Are Black Holes sufficiently characterized?

AI Thread Summary
The discussion centers on whether mass, angular momentum, and charge are sufficient for characterizing black holes, or if entropy and surface area should also be considered. The no-hair theorem suggests that these three parameters are all that is necessary to describe a black hole, with entropy and surface area being derived from them. It is noted that in real astrophysical black holes, charge can typically be assumed to be zero due to the equal numbers of protons and electrons. Despite this, the consensus is that all three parameters—mass, angular momentum, and charge—are essential for a complete description. Overall, the characterization of black holes remains a nuanced topic in astrophysics.
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Is mass, angular momentum, and charge sufficient for black hole characterization? Or is also entropy, and hence surface area, also required? Thus is the shape for a given mass black hole also a required consideration?
 
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From all the reading I've done, I gather that the mass and spin are the properties that matter. I haven't read of charge being much of an issue in real BHs and size seems to be mentioned only as the diameter of the event horizon.
 
This is precisely the statement of the no-hair theorem, that mass, angular momentum, and charge are the only three numbers necessary to describe a BH. The quantities you mention, entropy and surface area, are derived from the above three.
 
phinds said:
From all the reading I've done, I gather that the mass and spin are the properties that matter.
For real, astrophysical black-holes -- the charge can be assumed to be zero, as a black-hole will be formed from (ridiculously close to) equal numbers of protons and electrons. But all three parameters are actually needed for a complete description, as Nabeshin said---according to the http://en.wikipedia.org/wiki/No_hair_theorem"
 
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