Shaw
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Is there theoretically a smallest possible Schwarzschild radius?
The discussion centers on the theoretical aspects of the smallest possible Schwarzschild radius, concluding that classically there is no lower limit due to the proportional relationship between mass and Schwarzschild radius. The conversation highlights that while a black hole (BH) can theoretically form from gravitational collapse with a minimum mass of approximately 3 solar masses, primordial black holes may exist at around 1011 kg. Speculative theories suggest that a Planck mass black hole could remain after evaporation, but there is currently no empirical evidence supporting the formation of black holes at the Large Hadron Collider (LHC).
PREREQUISITESAstronomers, physicists, and students interested in theoretical physics, particularly those focusing on black hole research and quantum gravity theories.
Yep, I still remember this.PAllen said:What do you want? For quantum case, there can be no detail because [..]
PAllen said:Each k in your series is smaller each time [..]Of course, this is all nonsense - no mirror is anywhere near that perfect. Also, of course, I do ignore quantum effects because [..]
Yeah, unlike ##\sqrt{1-v^2}##, here the limit for V is C.PAllen said:What do you want? [..]Since there is no lower limit on mass, there is no lower limit on Schwarzschild radius.
For natural BH you mean? I heard that CERN is creating tiny BH on daily basis.PAllen said:I1) What is the smallest BH that can form from gravitational collapse? This is not well known, but a guesstimate is around 3 solar masses.
Natural of course. Should have read that a minute longer before posting.Stephanus said:For natural BH you mean? I heard that CERN is creating tiny BH on daily basis.PAllen said:1) What is the smallest BH that can form from gravitational collapse? This is not well known, but a guesstimate is around 3 solar masses.
Stephanus said:For natural BH you mean? I heard that CERN is creating tiny BH on daily basis.
Perhaps if you calculate the momentum energy of two colliding protons each travels at 99.99%c multiply it by 2G in less then ##\frac{2GM_{proton}}{c^2}## radius, I don't know. I should have calculated it. Perhaps the concentration of the momentum energy in much less tiny radius could be called black hole. And I heard that for such tiny black hole, the hawking radiation will evaporate it in less then 1 second. You know better. Btw, I'm still studying your post about doppler effect in SR. Still trying to make sense out of it.PAllen said:There is currently exactly zero evidence that LHC has formed any BH [..]
http://phys.org/news/2010-12-large-hadron-collider-signatures-microscopic.html#nRlvStephanus said:Perhaps if you calculate the momentum energy of two colliding protons each travels at 99.99%c multiply it by 2G in less then ##\frac{2GM_{proton}}{c^2}## radius, I don't know. I should have calculated it. Perhaps the concentration of the momentum energy in much less tiny radius could be called black hole. And I heard that for such tiny black hole, the hawking radiation will evaporate it in less then 1 second. You know better. Btw, I'm still studying your post about doppler effect in SR. Still trying to make sense out of it.
Ok.Large Hadron Collider finds no signatures of microscopic black holes
Shaw said:your replies lack detail