CTPA Project

Theory

Physical and mathematical foundations of Z. Zakir’s Frozar theory and the global description of relativistic gravitational collapse.

Two levels of presentation

A · Physical picture — rigorous explanation without formulas.

B · Mathematical formulation — the same physics in precise mathematical form.

1. One star — one world time

Physical picture

A collapsing star is one extended physical system. To describe its state at a given moment, one must determine where all of its layers are simultaneously. In the Frozar formulation this is done in a reference frame at rest with the source, using a single world time that labels its hypersurfaces of simultaneity.

Every layer has local physical processes — particle motion, atomic oscillations, radiation, chemical and nuclear reactions. Their local rate is expressed by the proper time of that layer. Proper times at different radii need not run at the same rate relative to world time.

World time has a different role. It is defined throughout the reference frame and tells which events at different places belong to the same global state. In an asymptotically flat system, far from the source where the field becomes negligible, its rate is synchronized with the proper time of a distant observer at rest.

Therefore the proper times of different layers cannot be chosen independently when one wants the state of one star at one moment. They must all be related to the same world time.

Mathematical formulation

Let R label a spherical layer. Its radius in the global frame is

r = r(t, R),

and its proper time is

τ = τ(t, R).

The hypersurface

t = const

defines the events that are simultaneous in this world-time description. If a local solution is first obtained as r = r(τ, R), then the global evolution is obtained only after finding τ = τ(t, R):

r(t, R) = r[τ(t, R), R].

2. Not “time slowing”, but slowing of proper times

Physical picture

The customary phrase “gravitational time dilation” or “slowing of time” is convenient, but it can obscure what is physically happening. In the Frozar framework, this terminological conflation is treated as one of the methodological sources of confusion in gravitational collapse.

The physical effect is not that an independent entity called “time” itself changes its rate. What is observed is a synchronous slowing of all local physical processes in a gravitational field relative to the chosen world time. The closer to the source and the stronger the field, the greater this slowing.

Every possible clock is only one example of such a local process. Atomic transitions, oscillations, motion of matter, radiation processes, chemical and nuclear reactions all slow by the same local relativistic factor.

A more precise expression is therefore: slowing of local proper times relative to the world time of the hypersurfaces of simultaneity.

Mathematical formulation

The rate of local physical evolution of layer R relative to world time is characterized by

∂τ(t, R) / ∂t.

Far from the source in the asymptotically flat region,

∂τ/∂t → 1.

As the gravitational field becomes stronger this factor decreases. In the limiting strong-field regime,

∂τ/∂t → 0.

For a trajectory r = r[τ(t,R),R],

∂r/∂t = (∂r/∂τ)(∂τ/∂t).

Thus, if ∂r/∂τ remains finite, the slowing of proper time implies

∂r/∂t → 0.

3. First example: a thin dust shell

Physical picture

The clearest first model is a spherical thin shell made of pressureless matter. Far from its gravitational radius the shell contracts comparatively rapidly. As it enters a stronger gravitational field, all of its local processes slow increasingly relative to world time, and so does the contraction itself.

On a world-time diagram the radial motion becomes progressively slower. The shell approaches its limiting radius ever more closely, while crossing it is pushed to ever later world-time moments. This simple model already contains the basic mechanism of frozarization.

Mathematical formulation

For a spherical shell of mass M, the gravitational radius is

rg = 2GM/c².

The global trajectory is r = r(t). In the limiting regime,

r(t) → rg,   dτ/dt → 0,   dr/dt → 0.

In the Frozar description, for every finite world time,

r(t) > rg,

while equality is reached only as an asymptotic limit.

4. From a shell to an extended star

Physical picture

A real star consists of many nested layers. For each layer, the relevant gravitational scale is determined by the mass enclosed inside that layer, not only by the total mass of the star.

Therefore different layers enter the strong-slowing regime under different local conditions. Frozarization is not confined to the visible surface: it is a layer-by-layer process involving the whole stellar structure.

The resulting object is therefore not an empty region bounded by a single frozen surface, but an ultra-compact material configuration whose internal layers are themselves strongly slowed relative to world time.

Mathematical formulation

Let m(R) be the mass enclosed inside layer R. Its gravitational radius is

rg(R) = 2Gm(R)/c².

The global state is the family

r = r(t, R).

Frozarization of each layer is characterized by

r(t,R) → rg(R),   ∂r(t,R)/∂t → 0

at large world time. The limiting structure is therefore controlled by the full distribution R ↦ rg(R), not by one radius alone.

