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Currently, these are the ultra-short gravitational waves, those associated preci...

Piotr Kosek: "Currently, these are the ultra-short gravitational waves, those associated precisely with merging neutron stars, black holes, and so on. Yes..." — True

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📅 02.02.2026 · Einstein wątpił w ich istnienie. Dowód mniejszy niż 1/1... · 👁️ 3

True. Currently observed gravitational waves are indeed associated with merging neutron stars and black holes. The merger and ringdown phases of these events, which generate the strongest signals, last from a few to tens of mi...

"Currently, these are the ultra-short gravitational waves, those associated precisely with merging neutron stars, black holes, and so on. Yes, these are precisely those gravitational waves, and these are precisely on the order of milliseconds." "Obecnie to są te ultra krótkie fale grawitacyjne, te związane właśnie z ze zlewającymi się gwiazdami neutronowymi, czarnymi dziurami i tak dalej. Tak, to są te właśnie fale grawitacyjne i to są właśnie rzędy milisekund."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
Factual claim 🔹 Other AI assessment confidence: 90% Source on YouTube

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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

ą być związane z obiektami o odpowiedniej jakby konfiguracji. Tutaj takim najlepszym obiektem i takim, który jakby był najczęściej używany w symulacjach, to jest taka wirująca hantla. I taka wirująca handtla, gdy przyspiesza, jest źródłem fal grawitacyjnym. Im większe masy, tak, im te odległości różne, tym różnie się to dzieje. I to co obserwujemy obecnie to są te ultra krótkie fale grawitacyjne, te związane właśnie z ze zlewającymi się gwiazdami neutronowymi, czarnymi dziurami i tak dalej. Tak, to są te właśnie fale grawitacyjne i to są właśnie rzędy milisekund. Będziemy mogli pewnie zaobserwować o tym w tym odcinku dodatkowym trochę więcej powiemy o tych innych metodach obserwacji pulsarów troszeczkę troszeczkę więcej o tych już wchodzących albo tych przyszłościowych, a mianowicie planowany jest detektor kosmiczny, gdzie będziemy mieli ramiona może mniej dokładne, ale dużo, dużo dłuższe I tutaj będzie mo

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