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Scientists Discover Way to Send Information into Black Holes Without Using Energy

A Shadow with Sharp Edges: Are We Seeing Signs of a Wormhole in Space?

In astronomy, a shadow is not just darkness. It is a powerful clue about how gravity works near extremely dense objects. When light passes close to a very strong gravitational field, its path bends. Some light escapes, and some gets trapped. To a distant observer, this creates a dark region called a shadow.

In recent years, images from the Event Horizon Telescope have shown the shadows of supermassive black holes. These images confirmed many predictions of Einstein’s theory of gravity. But black holes are not the only objects that could cast shadows. Other strange objects, such as traversable wormholes, may also leave visible shadow patterns.

In this article, we explain the work of Cheng, Xu, and Zhao. They studied the shadow of a rotating traversable wormhole and found new and surprising features—especially sharp points called cusps. These features could help scientists tell wormholes apart from black holes in the future.


What Is a Traversable Wormhole?

A wormhole is a theoretical tunnel in space and time. It connects two distant regions of the universe, or possibly even two different universes. A traversable wormhole is one that light—and in theory people or spacecraft—could pass through safely.

Unlike black holes, wormholes:

  • Do not have an event horizon

  • Do not trap everything forever

  • Can allow light to pass through the throat (the narrowest part)

Some wormholes can also rotate, just like spinning black holes. This rotation strongly affects how light moves around them.


Why Study Wormhole Shadows?

Studying wormhole shadows is important for one main reason:
👉 They may look similar to black hole shadows, but not exactly the same.

If astronomers observe a shadow that does not perfectly match black hole predictions, it could be evidence of something more exotic, like a wormhole.

Wormhole shadows help scientists:

  • Test Einstein’s gravity in extreme conditions

  • Search for alternatives to black holes

  • Understand how light behaves in strange spacetime geometries


How Does a Shadow Form?

The boundary of a shadow is controlled by photon orbits. These are paths where light moves in circles because gravity is extremely strong.

In a rotating traversable wormhole, Cheng, Xu, and Zhao found two main types of important photon orbits:

  1. Unstable circular orbits outside the throat

    • Light circles the wormhole but can escape if disturbed

  2. Critical orbits at the throat

    • Light moves right at the narrow center of the wormhole

The shadow edge is created where these two orbit families come together. This interaction is the key to understanding the strange shapes seen in wormhole shadows.


What Is a Cusp?

A cusp is a sharp, pointed feature on the edge of the shadow. It looks like a corner or spike instead of a smooth curve.

Important points about cusps:

  • They are real physical features, not errors

  • They show a sudden change in photon motion

  • They signal a transition in the shadow’s structure

Earlier wormhole studies often did not find cusps because they used very simple gravity models. Cheng, Xu, and Zhao showed that when gravity is described more realistically, cusps naturally appear.


The Redshift Parameter λ: A Key Factor

The researchers used a more general description of gravity near the wormhole. This description includes a parameter called λ (lambda).

In simple terms:

  • λ controls how quickly gravity becomes strong near the throat

  • Small λ → gentle gravity change

  • Large λ → steep gravity change

The most important discovery is a critical value of λ:

λc=514

This value is special because:

  • It is universal

  • It does not depend on how fast the wormhole spins

  • It does not depend on the size of the throat

What happens at λc?

  • If λ < λc → shadow edge is smooth

  • If λ > λc → a sharp cusp suddenly appears

This is like a phase change, similar to water freezing into ice.


Four Types of Wormhole Shadow Shapes

By changing the spin (a) and redshift parameter (λ), the researchers mapped out all possible shadow shapes. They found four main shadow types:

1. Smooth Shadow

  • Occurs at small λ

  • Shadow boundary is round and smooth

  • Can look similar to a black hole shadow

2. Cuspy Shadow

  • Appears when λ crosses the critical value

  • A sharp cusp forms on the edge

  • Strong sign of exotic spacetime

3. Ears Touching

  • Happens at higher spin

  • Shadow develops two side “ears” that touch

  • Very different from black hole shadows

4. Throat Drowning

  • The throat-related orbits disappear from view

  • Shadow shape changes dramatically

  • Dominated by outer photon paths

These shapes form a phase diagram, similar to phases of matter.


Re-Entrant Behavior: A Strange Effect

One surprising result is re-entrant behavior. This means:

  • As parameters change, the throat orbit may disappear

  • With further changes, it can reappear again

This back-and-forth behavior shows that wormhole shadows evolve in a complex and non-simple way. Black hole shadows do not show this kind of behavior.


Connection to Deep Physics

Recent research on black hole shadows shows that cusp formation is linked to:

  • Topological phase transitions

  • Changes in mathematical properties of spacetime

  • Universal physical laws

The similarities between black hole cusps and wormhole cusps suggest that the same deep physics may be at work. This makes cusps especially important for understanding gravity itself.


Why This Matters for Future Observations

Astronomy is moving fast. Future telescopes will produce even sharper images of cosmic shadows.

If scientists observe:

  • Sharp cusps

  • Ear-like extensions

  • Unusual shadow transitions

then rotating traversable wormholes could become serious candidates for what we are seeing.

