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Before getting to the essential point of whether black hole destroys information or not, it is necessary to clarify the meaning of information (Figure 09xaa). According to Leonard Susskind, who played a principle role in the debate, entropy is hidden information. This view considers the basic units (or bits) of information to be the microscopic particles, which can be atoms, elementary particles, or down to the smallest unit the size of Planck length (~ 10-33cm). They are hidden because its existence is not known to us. Once we are aware of its presence (such as an electron in a collision experiment), it becomes information, and generates events that we can keep track of. The information is said to be conserved because we can always recover the original event by time reversal operations (at least in theory, which asserts that the laws of physics are the same in both forward and backward time directions, the "Second Law of Thermodynamics" notwithstanding because it is actually applicable to one or at most few particles). | |
Figure 09xaa Black Hole Information Paradox |
Figure 09xa Typical Information |
Figure 09xb Eigen-states |
The total probability is P = 1 (absolute certainty) again regradless of which state it collapses into (Figure 09xb). Such process is called decoherence. |
Figure 09xc shows the time varying probability in spite of the invariance form of the total probability P. Figure 09xd illustrates the collapse of the superposition via a measurement using the mixed spin states as example. BTW, a deterministic process such as the Schrodinger Equation is time-reversible, i.e., it is invariant under a change of time t - t. | ||
Figure 09xc Unitary State as Info |
Figure 09xd Quantum Measurement |
inverse, which in turn implies that it is possible to return to the initial state from the final state at least in principle although the probability is almost zero in practice so that the second law of thermodynamics is "almost" never violated. This is another example of the conservation of information. Here's a Feynman diagram for e- + e+ scattering with probability amplitude S11 | |
Figure 09xd1 S-Matrix |
(Figure 09xd1) . Detection of the process is equivalent to decoheren of quantum states. |
the superposition in the decoherent process. If that's the case, there would be no problem with the loss of information, because the superposition is terminated normally. The paradox is about the existence of the "measuring device" - there is none at the event horizon according to general relativity. Or else the superposition is somehow trapped inside the black hole, for which plenty of opinions are proposed about its fate - whether it is lost forever or can be recovered eventually. | |
Figure 09xd2 No-hair Theorem [view large image] |
Figure 09xe Hawking Radiation |
Figure 09xf Black Hole Evaporation |
seems that the opinions are divided into two camps. There is the General Relativity (GR) proponents (the relativists) who favor information loss. They blame the controversy on the incompleteness of quantum theory, in particular the discontinuous jump from superposition to a definite state. |
While for observer B inside the black hole, the elephant crosses the event horizon into the black hole, nothing untoward happens until the tidal force takes over ... information is carried to the singularity (see "Black Hole Space-time"). According to the quantum theorists the information is not lost from both points of view. | |
Figure 09xga Black Hole Complementarity |
This was when the "war" reached a stalemate. |
Figure 09xgb Holographic Space-time [view large image] |
It took a while for Hawking to concede defeat. He called a press conference in 2004 and announced to the world that he had changed his mind. Black holes did not, after all, irreversibly annihilate information. |
The bet with Preskill (his gambling partner) was duly settled in the form of a baseball encyclopedia. Meanwhile he lost another wager (on conservation of infromation) with Don Page (one of his students) and had it settled in 2007. Here's a photocopy of the original contract with his signature and fingerprint [view large image]. Stephen died on March 14, 2018. | |
and the Hawking radiation at the same time. The paradox can be resolved by severing the link with the twin (inside the black hole), but it is a violent process. The energy holding up the entanglement would incinerate the event horizon with a wall of fire (Figure 09xh). General relativity maintains that crossing over the event horizon should be uneventful but the firewall erects a signpost in violation of this doctrine. Figure 09xi illustrates the strange episodes surrounding the paradox. | ||
Figure 09xh Black Hole and Information |
Figure 09xi BH Firewall |
Then a few months later a new idea claims that entanglement of the photon in the Hawking radiation and its twin in the black hole can be replaced by a wormhole (Figure 09xj). Such connection may not be a problem for quantum monogamy in the way that normal entanglement would cause. The firewall could thus be dispensed with this scheme. Accordingly, there could be wormholes permeating over all the universe; what would happen when they encounter something ? would those things be sucked into the worm holes, going to another universe ? Or the wormholes exist only in the bulk dimensions, then we have to accept the reality of extra-dimensions. It seems that the scenarios are getting more and more bizarre and very difficult to comprehend. | |
Figure 09xj Wormhole Entanglement |
See "2022 Update". |
5. Quantum Numbers and Conservation Laws: Quantum numbers (like lepton number, baryon number, and other quantities tied to symmetries) are conserved in physical processes. Information about these values is fundamental because it's expected to be preserved in quantum processes. 6. Microstates: In thermodynamics and statistical mechanics, a system's "information" can refer to its microstates-the precise, microscopic configurations of particles that result in a particular macroscopic state. Black hole entropy, which describes the number of possible configurations of matter and energy in a black hole, suggests that a black hole has an enormous number of microstates. Information about these microstates would theoretically be lost if a black hole evaporates completely, deepening the paradox. In the context of the paradox, losing "information" means losing all of these properties and details about particles, fields, and correlations that describe the precise history of the system. This loss would violate the principle of unitarity in quantum mechanics, which mandates that such information must always be preserved, even if it cannot be accessed easily. The question of whether black holes truly destroy information, or if it is somehow preserved or encoded in ways we don't fully understand yet, is at the heart of the paradox. | |