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The main aim of the thesis is to study the properties of nuclear matter,i.e., finite nuclei to infinite nuclear matter, at zero and finite temperaturewithin effective field theory motived relativistic mean-field model by usingsome of the recent parameter sets. For this, we have chosen exotic, superheavy,and natural/neutron-rich thermally fissile nuclei and studied ground as well asexcited-state bulk and surface properties of nuclei. We have also tried tofigure out the possible constraints on the DM variables by considering WIMP, aDM candidate, inside the NS core and using gravitational-wave data GW170817.

A Systematic Study Of Nuclear Matter: Finite Nuclei To Neutron Star