  Theoretically, it has been proposed that objects traveling radially along
regular black holes (RBHs) would not be destroyed because of finite tidal
forces and the absence of a singularity. However, the matter source allows the
creation of an inner horizon linked to an unstable de Sitter core due to mass
inflation instability. This inner horizon also gives rise to the appearance of
a remnant, inhibiting complete evaporation. We introduce here a $d$-dimensional
black hole model with Localized Sources of Matter (LSM), characterized by the
absence of an inner horizon and featuring a central integrable singularity
instead of an unstable de Sitter core. In our model, any object tracing a
radial and timelike world-line would not be crushed by the singularity. This is
attributed to finite tidal forces, the extendability of radial geodesics, and
the weak nature of the singularity. Our LSM model enables the potential
complete evaporation down to $r_h=0$ without forming a remnant. In higher
dimensions, complete evaporation occurs through a phase transition, which could
occur at Planck scales and be speculatively driven by the Generalized
Uncertainty Principle (GUP). Unlike RBHs, our model satisfies the energy
conditions. We demonstrate a linear correction to the conventional area law of
entropy, distinct from the RBH's correction. Additionally, we investigate the
stability of the solutions through the speed of sound.
