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|    Message 7,299 of 9,209    |
|    Eli the Bearded to Johan de Koning    |
|    Re: ASCII math (7/10)    |
|    24 Jun 09 00:05:51    |
      [continued from previous message]              for example, the Clifford algebra, the Weyl algebra, noncommutative       tori, the quantum plane (and all other r-symmetric algebras), and       quantum groups. