How to extract energy from gamma ray burst release?
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Artist's illustration showing the life of a massive staras nuclear fusion converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a black hole. Theoretically, energy may be released during the collapse along the axis of rotation to form a gamma-ray burst.
In gamma-ray astronomy, gamma-ray bursts(GRBs) are extremely energetic explosions that have been observed in distant galaxies. They are the brightest electromagnetic events known to occur in the universe.[1] Bursts can last from ten milliseconds to several hours.[2][3][4] After an initial flash of gamma rays, a longer-lived "afterglow" is usually emitted at longer wavelengths (X-ray, ultraviolet, optical, infrared, microwave and radio).[5]
The intense radiation of most observed GRBs is thought to be released during a supernovaor superluminous supernova as a high-mass star collapses to form a neutron star or a black hole.
Artist's illustration showing the life of a massive staras nuclear fusion converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a black hole. Theoretically, energy may be released during the collapse along the axis of rotation to form a gamma-ray burst.
In gamma-ray astronomy, gamma-ray bursts(GRBs) are extremely energetic explosions that have been observed in distant galaxies. They are the brightest electromagnetic events known to occur in the universe.[1] Bursts can last from ten milliseconds to several hours.[2][3][4] After an initial flash of gamma rays, a longer-lived "afterglow" is usually emitted at longer wavelengths (X-ray, ultraviolet, optical, infrared, microwave and radio).[5]
The intense radiation of most observed GRBs is thought to be released during a supernovaor superluminous supernova as a high-mass star collapses to form a neutron star or a black hole.
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