Symmetry energy from nuclear multifragmentation
arXiv:1301.5615 · doi:10.1103/PhysRevC.87.011602
Abstract
The ratio of symmetry energy coefficient to temperature is extracted from different prescriptions using the isotopic as well as the isobaric yield distributions obtained in different projectile fragmentation reactions. It is found that the values extracted from our theoretical calculation agree with those extracted from the experimental data but they differ very much from the input value of the symmetry energy used. The best possible way to deduce the value of the symmetry energy coefficient is to use the fragment yield at the breakup stage of the reaction and it is better to use the grand canonical model for the fragmentation analysis. This is because the formulas that are used for the deduction of the symmetry energy coefficient are all derived in the framework of the grand canonical ensemble which is valid only at the break-up (equilibrium) condition. The yield of "cold" fragments either from the theoretical models or from experiments when used for extraction of the symmetry energy coefficient using these prescriptions might lead to the wrong conclusion.
6 pages, 4 figures
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- Heavy-ion Collisions: Direct and indirect probes of the density and temperature dependence of Esym
- Effect of particle fluctuation on isoscaling and isobaric yield ratio of nuclear multifragmentation
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- Isospin dependent hybrid model for studying isoscaling in heavy ion collisions around the Fermi energy domain
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- Intermediate Mass Fragment Emission in S +V, Ag, and U Collisions at E~=~31.6~MeV~A