The true bijection between quantum entropy and the mass associated with every gravitationally closed horizon.
ORAL
Abstract
A black hole, (BH), is a closed space time horizon. It is the edge of space time. We can measure the amount of quantum information that has fallen behind it. Every bit of quantum information is the same. It has an entropy. In 1915 Karl Schwarzschild gave us the mass and radius of this mathematical object. It took 59 more years before Stephen Hawking realized this horizon has a temperature. It has taken another 48 years to prove that every bit of quantum information that falls in, has a quantum of entropy. Every quantum of entropy must have the same temperature. It cannot be zero and cannot be lower than the black hole temperature for the mass of our universe. Every gravitationally closed space-time horizon knows this temperature, (Tu). All closed space-time horizons are quantized by this temperature (Tu). I know this temperature and can prove it. (Tu) is the temperature of our universe as a BH. Every BH has a mass, (M), radius, (R), and temperature, (T).
(2M)/(R2)(T) = (4ϖk)/(c2)(Lp2) = 1/(Tu)
(2M)/(R2)(T) = (4ϖk)/(c2)(Lp2) = 1/(Tu)
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Publication: none
Presenters
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Paul F Obrien
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Authors
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Paul F Obrien
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