Could LIGO project also be the start to explain Gamma Ray Bursts of small black holes?
The recent 2017 Black hole merger (GW 170104) seems to Fill the gap between the two former merger black holes, which raise the question what BH mass upper- and lower boundaries and BH ratios we could expect?
The recent 2017 Black hole merger (GW 170104) seems to Fill the gap between the two former merger black holes, which raise the question what BH mass upper- and lower boundaries and BH ratios we could expect?
Could it even explain the Gamma Ray Burst
(GRB) conundrum about the narrow energy focusing of the explosion energy by
assuming that we have to do with a splitting BH in two equal halves by a much
smaller one crashing into it?
Several
nebula ( like the Eagle -Spire) seem to show such splitting processes.
Consequently,
it would be interesting to investigate the directional focusing of Gamma Ray Bursts (GRBs) could be
originated by the merging and even
splitting of smaller lower bound BHs as suggested to take place in nebula like
the Eagle (Spire) nebula.
I would propose that there could be three
different merger and splitting systems of BHs depending on the size and ratios
of both BHs.
1: Normal
merger BHs as found by LIGO. Which seem so have rations between: 1/1.24 and
1/1.9 with masses of the participating BHs and resulting BHs between: 6 and 60
solar masses.
2: BH
splitting into two equal halves, observed in the Eagle ( spire) nebula with
unknown ratios
3:
Central Galaxy BHs gobbling up much
smaller BHs and growing in size with small steps.
