2025/11/18 by Parvez, Tausif, Shankaranarayanan, S.
#FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Phenomenology (hep-ph) #High Energy Physics - Theory (hep-th)
paper · doi:10.48550/arxiv.2511.14047
We present the first exact, non-singular black hole solution in General Relativity sourced by a Dirac-Born-Infeld (DBI) scalar field. Crucially, the solution is exclusively supported by the phantom branch of the DBI action, dynamically replacing the central singularity with a regular core. The solution is asymptotically flat, possesses non-trivial scalar hair, and replaces the central singularity with a regular 2-sphere. The mechanism for singularity resolution is a dynamical kinetic stiffness -- analogous to shear thickening in non-Newtonian fluids -- which also explains the evasion of classical no-hair theorems. We show these black holes evaporate to a stable, non-singular, extremal Planck-scale relic. This provides a robust mechanism to evade standard evaporation constraints, opening a vast, previously forbidden mass window for light Primordial Black Holes to constitute dark matter. The model is testable via distinctive gravitational-wave signatures from its scalar hair.