Differential isospin-fractionation in dilute asymmetric nuclear matter
arXiv:0710.2877 · doi:10.1103/PhysRevC.76.051601
Abstract
The differential isospin-fractionation (IsoF) during the liquid-gas phase transition in dilute asymmetric nuclear matter is studied as a function of nucleon momentum. Within a self-consistent thermal model it is shown that the neutron/proton ratio of the gas phase becomes {\it smaller} than that of the liquid phase for energetic nucleons, although the gas phase is overall more neutron-rich. Clear indications of the differential IsoF consistent with the thermal model predictions are demonstrated within a transport model for heavy-ion reactions. Future comparisons with experimental data will allow us to extract critical information about the momentum dependence of the isovector strong interaction.
arXiv commentRapid Communication, Phys. Rev. C (2007) in press
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Cited by in corpus (14)
- Nuclear constraints on properties of neutron star crusts
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Thermal properties of asymmetric nuclear matter with an improved isospin- and momentum-dependent interaction
- Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
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- Can the nuclear symmetry potential at supra-saturation densities be negative?
- Isospin and momentum dependence of liquid-gas phase transition in hot asymmetric nuclear matter
- Density functional approach to finite temperature nuclear properties and the role of a momentum dependent isovector interaction