Information Isn’t Conserved in Black Holes
Introduction
In standard black-hole physics, the phrase “information is conserved” usually means this: if something falls into a black hole, then every detail about it—its position, momentum, quantum state, amplitudes, phases, and correlations—must still exist somehow in the final outcome, even if in a scrambled form. That idea comes from the usual quantum requirement of unitary evolution and from the black-hole information paradox created by Hawking radiation. Hawking’s original semiclassical argument suggested that black holes radiate thermally and could erase fine details, while much of modern mainstream theory tries to recover those details in a more subtle way.
This article argues that this standard way of speaking is too biased toward a hidden assumption: that momentary states are the kinds of things that can be stored. From the Absolute Medium (AM) perspective, and from the informational framework that defines information as an interaction rather than a static object, that assumption is mistaken. Information is not a frozen thing sitting somewhere in the universe. It is a realized state-change, and once realized, it belongs to the one-way arrow of change. That means it is not the sort of thing that can literally remain conserved as the same existential event.
1. The standard claim already assumes too much
The usual black-hole-information statement sounds simple: if physics is fundamentally reversible, then nothing truly disappears. So if a star, particle, or observer falls into a black hole, every detail about that infalling system must still be encoded somewhere, perhaps in the radiation, perhaps on the horizon, perhaps in some quantum-gravitational bookkeeping. This is the backbone of the modern information-paradox debate.
But that statement quietly assumes that a state at one moment is a kind of stored object. It treats things like position, phase, and correlation as though they were entries in a universal archive. The AM information framework rejects that ontology. In that framework, information is not a thing in storage; it is a state-change induced through a transaction. Without a source, channel, and sink, information does not exist as an independent object. It exists only as a realized process of synchronization.
So before asking whether information is “still there,” we must ask a more basic question:
Was information ever the kind of thing that could simply remain there?
The AM answer is: not in the static sense usually assumed.
2. Momentary states are events, not stored objects
A black hole does not swallow abstract labels. It swallows realized physical states. Those states are not eternal snapshots. They are events in the arrow of change. A position is a momentary realized relation. A phase is a momentary relational condition. A correlation is a momentary structural alignment. Every one of these belongs to a living process of becoming, not to a timeless warehouse of facts. This matches the AM view that reality consists of evolving strain, flow, persistence, and admissible transitions in the medium, not of self-standing frozen entities.
Once a moment has passed, it has passed. The universe may preserve consequences, constraints, traces, topology, or lawful structure—but the original realized moment is no longer present as the same event. That is the crucial point. The standard conservation language confuses later recoverability of structure with continued existence of the original momentary state. Those are not the same.
So when one says, “the information must still be encoded somewhere,” one is already assuming a snapshot ontology that the AM framework does not accept. In this view, the momentary state itself is not conserved. At most, the universe may preserve enough lawful structure for a later reconstruction of an equivalent form.
3. The arrow of time makes exact state conservation impossible
The deeper objection is not only that states are events rather than objects, but that they are events in a one-way sequence. Time is not just a label; it is the order of realized change. Once some state has occurred, it has already moved through the process of becoming. That means the exact realized event is not available to persist as the same event later. A later state may resemble it, reproduce it, or be generated from similar conditions, but it is still a different realization.
This matters because the standard phrase “information is conserved” often slips from formal reversibility to ontological sameness. But sameness of pattern is not sameness of event. Even if all measurable details were somehow recreated later, the recreated state would still not be the original moment of reality. It would be a fresh realization. So exact conservation of the original momentary state is already false in the deepest ontological sense.
That is why the article’s claim is stronger than merely saying “we do not know where the information goes.” It says:
The original momentary state does not remain as a conserved object at all.
What remains, if anything, is something deeper and more abstract than the state itself.
4. Entropy makes reconstruction different from conservation
There is another decisive point: entropy. Once something has happened, it has already gone through a one-way physical process that increases disorder unless actively countered. In the AM informational framework, persistence requires resolution to keep up with or exceed incompatibility generation; otherwise the system moves toward breakdown or collapse. That same logic means that once a state has passed, recreating it is not free. It requires new order, new arrangement, and new energy input.
