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During the collapse of a star, matter becomes extremely hot and dense. Before th...

Piotr Kosek: "During the collapse of a star, matter becomes extremely hot and dense. Before the horizon closes, quantum processes may cause the star to ra..." — Pending

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📅 28.01.2026 · Czarne dziury nie istnieją? Nowa hipoteza fizyków - Ast... · 👁️ 1

Pending. The claim describes a hypothetical scenario in theoretical astrophysics where quantum processes could prevent the formation of a black hole's event horizon, causing the star to evaporate instead. This aligns with some sp...

"During the collapse of a star, matter becomes extremely hot and dense. Before the horizon closes, quantum processes may cause the star to radiate its mass so quickly that the horizon never forms. The star evaporates before becoming a black hole." "Podczas zapadania się gwiazdy materia staje się niezwykle gorąca i gęsta. Zanim horyzont się zamknie, procesy kwantowe mogą sprawić, że gwiazda wypromieniuje swoją masę tak szybko, że horyzont nigdy nie powstanie. Gwiazda wyparuje zanim stanie się czarną dziurą."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
🌐 Scenario 🔬 Technology AI confidence (unresolved): 80% Resolves by: 2031 🌐 Zanim horyzont się zamknie, procesy kwantowe mogą sprawić, ż... Assertiveness: medium 🌍 Global Source on YouTube

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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

sprawia, że czarna dziura traci masę, no i ostatecznie wyparowuje. A dlaczego masę, skoro to zakrzywienie czasoprzestrzeni? No bo masa i energia to właściwie jest jedno i to samo. A żeby zakrzywić czasoprzestrzeń, potrzebujemy energii, która jest też poniekąd masą. Brzmi dziwnie, no ale tak to właśnie wygląda. Argument sceptyków brzmi następująco. Podczas zapadania się gwiazdy materia staje się niezwykle gorąca i gęsta. Zanim horyzont się zamknie, procesy kwantowe mogą sprawić, że gwiazda wypromieniuje swoją masę tak szybko, że horyzont nigdy nie powstanie. Gwiazda wyparuje zanim stanie się czarną dziurą. Brzmi sensownie. Problem w tym, że dla dużych astrofizycznych obiektów ten efekt jest matematycznie pomijalny. Obliczenia pokazują, że utrata masy przez promieniowanie Hawkinga dla obiektu o masie gwiazdy jest absurdalnie mała w porównaniu do tempa zapadania się grawitacyjnego. To promieniowanie Hawkinga po prostu nie nadąży. Jest to jak próba opr

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