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  2. Gamma ray - Wikipedia

    en.wikipedia.org/wiki/Gamma_ray

    Gamma rays are produced during gamma decay, which normally occurs after other forms of decay occur, such as alpha or beta decay. A radioactive nucleus can decay by the emission of an α or β particle. The daughter nucleus that results is usually left in an excited state. It can then decay to a lower energy state by emitting a gamma ray photon ...

  3. Gamma-ray burst - Wikipedia

    en.wikipedia.org/wiki/Gamma-ray_burst

    With the discovery of GRB 190114C, astronomers may have been missing half of the total energy that gamma-ray bursts produce, [110] with Konstancja Satalecka, an astrophysicist at the German Electron Synchrotron, stating that "Our measurements show that the energy released in very-high-energy gamma-rays is comparable to the amount radiated at ...

  4. Gamma-ray astronomy - Wikipedia

    en.wikipedia.org/wiki/Gamma-ray_astronomy

    Long before experiments could detect gamma rays emitted by cosmic sources, scientists had known that the universe should be producing them. Work by Eugene Feenberg and Henry Primakoff in 1948, Sachio Hayakawa and I.B. Hutchinson in 1952, and, especially, Philip Morrison in 1958 [6] had led scientists to believe that a number of different processes which were occurring in the universe would ...

  5. Very-high-energy gamma ray - Wikipedia

    en.wikipedia.org/wiki/Very-high-energy_gamma_ray

    Air showers of elementary particles made by gamma rays can also be distinguished from those produced by cosmic rays by the much greater depth of shower maximum, and the much lower quantity of muons. [7] Very-high-energy gamma rays are too low energy to show the Landau–Pomeranchuk–Migdal effect. Only magnetic fields perpendicular to the path ...

  6. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    Terrestrial lightnings produce high-speed electrons that create bursts of gamma-rays as bremsstrahlung. The energy of these rays is sometimes sufficient to start photonuclear reactions resulting in emitted neutrons. One such reaction, 14 7 N (γ,n) 13 7 N, is the only natural process other than those induced by cosmic rays in which 13 7 N is ...

  7. Ultra-high-energy gamma ray - Wikipedia

    en.wikipedia.org/wiki/Ultra-high-energy_gamma_ray

    The ratio of primary cosmic ray hadrons to gamma rays also gives a clue as to the origin of cosmic rays. Although gamma rays could be produced near the source of cosmic rays, they could also be produced by interaction with cosmic microwave background by way of the Greisen–Zatsepin–Kuzmin limit cutoff above 50 EeV. [4]

  8. 25 hostess gifts from Walmart are way better than a bottle of ...

    www.aol.com/lifestyle/hostess-gifts-from-walmart...

    The holiday season is well underway, which means your calendar is probably filled up with social events ranging from Secret Santa gift swaps to work holiday parties. All of that socializing means ...

  9. Terrestrial gamma-ray flash - Wikipedia

    en.wikipedia.org/wiki/Terrestrial_gamma-ray_flash

    A terrestrial gamma-ray flash (TGF), also known as dark lightning, is a burst of gamma rays produced in Earth's atmosphere. TGFs have been recorded to last 0.2 to 3.5 milliseconds , and have energies of up to 20 million electronvolts .