A Few notes on SN2006GY & W49B

The Mechanics of Novadic Distributions

by Joseph_Sixpack

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Abstract:
Black Holes 'explode' or 'go off' when the solar mass 
escaping thru the zero gravity port or thru evaporation, 
drops beneath the escape velocity required to hold 
radiation.

As probably an unnecessary note, that escape velocitgy value 
corresponds to the value of 186,000 miles per second, or c, 
the speed of light.  If the escape velocity is only 185,999 
miles per second, everything gets to leave at once, like 
kids getting out of school on the last day of school before 
summer vacation, off it goes in every direction at once.

All of these types of super novas would have perhaps the 
same visible physical displaying realities since the release 
event would be the same solar mass number for all of them.  
Any minor differences could be attributed to the rate of 
plasma leakage thru the zero gravity port

That is, they would release all their pent up plasma or 
radiation at approximately the same solar mass value.  
Initial escape velocities, for say the first few time 
periods, may somewhat depend on how fast the retention rate 
deteriorates.   

Establishing this value could give insight as to just what 
solar mass requirements would be necessary for 'black hole 
status'.

The hypothesis presented by joe is that SN2006gy was just 
such a system event.

No internal collapse of mass was required to set off the 
nova.

If anything, a collapse of internal mass would increase 
gravitation by increasing gravitational efficiency, and 
extend the event horizon outwards even more, and interdict 
any immediate distribution of relieved plasma by retaining 
all radiation well within its event horizon.  An internal 
collapse is or would be, a silent and invisible event.


W49b W49b as well as the crab nebulae are examples of distributed black holes, one definitely a binary, whose solar mass values dipped beneath the necessary retention value to retain mass. The other probably made its distribution the same way. W49b needs to be checked out for any quasar or pulsar broadcasting if it hasn't already.
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