Shadow shapes may allow astronomers to:

  • Measure the wormhole’s spin

  • Estimate the redshift parameter λ

  • Distinguish wormholes from black holes


Conclusion: Shadows as Cosmic Clues

The study by Cheng, Xu, and Zhao shows that rotating traversable wormholes cast rich and complex shadows. Their work reveals:

  • A universal critical value for cusp formation

  • Four distinct shadow shapes

  • Strange re-entrant behavior

  • Strong differences from black hole shadows

These discoveries deepen our understanding of exotic spacetime and open a new path for testing gravity using astronomical observations.

In the future, the dark shapes we see in the sky may tell us whether we are looking at a black hole—or a doorway through spacetime itself.

Reference: Peng Cheng, Ruo-Fan Xu, Peng Zhao, "On the Cuspy Structure of Rotating Wormhole Shadows", Arxiv, 2026. https://arxiv.org/abs/2602.14182


Technical Terms


1. Shadow (of a compact object)

A shadow is a dark shape seen against bright light coming from hot gas around a very massive object.
It forms because strong gravity bends light, and some light cannot reach the observer.
The shape of the shadow tells us how space and gravity behave near that object.


2. Compact Object

A compact object is something extremely massive but very small in size.
Examples include:

  • Black holes

  • Neutron stars

  • Wormholes (theoretical)

Because their gravity is very strong, compact objects strongly affect light.


3. Traversable Wormhole

A wormhole is a tunnel in space and time that connects two faraway places.
A traversable wormhole means:

  • Light can pass through it

  • In theory, matter could pass safely

  • It has no event horizon like a black hole

It is a prediction of Einstein’s gravity, not yet observed.


4. Throat (of a Wormhole)

The throat is the narrowest part of a wormhole.
Think of it like the middle of a tunnel.
Light passing very close to the throat behaves differently than light farther away.


5. Rotating Wormhole

A rotating wormhole is a wormhole that spins around its axis.
Rotation causes:

  • Strong twisting of spacetime

  • Different bending of light on each side

  • More complex shadow shapes

Rotation is described using a parameter called spin.


6. Spin Parameter (a)

The spin parameter, usually written as a, tells us how fast the object is rotating.

  • Small a → slow rotation

  • Large a → fast rotation

Spin strongly affects the shape of the shadow.


7. Photon

A photon is a tiny particle of light.
In strong gravity, photons do not travel in straight lines. Instead, their paths bend or curve.


8. Photon Orbit

A photon orbit is a path where light circles around a massive object due to gravity.

  • These orbits are usually unstable

  • A tiny push can make the photon escape or fall away

  • Photon orbits define the edge of the shadow


9. Unstable Circular Orbit

An unstable circular orbit means:

  • Light can move in a circle

  • But the orbit is fragile

  • Any small disturbance breaks it

These orbits are crucial in forming shadow boundaries.


10. Critical Orbit

A critical orbit is a special photon path that separates:

  • Light that escapes

  • Light that gets trapped or diverted

At the wormhole throat, critical orbits play a major role in shaping the shadow.


11. Redshift

Redshift means light loses energy and becomes “redder” when escaping strong gravity.

In simple words:

  • Strong gravity slows down time

  • Light climbing out loses energy

Redshift tells us how intense gravity is.


12. Redshift Function

The redshift function describes how gravity strength changes with distance from the wormhole.

It controls:

  • How sharply gravity increases near the throat

  • How light paths bend

Different redshift functions lead to different shadow shapes.


13. Redshift Parameter (λ – Lambda)

The parameter λ (lambda) controls the steepness of gravity near the wormhole throat.

  • Small λ → gentle gravity change

  • Large λ → very steep gravity change

This parameter is key to whether cusps appear or not.


14. Critical Value (λc)

The critical value λc is a special number where behavior suddenly changes.

  • Below λc → smooth shadow

  • Above λc → cusp appears

This is similar to water freezing at 0°C.


15. Cusp

A cusp is a sharp, pointed feature on the edge of the shadow.

Important facts:

  • It is not an error

  • It shows a sudden change in photon behavior

  • It marks a phase transition in shadow shape

Cusps are strong clues of exotic gravity.


16. Smooth Shadow

A smooth shadow has a round, continuous edge with no sharp points.
Most simple black hole shadows look smooth.


17. Cuspy Shadow

A cuspy shadow has one or more sharp points on its boundary.
This shape is harder to produce and hints at non-black-hole physics, like wormholes.


18. Phase Diagram

A phase diagram is a map that shows different behaviors depending on parameters.

Here, it shows:

  • Shadow shapes

  • As spin (a) and redshift (λ) change

It is similar to diagrams showing solid, liquid, and gas phases of matter.


19. Re-Entrant Behavior

Re-entrant behavior means something:

  • Appears

  • Disappears

  • Then appears again as parameters change

In this case, certain photon orbits vanish and later return.
This behavior is unusual and very important.


20. Throat Drowning

Throat drowning means:

  • Photon orbits near the throat stop contributing to the shadow

  • The throat becomes “hidden” in the shadow shape

This leads to a dramatic change in appearance.


21. Topological Phase Transition

A topological phase transition is a deep mathematical change in structure, not just shape.

In shadows:

  • Smooth edge → cuspy edge

  • A fundamental change in how orbits connect

This concept comes from advanced physics but shows up clearly as cusps.


22. Observational Diagnostic

An observational diagnostic is a visible feature that helps identify what kind of object we are seeing.

Cusps, ears, and strange shadow shapes act as diagnostics to:

  • Tell wormholes apart from black holes

  • Measure their properties

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