A Complete, Non-Singular Spacetime in General Relativity

The Penrose-Hawking singularity theorems suggest that, under physically reasonable assumptions, the formation of singularities in General Relativity is inevitable. We present an exact, static, spherically symmetric solution to the Einstein Field Equations that is geodesically complete and free from singularities, yet satisfies the Null, Weak, Dominant, and Strong Energy Conditions.