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Extra resources for [Magazine] Scientific American. Vol. 275. No 1
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This loss of information didn’t really matter in the classical theory. One could say that all the information about the collapsing body was still inside the black hole. It would be very difficult for an observer outside the black hole to determine what the collapsing body was like. However, in the classical theory it was still possible in principle. The observer would never actually lose sight of the collapsing body. Instead it would appear to slow down and get very dim as it approached the event horizon.
Ziegler, A. S. Jonason, D. J. Leffell, J. A. Simon, H. W. Sharma, J. Kimmelman, L. Remington, T. Jacks and D. E. Brash in Nature, Vol. 372, pages 773–776; December 22–29, 1994. Cancer Free: The Comprehensive Cancer Prevention Program. Sidney J. Winawer and Moshe Shike. Simon & Schuster, 1996. Sunlight, Ultraviolet Radiation and the Skin. NIH Consensus Statement. Vol. 7, No. 8, pages 1–29; May 8–10, 1989. html Sunlight and Skin Cancer Copyright 1996 Scientific American, Inc. Scientific American July 1996 59 The Nature of Space and Time Two relativists present their distinctive views on the universe, its evolution and the impact of quantum theory by Stephen W.
But this tiny information gain will be much smaller than the information loss in the collapse (in what I regard as any reasonable picture of the hole’s final PHASE SPACE disappearance). A phase-space diagram is a mathematical volume If we enclose the system in a vast box, as a thought experiment, we of many dimensions formed when coordinate axes can consider the phase-space evolution of matter inside the box. In the are assigned to each of the distance and momenregion of phase space corresponding to situations in which a black hole tum values of each particle.
[Magazine] Scientific American. Vol. 275. No 1
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