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Author Tews, Ingo ♦ Lattimer, James M. ♦ Ohnishi, Akira ♦ Kolomeitsev, Evgeni E.
Source United States Department of Energy Office of Scientific and Technical Information
Content type Text
Language English
Subject Keyword ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ♦ ASTROPHYSICS ♦ DENSITY ♦ EQUATIONS OF STATE ♦ HEAVY ION REACTIONS ♦ HEAVY IONS ♦ NEUTRON STARS ♦ NEUTRON-RICH ISOTOPES ♦ NUCLEAR MATTER ♦ NUCLEAR PHYSICS ♦ SATURATION ♦ SIMULATION ♦ SUPERNOVAE ♦ SURFACES ♦ SYMMETRY ♦ THICKNESS
Abstract We propose the existence of a lower bound on the energy of pure neutron matter (PNM) on the basis of unitary-gas considerations. We discuss its justification from experimental studies of cold atoms as well as from theoretical studies of neutron matter. We demonstrate that this bound results in limits to the density-dependent symmetry energy, which is the difference between the energies of symmetric nuclear matter and PNM. In particular, this bound leads to a lower limit to the volume symmetry energy parameter S {sub 0}. In addition, for assumed values of S {sub 0} above this minimum, this bound implies both upper and lower limits to the symmetry energy slope parameter L , which describes the lowest-order density dependence of the symmetry energy. A lower bound on neutron-matter incompressibility is also obtained. These bounds are found to be consistent with both recent calculations of the energies of PNM and constraints from nuclear experiments. Our results are significant because several equations of state that are currently used in astrophysical simulations of supernovae and neutron star mergers, as well as in nuclear physics simulations of heavy-ion collisions, have symmetry energy parameters that violate these bounds. Furthermore, below the nuclear saturation density, the bound on neutron-matter energies leads to a lower limit to the density-dependent symmetry energy, which leads to upper limits to the nuclear surface symmetry parameter and the neutron-star crust–core boundary. We also obtain a lower limit to the neutron-skin thicknesses of neutron-rich nuclei. Above the nuclear saturation density, the bound on neutron-matter energies also leads to an upper limit to the symmetry energy, with implications for neutron-star cooling via the direct Urca process.
ISSN 0004637X
Educational Use Research
Learning Resource Type Article
Publisher Date 2017-10-20
Publisher Place United States
Journal Astrophysical Journal
Volume Number 848
Issue Number 2


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