Kdy se fyzika přestala ptát a začala vymýšlet

Foreword

This text is not a critique. It is a tribute to those who asked the right questions — and an obituary for the habit that died after them.

Newton (1687)

Gravity. One force, one law, the entire universe.

F = GMm/r².

So simple we still use it today. We send probes to Pluto, land on comets, navigate satellites — Newton. Three hundred and forty years and it still works.

He didn't say why gravity exists. He said how it behaves. And that was enough for three centuries of physics.

We still calculate with Newton. In the conventional model and in ours. That says something.

F = GMm/r² — 340 years and still works. In the conventional model and in ours

Mendeleev (1869)

He faced chaos. Sixty known elements, no order, no system.

He did something brilliant: arranged the elements by mass, noticed the periodicity, and — this is the key — left empty spaces. He said: something is missing here. I don't know what. But I know what properties it will have.

Gallium was discovered six years later. Exactly where he left the gap.

Mendeleev saw order in nature before the tools to understand it existed. He didn't know why the periodicity existed — he had no quantum mechanics, no orbitals, no electron configuration. He saw a pattern and trusted it. That takes courage.

Mendeleev left empty spaces in his table — and was right. He saw the pattern before the tools to understand it existed

Einstein (1905–1915)

Two contributions that changed everything. And both remain misunderstood to this day — paradoxically by those who cite him most.

First: A body curves spacetime.

This is not abstract mathematics. It is a direct statement: where there is mass, space is different from where there is no mass. Every star, every galaxy, every cluster changes the geometry of its surroundings.

This is the definition of an inhomogeneous universe. Einstein said this in 1915.

And what did cosmology do? It took his equations and said: but at large scales, the universe is homogeneous. The cosmological principle. We smooth out everything — filaments, voids, clusters — and calculate with averages.

They took Einstein's theory and the first thing they did was deny its fundamental consequence.

Second: E = mc².

Energy is mass. Mass is energy. They are two sides of the same coin.

And what did astrophysics do? When calculating galaxy rotation curves, it adds up mass. Stars, gas, dust. Visible matter.

But Einstein said that energy is mass. Every photon, every magnetic field, every cosmic ray, all kinetic energy, all radiation — all of it contributes to gravity. E = mc² doesn't just mean bombs work. It means that when calculating a galaxy's gravity, you must account for all energy, not just what you see in the telescope as stars.

They ignore half of Einstein's own equation and then wonder why mass is missing. And instead of going back to E = mc² and calculating the whole thing, they invent dark matter.

Einstein would weep.

Cosmology denied both fundamental consequences of Einstein's theory — the inhomogeneity of space and the mass-energy equivalence — then wondered why its equations didn't work

Hawking (1974)

A brilliant mathematician. Perhaps the best modern physics has had.

He showed that black holes aren't black — they radiate. They have temperature. They evaporate. He connected quantum mechanics with gravity at the event horizon and opened an information paradox that remains unsolved.

He wasn't afraid to break what he himself helped build.

But — and here is the tragedy — he worked within the conventional model. He had the mathematical tools to see further. But the framework he moved within held him back. He calculated within boundaries he didn't set himself.

A victim of genius imprisoned by paradigm.

Hawking had the tools to see further — but the paradigm of the conventional model held him within boundaries he didn't set himself

Feynman

And then someone came along who looked at it all differently.

Path integrals. A particle doesn't go from point A to point B by one path. It goes by all paths simultaneously. Each path has its amplitude, its phase. And reality — what we observe — is the sum of information from all paths.

This is not probability like rolling dice. This is the informational structure of reality.

Feynman didn't say: the world is random and we calculate probabilities. He said: the world is complete and we only see a projection. Every experimental result is a shadow of a whole we cannot observe directly — but we can calculate it.

And then he said something even more important: 'If you can't explain it simply, you don't understand it yourself.'

Try to simply explain dark matter. Dark energy. Inflation. The multiverse.

You can't. Because nobody understands them.

Feynman opened the door to the informational layer of reality. To understanding that beneath matter, beneath energy, beneath forces, there is something more fundamental. Structure. Geometry. Information.

That's where we want to get.

Feynman opened the door to the informational layer of reality — beneath matter, energy, and forces lies structure, geometry, information

What Happened Next

This is where the story breaks.

Zwicky (1933)

Galaxies in the Coma cluster were rotating too fast. It doesn't add up.

Reasonable hypothesis: there is matter there that we can't see yet.

That was ninety years ago. We still can't see it.

Rubin (1970s)

Galaxy rotation curves. Stars at the edges rotate too fast. Systematically. Everywhere.

Instead of someone going back to Einstein and calculating all the energy — they added more invisible matter. Around every galaxy. Five times more than everything visible.

Perlmutter, Schmidt, Riess (1998)

The universe is expanding and accelerating. Nobel Prize for the observation. Deserved.

Interpretation: we add dark energy. Seventy percent of the universe. Nobody knows what it is.

Inflation (1981)

The universe is too flat. Solution: in the first 10⁻³⁶ seconds, the universe expanded exponentially. Driven by a field nobody has observed and which vanished without a trace.

Multiverse (2000s)

The cosmological constant is too precisely tuned. Solution: there exist 10⁵⁰⁰ different universes.

That is no longer physics. That is resignation.

The Pattern

Newton: observation → simple law → works for 340 years.

Mendeleev: chaos → order → empty spaces → confirmation.

Einstein: contradiction → change of perspective → simpler theory.

Hawking: paradox → new mathematics → open questions.

Feynman: new perspective → informational structure → path to understanding.

Dark matter: doesn't fit → add something invisible → 90 years of searching → nothing.

Dark energy: doesn't fit → add something invisible → we don't know what it is.

Inflation: doesn't fit → add something invisible → vanished without a trace.

Multiverse: doesn't fit → add 10⁵⁰⁰ invisible things → cannot be tested.

See the pattern?

Before: something doesn't fit → change the perspective → simpler equations.

After: something doesn't fit → add an invisible thing → more complex model.

The break in physics: from 'change perspective → simpler equations' to 'add something invisible → more complex model'

Over Coffee

Newton, Mendeleev, Einstein, Hawking, Feynman.

Five people whose work underlies everything we do. Each of them took a step without which the next one couldn't begin. Newton gave the law. Mendeleev gave order. Einstein gave perspective. Hawking gave mathematics. Feynman gave information.

I would go for coffee with each of them. And I would ask each one question:

To Newton: Why does gravity work, not just how?

To Mendeleev: Did you know that periodicity goes much further than elements?

To Einstein: Did you look at the full equation? Really the full one?

To Hawking: What would you calculate if you didn't have to follow the rules?

To Feynman: How far does that informational layer go?

Newton would answer with an equation. Mendeleev would smile. Einstein would pause to think. Hawking would write a new theory. Feynman would say: 'Shut up and calculate.'

Some of us are calculating.

Newton gave the law, Mendeleev gave order, Einstein gave perspective, Hawking gave mathematics, Feynman gave information — and some of us keep calculating

Where We Meet Standard Physics

Kuhn (1962) described paradigm shifts. Hossenfelder (Lost in Math, 2018) critiques aesthetically motivated physics. Smolin (The Trouble with Physics, 2006) warns of stagnation. The last fundamental discovery confirmed by experiment -- the Higgs boson (2012). Since then: no new signal at the LHC. Supersymmetry not found. Extra dimensions not found.