Скачать или смотреть The Milky Way’s Next Supernova Will Reveal PHYSICAL Dark Matter

The mystery of dark matter remains unsolved, as its presence is inferred indirectly from astrophysical measurements rather than directly detected. Efforts to find dark matter have been based on its possible interaction with normal matter, but all experiments have failed so far. One possible key to revealing dark matter lies in the next supernova within the Milky Way, specifically a core-collapse (Type II) supernova. These events release 99% of their energy in the form of neutrinos, weakly interacting particles that carry away massive amounts of energy during the supernova explosion.

Supernovae like these are crucial in our understanding of dark matter and neutrinos. The detection of neutrinos from supernova explosions is rare, with notable examples like Supernova 1987A, which provided groundbreaking insight. As our detection technologies have evolved, such as with IceCube, JUNO, and Hyper-K, the next Milky Way supernova could potentially reveal millions of neutrinos. Comparing observed neutrino counts with theoretical predictions could show discrepancies, possibly indicating dark matter's role in carrying away energy.

The video highlights the limitations of lab experiments in recreating the extreme conditions of supernovae, suggesting that astrophysical observations could offer insights that controlled experiments cannot. Furthermore, if dark matter does contribute to energy loss during these cosmic events, it could finally point to a way to detect it.

The next supernova, if it happens soon, will provide a flood of data, but whether it will show signs of dark matter remains uncertain. Even if the results align with the current Standard Model, astronomers remain hopeful that such a cosmic event will unlock new physics and lead to revolutionary discoveries about dark matter and neutrinos.

#AHAstronomy #astronomy #cosmology #DarkMatter #Supernova #Neutrinos #Astrophysics #CosmicRays #ParticlePhysics #Neutrino #ScienceDiscovery

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