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Some scientists now propose that our universe might have been born inside a massive black hole within a larger parent cosmos. In their model, the universe before ours followed the same laws of physics we know today, expanding for billions of years before gravity overcame that outward push. Space began to contract, galaxies moved closer, and the cosmos collapsed toward extreme densities. Instead of ending in a singularity where physics breaks down, quantum effects pushed back against gravity, halting the collapse and triggering a cosmic rebound. That bounce could have launched our own universe’s expansion, making the Big Bang not the true beginning, but a continuation.
This idea draws on the Pauli Exclusion Principle and degeneracy pressure, which in smaller-scale examples prevent white dwarfs and neutron stars from collapsing indefinitely. The same resistance, applied on a universe-wide scale, could stop total collapse inside a black hole. Simulations suggest such a process could occur without invoking exotic new particles or forces. In this framework, the formation of our universe is a purely gravitational event, governed by the physics we already understand, just operating under extreme conditions beyond what we have directly observed.
One striking prediction is that ancient relics from the parent universe could have survived the bounce. These might include primordial black holes or neutron stars that predate our own cosmos. If detected, especially in the early universe, they could serve as evidence that a cosmic bounce occurred. The James Webb Space Telescope’s discovery of unexpectedly massive galaxies soon after the Big Bang could align with this idea, as such galaxies may have formed more easily if early black holes were already present to seed them.
Recent JWST findings on how galaxies spin across the universe may also fit the model. If confirmed, these patterns could point toward a shared origin and support the possibility that we live inside a black hole. While the concept remains controversial, it offers a potential bridge between general relativity and quantum mechanics, challenging the assumption that singularities are inevitable and suggesting that the life cycle of universes may be far more connected than we thought.
