Nuclear symmetry energy from nuclear observables by Prof. B.K.Agrawal from Saha Institute of Nuclear Physics (Kolkata) /iTHES visitor
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Asia/Tokyo
201 (RIBF Conference Hall, RIBF building)
201
RIBF Conference Hall, RIBF building
Description
Title:
Nuclear symmetry energy from nuclear observables
Abstract:
The nature of equation of state for the neutron star matter is crucially governed by the density dependence of the nuclear symmetry energy. The density content of nuclear symmetry energy remains yet poorly constrained. I would present our recent results on the density content of the nuclear symmetry energy around the saturation density extracted using accurately known nuclear observables such as nuclear masses, iso-vector giant resonances and neutron-skin thickness in heavy nuclei.
