Photon Spheres and shadow of Schwarzschild black hole on the EUP framework

This paper establishes a correspondence between the Extended Uncertainty Principle (EUP) and the Schwarzschild black hole metric to demonstrate that while the event horizon remains unchanged, increasing EUP parameters expand the photon sphere but shrink the shadow size, thereby allowing observational data from Sgr A* to constrain EUP parameters.

Hai-Long Zhen, Jian-Hua Shi, Huai-Fan Li, Yu-Bo Ma

Published 2026-03-05
📖 5 min read🧠 Deep dive

Imagine the universe as a giant, cosmic stage. For a long time, we thought we knew the rules of the show, especially when it came to the most dramatic actors: Black Holes. These are the ultimate cosmic vacuum cleaners, so heavy that not even light can escape their grasp.

In 2019, we finally took a picture of one (the famous "donut" image of M87 and later Sgr A* at the center of our galaxy). This was like finally seeing the actor's face after only hearing their voice. But now, scientists are asking: Is our script for how black holes work perfect? Or are there tiny, hidden notes in the margins that change the whole story?

This paper by Zhen, Shi, Li, and Ma is about finding those hidden notes. Here is the story in simple terms:

1. The "Fuzzy" Rules of the Universe (The EUP)

In the world of the very small (quantum mechanics), there is a rule called the Uncertainty Principle. It's like trying to take a photo of a speeding bullet; the faster it moves, the blurrier the picture gets. You can't know exactly where it is and exactly how fast it is at the same time.

Usually, this rule applies to tiny particles. But this paper asks: What if this "fuzziness" also applies to the very large, like the whole universe?

The authors use a concept called the Extended Uncertainty Principle (EUP). Think of it as a cosmic "graininess" in the fabric of space itself. Just like a digital photo looks smooth from far away but is made of tiny pixels up close, the universe might have a fundamental "pixel size" that we haven't noticed yet.

2. Rewriting the Black Hole's "Recipe"

Black holes are usually described by a mathematical recipe called the Schwarzschild metric. It tells us how space bends around the hole.

The authors realized that if you change the "temperature" of a black hole (how hot it glows due to quantum effects) using this new "grainy" EUP rule, you have to rewrite the recipe for how space bends.

  • The Analogy: Imagine a trampoline with a bowling ball in the middle. The fabric curves down. The standard recipe says exactly how deep that curve is. The authors say, "Wait, if the trampoline fabric is made of a slightly different, 'grainier' material (EUP), the curve changes shape."

3. The Three Key Players: The Horizon, The Photon Sphere, and The Shadow

To understand what changed, we need to know three things about a black hole:

  1. The Event Horizon: The "Point of No Return." Once you cross this invisible line, you can't get out.
    • The Paper's Finding: Even with the new "grainy" rules, this line stays exactly where it is. The black hole's size doesn't change.
  2. The Photon Sphere: A ring of light circling the black hole. It's like a racetrack where light runs in circles before either falling in or escaping.
    • The Paper's Finding: With the EUP "graininess," this racetrack moves outward. The light has to run a wider circle.
  3. The Shadow: The dark circle we see in photos. It's the "silhouette" of the black hole against the bright background.
    • The Paper's Finding: Here is the twist! Even though the light ring (photon sphere) got bigger, the dark shadow actually got smaller.

4. The Magic Trick: Why did the shadow shrink?

This is the most surprising part. Usually, if you make the ring of light bigger, you'd expect the shadow to get bigger too. But here, the "graininess" of the universe acts like a weird lens.

  • The Analogy: Imagine you are looking at a lighthouse through a foggy window.
    • Standard physics: The light beam spreads out, and the dark area behind it is big.
    • EUP physics: The "fog" (the uncertainty) bends the light in a way that makes the dark area behind the lighthouse look smaller, even though the light beam itself is wider.

The authors call this an "optical shift." The universe is playing a trick on our eyes.

5. Checking the Script Against Reality (Sgr A*)

The authors didn't just do math; they checked it against real data. They looked at the black hole at the center of our galaxy, Sagittarius A* (Sgr A*), using the Event Horizon Telescope (EHT).

They asked: "How much 'graininess' (EUP parameter) can we have before our math stops matching the photo?"

  • The Result: They found that the "graininess" can't be too strong. If it were, the shadow would look different than what the telescope saw.
  • The Constraint: They set a new limit on how "fuzzy" the universe can be. It's like saying, "The pixels in the universe's photo can only be this small, or else the picture of the black hole wouldn't match what we see."

Summary: What Does This Mean for Us?

This paper is a detective story. The authors took a theoretical idea (that the universe is "grainy" at a fundamental level), applied it to black holes, and saw how it changed the way light behaves.

  • The Good News: The black hole's "size" (horizon) is stable.
  • The Weird News: The way light orbits and the size of the shadow change in a counter-intuitive way (bigger orbit, smaller shadow).
  • The Big Picture: By comparing their math to the actual photos of black holes, they are helping us test the laws of physics. They are essentially using black holes as giant laboratories to see if our understanding of space, time, and uncertainty is correct.

If future telescopes see a black hole shadow that is slightly smaller than Einstein predicted, it might mean we finally found the "pixels" of the universe!