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Why neutrinos in a supernova reach consensus faster ⚡ экспресс

Original: "Two-beam Multiparticle Many-body simulations of Inhomogeneous FFI"
· Zoha Laraib, Sherwood Richers
arXiv:2511.16506 · 2025-11-20 · CC BY · ⏱ 1 min · High Energy
Neutrinos in a supernova team up, which speeds up their flavor changes and could alter the story of a star’s explosion.
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Every second, trillions of neutrinos zip through us. But in the heart of a supernova, these ghost particles become sociable: they swap properties and reach equilibrium faster. New modeling opens the door to unlocking the secrets of stellar explosions.

🎯 From supernova 1987A, Earth’s detectors caught just 25 neutrinos—but that was enough to confirm the theory of stellar collapse.

Scientists
Emmy NoetherEnrico FermiPaul DiracWolfgang PauliSubrahmanyan ChandrasekharJocelyn Bell Burnell
Tags
supernova neutron star Standard Model
Laws
Noether's theoremFermi–Dirac statisticsspin–statistics theoremFermi's golden ruleChandrasekhar limitFermi acceleration
Original: arXiv:2511.16506 · CC BY · bridge42worlds