GMR” akin to pigmy GDR’s. • Need inverse reactions 2H, 4He, or 6Li targets beams of 35-100 MeV/A • First experiment performed at • GANIL • 56Ni + 2H, with active target MAYA
Ionization chamber Si wall Drift chamber Moving flap CsI wall Au foil Diamond MAYA @ GANIL MAYA
58Ni (d, d’) d break-up # counts/MeV MAYA @ GANIL C. Monrozeau et al., Phys. Rev. Lett. 100, 042501 (2008)