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The Hawking radiation from an ordinary black hole is then identified with the white-hole emission. Instead, the collapsing matter on the other side of the event horizon reaches an enormous but finite density and rebounds, forming a regular Einstein—Rosen bridge. In quantum mechanics , the black hole emits Hawking radiation and so can come to thermal equilibrium with a gas of radiation not compulsory. Strings, Branes and Gravity. Accordingly, the observable universe is the Einstein—Rosen interior of a black hole existing as one of possibly many inside a larger universe. Torsion naturally accounts for the quantum-mechanical, intrinsic angular momentum spin of matter. Black holes Most massive Nearest Quasars Microquasars.

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