Happy 100-year birthday, quantum mechanics.
The GIF above this text introduces field interaction. When the outside field pushes the inner field, the inner field’s or structures' size will turn smaller. Until the pressure or energy level in it can break that process. Or the pressure or energy level turns so high that it can resist the outside field.
It’s 100 years of quantum mechanics. In 1925, young scientists named Werner Heisenberg went to Helgoland Island and developed the concept of quantum mechanics. In Helgoland, he realized that all things in the universe are in interaction. There, that person realized that the sky is blue because some kind of particles hit it.
And then that thing caused shockwaves that we see as blue light. The blue light is so-called Cherenkov radiation. That radiation forms when a particle that travels speed of light hits the atmosphere. Those particles must slow their speed because the speed of light is lower in the atmosphere than outside the atmosphere.
When a particle slows its speed, it must transfer its kinetic energy into its environment. When a particle hits the atmosphere. It sends a shockwave. The shockwave that we see as a photon is the thing that slows the particle's speed. When we think that the universe and all other systems are growing entropy, that means. We see that chaos is increasing in the system. But then we must wake up and make one decision.
If the system is limited, any phenomena in it cannot be unlimited. And then we can see that entropy is not literally “chaos”. It's the thing that might look like chaos. But there can be repeating structures. Like in fractals. If researchers can someday find the order in the system’s entropy, they can calculate changes in its shape backward. And if those calculations are made right, they can uncover the shape of the original system.
That makes this type of thing interesting. When a particle travels through the universe, it collects information from its environment. That information is on the particle like plague. And the problem is that. We cannot touch the particle. But if we could see the shape of the information that forms hills and potholes on the particle’s shell. If researchers know the route and entire systems. If the particle passes, it makes it possible to reorder that information. The problem is that near all stars, molecular nebulae, X- and gamma-ray bursts, and all other things involve quantum systems.
The quantum fields in those systems are unique. And that makes this model theoretical. But if researchers know everything about the particle’s route. They could restore information and see what things look like in that particle’s route. If that kind of thing is possible. That makes the quantum network possible. Data travels in a quantum network connected to particles. And if researchers can protect the data and calculate it back in the form. Where information was at the beginning of the particle’s journey. It allows sending bottle-post where information is stored in electrons.
The ability to remove entropy. Makes it possible to see distant objects. And it can also allow researchers to transport information from the past to the future. Or from the future to the past. The black hole is the thing that can transport information from the future to the past. But the problem is that the entropy at the edge of the event horizon turns information into a mess that nobody understands.
That entropy is like a series of whirls that mix information into a form. That makes no sense. But if researchers know how that border behaves and what kind of whirls there are. That allows them to re-order that information. That requires complete knowledge of the systems. And how those things behave in interaction.
