Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
X. Roca-Maza, M. Brenna, B. K. Agrawal, P. F. Bortignon, G. Col\`o,, Li-Gang Cao, N. Paar, D. Vretenar

TL;DR
This paper investigates the properties of giant quadrupole resonances in 208Pb to constrain the nuclear symmetry energy and neutron skin thickness using both macroscopic and microscopic models, aligning experimental data with theoretical predictions.
Contribution
It provides a combined macroscopic and microscopic analysis of IVGQR in 208Pb, linking resonance energies to symmetry energy and neutron skin thickness, and offers new constraints on these nuclear properties.
Findings
Estimated symmetry energy at 0.1 fm^{-3}: 23.3 +/- 0.6 MeV
Neutron skin thickness of 208Pb: 0.14 +/- 0.03 fm
Slope parameter of symmetry energy: 37 +/- 18 MeV
Abstract
Recent improvements in the experimental determination of properties of the Isovector Giant Quadrupole Resonance (IVGQR), as demonstrated in the A=208 mass region, may be instrumental for characterizing the isovector channel of the effective nuclear interaction. We analyze properties of the IVGQR in 208Pb, using both macroscopic and microscopic approaches. The microscopic method is based on families of non-relativistic and covariant Energy Density Functionals (EDF), characterized by a systematic variation of isoscalar and isovector properties of the corresponding nuclear matter equations of state. The macroscopic approach yields an explicit dependence of the nuclear symmetry energy at some subsaturation density, for instance S(\rho=0.1 fm^{-3}), or the neutron skin thickness \Delta r_{np} of a heavy nucleus, on the excitation energies of isoscalar and isovector GQRs. Using available data…
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