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Constraining the density dependence of the symmetry energy in the nuclear equation of state using heavy ion beams
D. V. Shetty, S. J. Yennello, G. A. Souliotis
The density dependence of the symmetry energy in the equation of state of asymmetric nuclear matter (N/Z 1) is important for understanding the structure of systems as diverse a…
Symmetry Energy, Temperature, Density and Isoscaling Parameter as a Function of Excitation energy in A 100 mass region
D. V. Shetty, S. J. Yennello, G. A. Souliotis +4
The symmetry energy, temperature, density and isoscaling parameter, in Ni + Ni, Fe + Ni and Fe + Fe reactions at beam energies of 30, 40 a…
Neutron to proton ratios of quasiprojectile and midrapidity emission in the Zn + Zn reaction at 45 MeV/nucleon
D. Theriault, J. Gauthier, F. Grenier +18
Simultaneous measurement of both neutrons and charged particles emitted in the reaction Zn + Zn at 45 MeV/nucleon allows comparison of the neutron to proton ratio at…
Reply to ``Comment on `Symmetry energy and the isospin dependent equation of state' "
D. V. Shetty, S. J. Yennello, A. S. Botvina +7
We show that the large sequential decay corrections obtained by Ono {\it et al} [nucl-ex/0507018], is in contradiction with both the other dynamical and statistical model calculati…
Properties of the Initial Participant Matter Interaction Zone in Near Fermi-Energy Heavy Ion Collisions
J. Wang, T. Keutgen, R. Wada +34
The sizes, temperatures and free neutron to proton ratios of the initial interaction zones produced in the collisions of 40 MeV/nucleon Ar + Sn and 55 MeV/nucleon$^{…
Comment on Breakup Densities of Hot Nuclei
V. E. Viola, K. Kwiatkowski, S. J. Yennello +1
In [1,2]the observed decrease in spectral peak energies of IMFs emitted from hot nuclei was interpreted in terms of a breakup density that decreased with increasing energy. Subsequ…