- #36
Haelfix
Science Advisor
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To the OP. In order to have a matter/antimatter asymmetry the necessary and sufficient conditions were layed out by Sakharov in the 60s.
A black hole in and of itself is not sufficient to meet these bounds, however a black hole and other physics is. So while this isn't exactly what you had in mind, its somewhat related.
For instance Grand unified theories provide a mechanism to have baryon number nonconservation and CP violation. So indeed, if you combine a black hole with something like that, you presumably satisfy the conditions necessary.
This is what's called black hole baryogenesis, and it has been looked at before (Hawkings and Zeldovitch were the pioneers afair). The idea being, a black hole while its radiating under the Hawking process can spit out a bunch of heavy particles, and they in turn can violate lepton or baryon number. The black hole in that case, acts like a sort of multiplier to the final observed asymmetry.
The problem is, you need a lot of primordial black holes in the early universe to be of relevance, and this in turn is very sensitive to inflation and is highly model dependant. Moreover Sphaleoron processes damp some of this as well.
You'd probably have to search arxiv for the modern parameter spaces where this hypothesis lives in. I don't know off the top of my head if its been falsified or whether its still active.
A black hole in and of itself is not sufficient to meet these bounds, however a black hole and other physics is. So while this isn't exactly what you had in mind, its somewhat related.
For instance Grand unified theories provide a mechanism to have baryon number nonconservation and CP violation. So indeed, if you combine a black hole with something like that, you presumably satisfy the conditions necessary.
This is what's called black hole baryogenesis, and it has been looked at before (Hawkings and Zeldovitch were the pioneers afair). The idea being, a black hole while its radiating under the Hawking process can spit out a bunch of heavy particles, and they in turn can violate lepton or baryon number. The black hole in that case, acts like a sort of multiplier to the final observed asymmetry.
The problem is, you need a lot of primordial black holes in the early universe to be of relevance, and this in turn is very sensitive to inflation and is highly model dependant. Moreover Sphaleoron processes damp some of this as well.
You'd probably have to search arxiv for the modern parameter spaces where this hypothesis lives in. I don't know off the top of my head if its been falsified or whether its still active.