So even if one says, “under the right conditions the state can be recreated,” that does not mean the state was conserved all along. It means a new state can be built that is structurally similar. But to do that, one must inject energy, organization, and boundary control from outside the purely forward-dissipative process. That is reconstruction, not conservation.
This is a powerful correction to the standard black-hole debate. Standard language says: if the details can reappear, they must have been stored. The AM-style objection says: no. A pattern can reappear because lawful generative structure still exists, not because the original state sat there intact waiting to be read out.
5. What really persists: generative structure
If momentary state is not conserved, then what does persist?
The strongest AM-compatible answer is:
Not the state itself, but the generative structure from which equivalent states may later be produced.
That generative structure includes:
admissible boundary conditions,
causal drivers,
topological constraints,
persistence conditions,
and the medium’s lawful capacity to produce structured forms.
This is a much deeper idea than “hidden information storage.” It says the universe does not keep a perfect museum of past moments. Rather, it preserves lawful pathways, structural classes, and admissible patterns of re-formation. In AM terms, what survives is not the exact snapshot but the persistent generative potential of the medium.
So the correct replacement for “information conservation” is something like:
Generative structure persists enough to permit conditional reconstruction of structurally equivalent states.
That is weaker than snapshot conservation, but deeper and more realistic.
6. Why this matters specifically for black holes
Now apply that to black holes.
In mainstream black-hole thermodynamics, one often says that if information is preserved, it must be hidden in the horizon area, in subtle correlations in Hawking radiation, or in some holographic encoding. Those ideas come from Bekenstein–Hawking entropy and the effort to keep quantum evolution unitary. [arxiv.org], [en.wikipedia.org], [mdpi.com]
But if the AM criticism is right, the question itself must be rewritten. The real question is not:
“Where is the original information stored?”
but:
“What lawful structure survives black-hole collapse such that prior forms could, in principle, be re-instantiated?”
That is a different problem. It shifts the focus from static storage to admissible generative persistence.
This fits especially well with the AM-UFT because that framework already rejects singular continuation. It says there is a hard boundary beyond which pathological continuation is forbidden, and when smooth continuation fails, admissibility is preserved by a topological phase transition instead. So black-hole collapse is naturally interpreted not as “information hidden forever in a singularity,” but as a reorganization of medium structure under hard-boundary and admissibility constraints.
In that picture, what survives black-hole evolution is not a perfect record of every momentary phase and position. What survives is:
topological lineage,
admissible structural constraints,
horizon or boundary organization,
and the medium’s lawful potential to generate related states later.
7. So why information isn’t conserved in black holes
Here is the argument in plain language:
Information in the usual sense refers to momentary state details—position, momentum, phases, correlations, and so on.
Those details are not static objects; they are realized events of change. In the AM informational view, information itself is state-change in a source–channel–sink process, not an independent stored entity.
Because realized moments belong to a one-way arrow of change, they do not continue to exist later as the same momentary beings.
If something like the earlier state appears again, that requires new energy, new arrangement, and new organization after entropy has already increased. That is reconstruction, not conservation.
Therefore black holes do not conserve information in the naive sense of preserving every original momentary detail as a stored object. What may persist instead is lawful, admissible, generative structure.
So the final conclusion is:
Information is not conserved in black holes if “information” means the literal persistence of momentary state details as stored reality.
What may persist is only the deeper generative structure from which equivalent patterns could, under proper conditions, later be produced.
Final closing thought
The standard black-hole information debate asks whether the universe keeps a perfect record of everything that happened. This article says that is the wrong picture. The universe is not an archive of frozen moments. It is a medium of one-way realized change. Moments do not survive as stored things. What survives—if anything—is the power of lawful structure to generate form again. That is why, in the deepest ontological sense, information is not conserved in black holes.