Image Credit:
NASA/DOE/Fermi LAT Collaboration
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One explanation for the gamma-ray emission is that the blast creates multiple shock waves that expand into space at slightly different speeds. Faster shocks could interact with slower ones, accelerating particles to near the speed of light. These particles ultimately could produce gamma rays. See: NASA's Fermi Space Telescope Reveals New Source of Gamma Rays
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Credit: Weiqun Zhang and Stan Woosley |
This image is from a computer simulation of the beginning of a gamma-ray burst. Here we see the jet 9 seconds after its creation at the center of a Wolf Rayet star by the newly formed, accreting black hole within. The jet is now just erupting through the surface of the Wolf Rayet star, which has a radius comparable to that of the sun. Blue represents regions of low mass concentration, red is denser, and yellow denser still. Note the blue and red striations behind the head of the jet. These are bounded by internal shocks. See: "ROSETTA STONE" FOUND TO DECODE THE MYSTERY OF GAMMA RAY BURSTS
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