5. The Oppenheimer–Snyder exact solution

Physical picture

A central benchmark is the exact Oppenheimer–Snyder solution for the spherical collapse of a homogeneous dust star. It describes pressureless matter without adding a mechanism that could halt the contraction.

In comoving coordinates the motion of matter is naturally expressed through local proper time. But this local description alone does not yet answer the global question: where are all layers of the star at the same moment in the source-rest frame?

To obtain that picture, the proper time of every layer must be related to the common world time. Only then can the positions of all layers be plotted on one hypersurface of simultaneity.

Mathematical formulation

In the comoving description the exact solution gives

r = r(τ, R).

The global description requires the transformation

t = t(τ, R)

and, after inversion,

τ = τ(t, R).

Hence the physical global evolution is

r(t,R) = r[τ(t,R),R].

A slice t = const intersects the world lines of different layers at different values of their proper times. Those values — not independently selected values of τ — form one global state of the star.

6. How a frozar forms

Physical picture

As collapse proceeds, proper times of the stellar layers run increasingly slowly relative to world time. Their radial evolution in world time slows at the same time.

Each layer approaches the limiting radius determined by the mass inside it. For an external description, further change becomes ever slower. The star evolves into a frozar: a relativistically collapsed material object whose internal evolution is extremely slowed relative to world time.

“Frozen” does not mean that local physics ceases in the layer’s own proper time. It means that the layer’s proper time advances asymptotically slowly relative to the global world time.

Mathematical formulation

For each layer in the limiting regime,

∂τ(t,R)/∂t → 0,

∂r(t,R)/∂t → 0,

and

r(t,R) → rg(R).

For finite world time, the Frozar description has

r(t,R) > rg(R).

7. Global structure and the gravitational radius

Physical picture

The decisive question is not merely what one freely falling observer experiences. It is the structure of the whole star on one global hypersurface of simultaneity.

In the Frozar picture all material layers remain parts of the same global configuration. The gravitational radius is essential, but it is interpreted as an asymptotic limit of the world-time evolution of the corresponding layer.

This separates two logically different questions: whether a coordinate or analytic continuation of a metric can be written beyond a surface, and whether that surface is physically formed by collapsing matter at a finite world time. Frozar theory addresses the second question.

Mathematical formulation

At fixed world time the star is represented by

R ↦ r(t,R),

with the associated proper-time distribution

R ↦ τ(t,R).

If

limt→∞ r(t,R) = rg(R)

but

r(t,R) > rg(R)

for every finite t, then r = rg(R) is an asymptotic boundary of that world-time matter evolution. This statement concerns the physical trajectories of matter and is distinct from coordinate continuation of the metric.

8. What can be observed

Physical picture

As a star approaches the frozar state, radiation from its deep gravitational field is increasingly redshifted and the observed evolution becomes slower. The object becomes extremely compact and dark, while retaining a material internal structure in the global description.

Observable differences must therefore be sought in processes sensitive to that near-limiting structure: accretion, mergers, gravitational waves, interactions with neutron stars, and the behavior of supermassive compact objects in galactic nuclei.

Each such test requires a separate quantitative model; the purpose of the theory is to identify which physical quantities must be calculated and compared with observations.

Mathematical formulation

Observational signatures must be derived from the functions

r(t,R),   τ(t,R)

and from the distribution of matter in the region

r - rg(R) ≪ rg(R).

Relevant quantities may include the dynamical response of near-limiting layers, merger waveforms, time structure of radiation and post-merger evolution. Their exact form depends on the specific metric and matter model.

Main conclusion

Physical picture

The methodological starting point is simple: the state of one star must be specified for the whole star at one and the same world time. In that description, the gravitational slowing of local proper times is accompanied by the slowing of the collapse itself. Each layer approaches its own gravitational limit asymptotically, and the star evolves into a frozar.

Mathematical formulation

The global description is the coupled system

r = r(t,R),   τ = τ(t,R),

with

r(t,R) = r[τ(t,R),R].

In the frozarization regime,

∂τ/∂t → 0,   ∂r/∂t → 0,   r(t,R) → rg(R).

Peer-reviewed publication in an international journal

The Oppenheimer–Snyder interpretation used here is presented in a peer-reviewed publication in an international journal:

On the consistency of the Oppenheimer–Snyder solution for a dust star. Reply to Marshall’s criticism
Zahid Zakir · Astrophysics and Space Science 363, Article 30 (2018) · Springer