Simple

Information — The Shadow of What Never Was ⚡ экспресс

Original: "Information Is Not Physical: Possibility Spaces, Erasure, and the Structure of Unrealized Alternatives"
· Madhurendra Mishra
arXiv:2606.15120 · 2026-06-13 · CC BY · ⏱ 1 min · History and Philosophy of Physics Quantum Physics
Physicists have proposed a new view: information is not a substance, but the shadow of all possible events.
Abstract

Information is like the shadow of all the paths we didn't take. The article argues that it’s precisely the unrealized alternatives that give meaning to what actually happened—and even have physical consequences (for instance, erasing data heats up a computer). So, maybe reality isn’t just what is, but also what isn’t?

Links in the knowledge graph 1

Erasing even a single bit means releasing heat. This discovery by Rolf Landauer hinted that information is neither material nor illusory. Imagine that every event casts a shadow—that is information, the collection of all unrealized possibilities. When you pick a key for a lock, the shadow of the other keys hangs in the air of your choice. Forgetting which key goes where extinguishes that shadow, and the world warms up ever so slightly.

Information is the shadow of what could have happened but didn’t.

With black holes, it’s the same story. Falling into one, an object loses not just its substance—it’s stripped of the history of its unrealized versions. One might think the shadow vanishes forever. But Jacob Bekenstein and Stephen Hawking proved otherwise. A black hole has entropy (a measure of disorder), and therefore it has information. Perhaps it returns to the world through spacetime curvature, which itself dictates which events are fated to occur. Thus, the shadows of the past define the boundaries of the future.

🎯 Erasing a single bit heats the environment by 10^-23 degrees. Over a year, all the data centers on Earth collectively release exactly as much heat from this as is needed to boil just one chicken egg.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole entropy spacetime curvature
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2606.15120 · CC BY · bridge42worlds