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When star matter collapses under its own weight, under its own mass, electrons s...

Piotr Kosek: "When star matter collapses under its own weight, under its own mass, electrons start rubbing against each other and resist. This resistance..." — True

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📅 22.02.2026 · Osobliwość czarnej dziury może działać inaczej. Portal... · 👁️ 8

True. The claim is true. Electron degeneracy pressure arises when electrons are forced into the same quantum states, which, according to the Pauli exclusion principle, generates resistance against further collapse. This pressu...

"When star matter collapses under its own weight, under its own mass, electrons start rubbing against each other and resist. This resistance is called electron degeneracy pressure. And it keeps white dwarfs alive. If gravity is stronger and crushes electrons with protons, neutrons are formed." "Kiedy materia gwiazdy zapada się pod własnym ciężarem, pod własną masą, elektrony zaczynają się o siebie ocierać i stawiają opór. Ten opór nazywamy ciśnieniem degeneracji elektronowej. I to ono utrzymuje przy życiu białe karły. Jeśli grawitacja jest silniejsza i zgniecie elektrony z protonami, powstają neutrony."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

Pasażerowie to fermiony, czyli cząstki materii takie jak elektrony albo neutrony. Zasada Pauliego mówi nam jasno. Dwa identyczne fermiony nie mogą zajmować dokładnie tego samego stanu kwantowego w tym samym czasie. W naszym metrze oznacza to, że dwie osoby nie mogą usiąść na tym samym fotelu, co zazwyczaj byłoby dziwne, jakby nie patrzeć. Kiedy materia gwiazdy zapada się pod własnym ciężarem, pod własną masą, elektrony zaczynają się o siebie ocierać i stawiają opór. Ten opór nazywamy ciśnieniem degeneracji elektronowej. I to ono utrzymuje przy życiu białe karły. Jeśli grawitacja jest silniejsza i zgniecie elektrony z protonami, powstają neutrony. Znowu działa zasada Pauliego. Neutrony mówią stop, ciaśniej już nie damy rady i tworzą gwiazdę neutronową. Ale jeśli masa jądra przekroczy pewną krytyczną granicę, to grawitacja staje się tak potężna, że łamie zasadę wykluczenia Pauliego. Wagon metra zostaje zgnieciony do rozmiarów atomu. Od tego momentu nie ma znanej nam siły we wszechświecie, kt

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