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Gamma Ray Bursts

Posted: Tue Apr 17, 2012 5:01 pm
by bperet
Gamma-ray bursts (GRBs) are flashes of gamma rays associated with extremely energetic explosions...
It occurs to me that when a cosmic star becomes a supernova, the core of that star would be exploding in space (the outer layers being ejecta in coordinate time). Space is what we observe and measure, so a cosmic supernova should show up in space as a huge burst of radiation and ejecta, corresponding with the cosmic supernova. As Larson describes in his astronomical research, the radiation emitted by white dwarfs and pulsars initially falls in the gamma ray, then X-ray bands, before cooling down sufficiently to start emitting light and radio waves. This has been detected by the BeppoSAX satellite for the Gamma Ray Burst.

There is a lot of guesswork regarding GRBs, and they are assumed to take place at extreme distances, and hence be extremely energetic. Larson, in Quasars & Pulsars, points out this fallacy that is based on an incorrect measurement of the redshift. Like quasars, the GRB is a cosmic event and is being displaced substantially in coordinate time, a factor not considered by conventional astronomy. Therefore, they would be significantly closer than believed because the radiation is still moving it time--in other words, the radiation is moving faster than light, but on a coordinate space vector. The amount of energy released would be on the scale of a supernova.

Because temporal motion has no direction in space (just as space has no direction in time), the burst will not be a ray, as theorized, but a spherical distribution.

It is likely that the association with distant galaxies is just a coincidence. Anyone who has looked at the NASA deep field knows that no matter where you point that telescope, you get a field full of galaxies. Stare long enough at any spot in the sky, and you're bound to spot a galaxy far behind any celestial event.

GRBs will not be limited just to supernovae, but to any cosmic event that generates motion in the inverse, ultra-high speed range, which includes the cores of cosmic galaxies and the resulting quasars.