Cancelled: Microscopic Calculations of Homogeneous and Inhomogeneous Neutron Matter (The 42nd Nuclear Theory Seminar)
by
DrStefano Gandolfi(LANL/JUSTIPEN)
→
Asia/Tokyo
201 (RIBF Hall)
201
RIBF Hall
Description
The 42nd Nuclear Theory Seminar by Stefano Gandolfi (LANL/JUSTIPEN)
has been CANCELED because of cancel of his trip to Japan.
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Recent advances in experiments of the symmetry energy of nuclear
matter and in neutron star observations yield important new insights
on the equation of state of neutron matter at nuclear densities.
In this regime the EOS of neutron matter plays a critical role in
determining the mass-radius relationship for neutron stars. We show how
microscopic calculations of neutron matter, based on realistic two- and
three-nucleon forces, make clear predictions for the relation between
the isospin-asymmetry energy of nuclear matter and its density
dependence, and the maximum mass and radius for a neutron star.
On the other side, the properties of inhomogeneous neutron matter at low
to moderate densities are very important to describe the neutron star
crust, and we show how microscopic calculations of confined neutrons can
put severe constraints on density functionals commonly used to describe
heavy nuclei and the crust.