Jirina Stone

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Jirina Stone

Academic Visitor

High density matter in supernovae and neutron stars
Low energy nuclear theory and experiment
Nuclear Magnetism
Quark-Meson-Coupling model

Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA

Department of Chemistry and Biochemistry, University of Maryland, College Park, MD 20742, USA

RIKEN, Japan

Frustrated matter in core-collapse supernovae
Neutron density distribution in a unit super-cell at density ρ = 0.10 fm-3
and temperature T = 2 MeV. Created by Helena Pais September 2012.
For more information see:
http://link.aps.org/doi/10.1103/PhysRevLett.109.151101

Exploring the Nuclear Pasta Phase in Core-Collapse Supernova Matter
link.aps.org/doi/10.1103/PhysRevLett.109.151101
Constraints on the symmetry energy and neutron skins from experiments and theory
link.aps.org/doi/10.1103/PhysRevC.86.015803
Magnetic Dipole Moment of the Doubly-Closed-Shell Plus One Proton Nucleus 49Sc
link.aps.org/doi/10.1103/PhysRevLett.109.032504
Skyrme interaction and nuclear matter constraints
link.aps.org/doi/10.1103/PhysRevC.85.035201
Dark Matter, Neutron Stars, and Strange Quark Matter
link.aps.org/doi/10.1103/PhysRevLett.105.141101