“…It is therefore that one rely on theoretical modeling of proto-neutron star matter (PNSM) to understand its composition and compute the EoS on its basis. A lot of work has been done in this regard to comprehend successfully the temperature dependence of nuclear matter properties [3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23] using a wide variety of approaches. Based on microscopic treatments, two and three body nuclear potentials were constructed using chiral effective theory [24,25] to compute the nuclear matter properties at finite temperature while nuclear dipolar strength was successfully calculated by adopting finite-temperature relativistic time blocking approximation [26].…”