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🇺🇸
Mar 1, 20222202.13475nucl-thUniverse15 citations
Author
Millerson, Randy
7 papers
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An overview of symmetric nuclear matter properties from chiral interactions up to fourth order of the chiral expansion
Francesca Sammarruca🇺🇸 · Randy Millerson🇺🇸
Sep 7, 20212109.01985nucl-thPRC25 citations
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🇺🇸
Jun 22, 20212106.11282nucl-thPRC21 citations
Exploring the relationship between nuclear matter and finite nuclei with chiral two- and three-nucleon forces
Francesca Sammarruca🇺🇸 · Randy Millerson🇺🇸
May 6, 20202005.01958nucl-thPRC22 citations
Temperature effects on the neutron matter equation of state obtained from chiral effective field theory
F. Sammarruca🇺🇸 · R. Machleidt🇺🇸 · R. Millerson🇺🇸
Jan 10, 20202001.02845nucl-thMod.Phys.Lett.A7 citations
Properties of isospin asymmetric matter derived from chiral effective field theory
Randy Millerson🇺🇸 · Francesca Sammarruca🇺🇸
Jun 10, 20191906.02905nucl-th5 citations
The radius of a typical-mass neutron star and chiral effective field theory
Francesca Sammarruca🇺🇸 · Randy Millerson🇺🇸
Mar 6, 20181803.01437nucl-thJ.Phys.9 citations
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