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

2009 ◽  
Author(s):  
Madappa Prakash
2016 ◽  
Vol 31 (34) ◽  
pp. 1650194 ◽  
Author(s):  
B. Behera ◽  
T. R. Routray ◽  
S. K. Tripathy

High density behavior of nuclear symmetry energy is studied on the basis of the stiffest density dependence of asymmetric contribution to energy per nucleon in charge neutral n + p + e + [Formula: see text] matter under beta equilibrium. The density dependence of nuclear symmetry energy obtained in this way is neither very stiff nor soft at high densities and is found to be in conformity with recent observations of neutron stars.


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