Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
The neutrino emission from thermal processes in very massive stars in the local universe
Shell model calculations of nuclear structure in "Island of inversion" N=20 region: Mg32-36 isotopes
Symmetry energy and neutron pressure of finite nuclei using the relativistic mean-field formalism
Evolution of solar-like stars. HA Kassim, N Yusof, M Idris and ZA Motahar
Analysis of cross sections using various nuclear potential
Fate of most massive stars
An Improved Reaction Rate Formulation for Charged-Particle Induced Thermonuclear Reaction of 2H(d,gamma)4He
Radiation Damage Study in Natural Zircon Using Neutrons Irradiation
