Quantum mechanical (QM) degeneracy pressure resists gravitational collapse in stars, but the immense mass of a star can ultimately overcome this pressure. The Pauli Exclusion Principle (PEP) remains valid, preventing electrons from losing heat and reaching a ground state. However, if gravity generates sufficient energy to make electrons relativistic, they can occupy a ground state without a defined radius, allowing for significant contraction. This process can be exacerbated by neutronization, which reduces kinetic energy through neutrino escape. Ultimately, gravity can collapse a star's core without violating the PEP, highlighting the complex interplay between these forces.