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To re-iterate for clarity, what we are talking about are phenomena that could be observed at gamma or x-ray wavelengths if you assume the Rovelli Vidotto model of black hole.
So it is a possible test of the new RV model of BH, the "planck star" model as applied to primordial BH in this case. The model is interesting, different in significant ways, and could of course be wrong. We need observations to tell.
In order to talk about this you need to know the BASICS of this new BH model. In particular that it looks like a conventional BH for most of its lifetime but that its lifespan is only 65% as long for the same initial mass.
It evaporates by Hawking radiation at the same rate as a conventional BH of the same initial mass until its mass has dwindled to about 70% of initial (which takes about 65% of conventional lifespan) and then it blows up in a gamma burst. These are the short or very short GRB which could be studied.
Their energy is predicted by the theory and depends on when they exploded. Those that exploded in the past would have calculably less energy. Those exploding in the approximate present would have an energy mass-equivalent of about 140 megaton, or if you like 1.4 x 1011 kg.
Folks can multiply that by the speed of light squared to get the ergs or joules if they like.
So it is a possible test of the new RV model of BH, the "planck star" model as applied to primordial BH in this case. The model is interesting, different in significant ways, and could of course be wrong. We need observations to tell.
In order to talk about this you need to know the BASICS of this new BH model. In particular that it looks like a conventional BH for most of its lifetime but that its lifespan is only 65% as long for the same initial mass.
It evaporates by Hawking radiation at the same rate as a conventional BH of the same initial mass until its mass has dwindled to about 70% of initial (which takes about 65% of conventional lifespan) and then it blows up in a gamma burst. These are the short or very short GRB which could be studied.
Their energy is predicted by the theory and depends on when they exploded. Those that exploded in the past would have calculably less energy. Those exploding in the approximate present would have an energy mass-equivalent of about 140 megaton, or if you like 1.4 x 1011 kg.
Folks can multiply that by the speed of light squared to get the ergs or joules if they like.