activity
20182022
most citedExploring the relationship between nuclear matter and finite nuclei with chiral two- and three-nucleon forces

23 citations · 59 across the 4 of their papers we have counts for

collaborators

6 papers

nucl-th202214 cited

The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star

Francesca Sammarruca, Randy Millerson

We report neutron star predictions based on our most recent equations of state. These are derived from chiral effective field theory, which allows for a systematic development of n…

nucl-th202120 cited

Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory

Francesca Sammarruca, Randy Millerson

We present predictions for the neutron matter equation of state, from leading to fourth order of chiral effective field theory, using recently developed, accurate chiral nucleon-nu…

nucl-th202023 cited

Exploring the relationship between nuclear matter and finite nuclei with chiral two- and three-nucleon forces

Francesca Sammarruca, Randy Millerson

We address the connection between the saturating behavior of infinite nuclear matter and the description of finite nuclei based on state-of-the-art chiral two- and three-nucleon fo…

nucl-th2020

Temperature effects on the neutron matter equation of state obtained from chiral effective field theory

F. Sammarruca, R. Machleidt, R. Millerson

Temperature effects on the neutron matter equation of state are investigated in the framework of chiral effective field theory. Latest, state-of-the-art chiral two-nucleon forces a…

nucl-th20192 cited

Properties of isospin asymmetric matter derived from chiral effective field theory

Randy Millerson, Francesca Sammarruca

We present and discuss properties of isospin asymmetric matter whose equation of state is derived from recent high-quality chiral nucleon-nucleon potentials and chiral effective th…

nucl-th2018

The radius of a typical-mass neutron star and chiral effective field theory

Francesca Sammarruca, Randy Millerson

We calculate neutron star masses and radii from equations of state based on recent high-quality chiral nucleon-nucleon potentials up to fifth order of the chiral expansion and the…