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The multifaceted role of the density dependent nuclear symmetry energy in thenuclear astrophysics involving neutron stars is highlighted. Efforts toward amodel independent determination of the dense matter equation state through adeconstruction of the neutron star structure equation utilizing the masses andradii of several individual neutron stars are described. The need forobservational data of both measurements for the same star is stressed.

The Pervasive Role of the Nuclear Symmetry Energy in the Structure and Evolution of Neutron Stars