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  2. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    The Diffuse Supernova Neutrino Background (DSNB) is a cosmic background of (anti)neutrinos formed by the accumulation of neutrinos emitted from all past core-collapse supernovae. [1] Their existence was predicted even before the observation of supernova neutrinos. [42] DSNB can be used to study physics on the cosmological scale. [43]

  3. SuperNova Early Warning System - Wikipedia

    en.wikipedia.org/wiki/Supernova_Early_Warning_System

    The SuperNova Early Warning System (SNEWS) is a network of neutrino detectors designed to give early warning to astronomers in the event of a supernova in the Milky Way, our home galaxy, or in a nearby galaxy such as the Large Magellanic Cloud or the Canis Major Dwarf Galaxy. As of March 2021, [1] SNEWS has

  4. Diffuse supernova neutrino background - Wikipedia

    en.wikipedia.org/wiki/Diffuse_supernova_neutrino...

    An individual supernova will release as many as neutrinos, which is detectable as a short burst of events on Earth provided that the supernova occurred close by enough, either within our own galaxy or one of its satellite galaxies; the only current example of which is SN1987A. In contrast, the DSNB is a continuous source of neutrinos ...

  5. Type II supernova - Wikipedia

    en.wikipedia.org/wiki/Type_II_supernova

    Because neutrinos rarely interact with normal matter, they can escape from the core, carrying away energy and further accelerating the collapse, which proceeds over a timescale of milliseconds. As the core detaches from the outer layers of the star, some of these neutrinos are absorbed by the star's outer layers, beginning the supernova explosion.

  6. Helium and Lead Observatory - Wikipedia

    en.wikipedia.org/wiki/Helium_And_Lead_Observatory

    It was designed to be a low-cost, low-maintenance detector [5] with limited capabilities [6]: 38 sufficient for the burst of neutrinos generated by a nearby supernova. Its major components are left over from other decommissioned experiments: 76 tons of lead from an earlier cosmic-ray experiment, and 128 three-metre-long helium-3 neutron ...

  7. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    The core collapse phase of a supernova is an extremely dense and energetic event. It is so dense that no known particles are able to escape the advancing core front except for neutrinos. Consequently, supernovae are known to release approximately 99% of their radiant energy in a short (10-second) burst of neutrinos. [110]

  8. AOL Mail

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    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  9. GRB 221009A - Wikipedia

    en.wikipedia.org/wiki/GRB_221009A

    The supernova was a Type Ic supernova, similar to SN 1998bw, the first supernova linked to a GRB. Lightning detectors in India and Germany picked up signs that the Earth's ionosphere was perturbed for several hours by the burst, though only mildly, [ 37 ] [ 17 ] [ 4 ] as well as an enormous influx of electrically charged particles, [ 38 ...