A singularity-free black hole model and its cosmological implications

We introduce a singularity-free black hole model based on a “Higgs-Buffer Zone” (HBZ), a 10 15 K central stellar core region where the Higgs field becomes inactive upon its collapse thus restoring electroweak symmetry. Grounded in the Standard Model, black hole interiors are treated as concentric layered spherical shells of distinct matter phases, including a solidlike hadron encompassing a perfect fluidlike quark‐gluon plasma shell encompassing a photon gaslike HBZ. Gravitational compression drives “evaporation” at the quark‐gluon plasma shell’s inner boundary. This phase transition due to external pressure causes the incompressible HBZ to expand (akin to a “negative pressure”), which halts singularity formation. Beyond stabilizing black holes, the HBZ model sheds light on early universe phenomena. Quantum fluctuations during the electroweak epoch could have triggered HBZ regions, driving bubble nucleation processes that influence primordial black hole formation, cosmic structure growth, and domain wall dynamics. The model also hints at gravitational wave signatures, cosmic microwave background anomalies, and possibly a novel mechanism for baryogenesis through CP-violating dynamics at HBZ boundaries. Furthermore, the HBZ’s effective negative pressure parallels inflationary cosmology, potentially acting as a complementary or secondary inflationary mechanism, linking black hole physics to dark energy or suggesting a possible compatibility with the Timescape model.