Neutron stars are created due to the cataclysmic merger of two superdense\nstellar corpses. It is now evident that neutron-star smash-ups are the source\nof much of the universeâ??s gold platinum, uranium and other heavy elements.\nHeavy elements contain large neutron excess and thus, neutron energy pairing\nwill play a very important role in the creation of such heavy element. Using\ntheoretical considerations and the results of experimental observations,\nsome important properties of neutron stars such as radius (R), the speed of\nsound inside the neutron star (Cs), the surface speed (Vs) and the most stable\nisotopes in the neutron star have been determined. The calculated values are\ncompared with the values known so far.
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