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Article #1410Re: Quantum Cosmological Boundaries and Determinisim?
From: Stephen Braham
Date: Thu, 23 Jul 1992 17:24
Date: Thu, 23 Jul 1992 17:24
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MRG3@psuvm.psu.edu writes: > [stuff deleted] >QM is generally taught.:) Generally, when the density matrix is introduced, >it is in terms of some level of ignorance (unknown measurement results, quantum >entanglement with other systems, etc.). While this may be a useful viewpoint >at first, I tend to think it results in confusion in the long run. >QM can be expressed solely in terms of density operators, without ever >referring to a state vector. A pure state is merely a minimum entropy >density operator. Evolution of isolated systems (in normal QM) is unitary >and preserves entropy (i.e. pure states stay pure), although alternatives >to standard QM, such as Quantum Mechanics with Spontanious Localization, >have nonunitary evolution(where we can only say entropy is nondecreasing). >In open quantum systems, there has a great deal of work done on >phenomenological evolution equations. When you start looking at >quantum open systems, or variants of the Schroedinger equation, paying >attention to things like "where did the information go" is distraction and >irrelevant (unless you are considering foundational issues). I think a >fairly good intro to density operators can be found in von Neuman's >Mathematical Foundarions of Quantum Mechanics. Yes, at, in some sense, ADH goes even further; once you define everything in terms of decoherence functionals, you can even get rid of the idea of a density matrix, or the concept of a state at a given time. It's this that interests us in QC, of course, where time is a dirty word. > The effective dynamics of an open quantum system tend to >reduce the coherence terms of the density operator of the >system of interest. They don't go away in a finite time, rather, the >the decoherence decays away (hopefully exponentially) with time. >The density operator can never be diagonal in a continuous >basis (such as position): it would not be normalizable. >Decoherence and the "superselection" are necessarily >approximate. Exactly, and this connects up with an earlier statement by Jase on the difficulty is getting perfectly decohered histories. Approximate decoherence seems to be the way to go, but it's hard to QUANTIFY it. I really worry that coarse graining may not preserve approximate decoherence (unlike perfect decoherence). We can almost see what needs to be done in the old density matrix, S-picture, type decoherence, but, as I said in another post, the ADH off-diagonal terms are not really connect to the off-diagonal terms in the effective density matrix (when that matrix exists, which, in general, it doesn't). There's a DYNAMICAL connection- the same squeezing together of the trajectories in the configuration space path integral produces both types of decoherence, but that's not enough for an _interpretation_. It helps, though :). > With regards to quantum coherence down the wormhole: >This strikes me as just another open quantum system with inaccessible >regions (to the observable universe, as opposed to the entire universe). >A minor point is that it is not degrees of freedom that go down the wormhole, >but rather, there is quantum entanglement between degrees of fredom (field >amplitudes) out here and degrees of freedom down in there. >There is still no dynamical mechanism for collapsing the wave function. Oh goody, I get to be in wormie mode for a bit; yeah, I know tend to believe that wormies don't help as much in that regard. On the other hand, I think we're pushing our paradigm a little far when we talk about information going down 'em- it's hard to give them a physical meaning outside the Euclidean path integral, and the interpretation of THAT is getting tougher. At a certain point, I'd go along with Jim Hartle and say let's define QM _by_ the decoherence functional, and forget about fields at a particular time. >mike gallis >mrg3@psuvm.psu.edu Steve -- | Name: Stephen P. Braham | Perversion: Quantum Cosmologist| | Hangout: UBC physics | Signature: Euclidean | | Vancouver, BC |--------------------------------+ | Canada | E-mail: braham@physics.ubc.ca |
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Path: arc1-ca.pugleaf.net!sparky!uunet!elroy.jpl.nasa.gov!swrinde!sdd.hp.com!caen!destroyer!ubc-cs!unixg.ubc.ca!physics.ubc.ca!braham From: braham@physics.ubc.ca (Stephen Braham) Newsgroups: sci.physics Subject: Re: Quantum Cosmological Boundaries and Determinisim? Message-ID: <braham.711912261@physics.ubc.ca> Date: 23 Jul 92 17:24:21 GMT References: <jtwamley.711766649@adelphi> <braham.711770201@physics.ubc.ca> <92204.111241MRG3@psuvm.psu.edu> <mcirvin.711851892@husc8> <92205.082205MRG3@psuvm.psu.edu> Sender: news@unixg.ubc.ca (Usenet News Maintenance) Organization: University of British Columbia, Vancouver, B.C., Canada Lines: 79 Nntp-Posting-Host: physics.ubc.ca