Expression of Interest To Perform a High-Statistics Neutrino Scattering Experiment using a Fine-grained Detector in the NuMI Beam Argonne - Athens - California/Irvine - Colorado…

Constraining the EoS and Symmetry Energy from HI collisions Statement of the problem Demonstration: symmetric matter EOS Laboratory constraints on the symmetry energy from…

Zbigniew Chajęcki National Superconducting Cyclotron Laboratory Michigan State University B. Lynch, B. Tsang, M. Kilburn, D. Coupland, M. Youngs Probing the symmetry energy…

EoS of asymmetric matter The Equation of State of Asymmetric Matter E/A (, ) = E/A (,0) + 2S()  = (n- p)/ (n+ p) = (N-Z)/A1 B.A. Brown,PRL85(2000)5296…

Progress Report Daniel Coupland Michigan State University National Superconducting Cyclotron Laboratory Constraints on the nuclear symmetry energy from transport equations…

Constraining the EoS and Symmetry Energy from HI collisions Statement of the problem Demonstration: symmetric matter EOS Laboratory constraints on the symmetry energy from…

PowerPoint Presentation Nuclear Equation of State of asymmetric matter E/A (,) = E/A (,0) + d2S() d = (n- p)/ (n+ p) = (N-Z)/A Density dependence…

PowerPoint Presentation Nuclear Equation of State of asymmetric matter E/A (,) = E/A (,0) + d2S() d = (n- p)/ (n+ p) = (N-Z)/A Density dependence…

EoS of asymmetric matter The Equation of State of Asymmetric Matter E/A (, ) = E/A (,0) + 2S()  = (n- p)/ (n+ p) = (N-Z)/A1 B.A. Brown,PRL85(2000)5296…