Evolution of Black Holes

Black holes are famous for being mysterious. They pull in everything, even light. For decades, physicists have argued about one big question: Do black holes last forever, or do they eventually vanish? 

A new idea, coming from an alternative view of Cosmos called the Absolute Medium (AM) Model, offers a surprisingly clear and beautiful answer. To understand it, we first have to change how we picture space itself. 

Imagine that what we call “empty space” is actually filled with an invisible, elastic medium – like a giant, stretchy fabric or a silent ocean. This is the core of the AM model. Everything we see – matter, light, gravity – is just a pattern or a disturbance in this medium. 

So stars, planets, and even you and me are not solid little things. They are movements and tensions inside a universal, living net.

What Is a Black Hole in This Picture? 

In the AM model, a black hole is not a “hole” at all. It is a region where the medium has been stretched to its absolute limit.
There is a special number, called ε (epsilon). It measures how stressed the medium is. 

When a region reaches ε = 1, everything freezes. Motion stops. Change stops. The system becomes a frozen knot of energy. That is the black hole. 

Two Ways to Think About What Happens Next 

For a long time, scientists thought such a frozen knot would stay frozen forever – like a perfect, eternal sculpture. But the AM model opens another possibility: Maybe the knot cannot stay frozen forever if it becomes too large. 

Think of a rubber band. A small rubber band can be stretched tight and remain strong. But if you make it bigger and bigger, eventually it loses its tension. It becomes loose and unstable. The same happens with black holes.

Article: https://doi.org/10.5281/zenodo.20184582

The Surprising Secret: Big Black Holes Are Actually Less Dense 

Here is the counter‑intuitive part. When a black hole grows by swallowing stars or merging with other black holes, its density – how tightly the medium is packed – actually goes down. Yes, a very big black hole is much less dense than a small one. 

At some point, a supermassive black hole becomes so large that its internal density drops below a critical threshold. The frozen structure can no longer hold itself together. It becomes unstable. 

The Great “Identity Transition” 

Instead of staying frozen forever, the black hole undergoes a terminal identity transition. 

That fancy phrase simply means: the system stops being a black hole and begins a new life as something else. It does not explode. It does not disappear in a flash. It slowly releases its stored energy, like a tight knot gradually loosening over billions of years. 

What emerges is not a point of no return, but a slowly relaxing strain field – a gentle, spread‑out wave in the cosmic medium. 

In physics language, the black hole transforms from a frozen L∞ state into a dynamic L² state – from a rigid, dead object into a living, breathing field. 

What Would We Observe? 

If this idea is correct, we should be able to see evidence in the universe. 

A Deeper Lesson About Nature 

This theory shows us something profound: Nothing in the universe stays frozen forever if it can no longer remain consistent.
When a system reaches its absolute limit, it does not break into chaos. It reorganizes into something new. 

Small black holes remain frozen and stable – they are the “eternal” ones. But very large black holes must transform and dissipate. They are not permanent monuments; they are just a phase in a cosmic cycle. 

Final Thought 

Black holes are not the end. They are not the final resting place of matter and energy. Instead, they are part of an ongoing, universal process: 

The universe is not a museum of frozen objects. It is a continuous story of change, resilience, and rebirth. And black holes – the most mysterious of all – may be its most powerful storytellers.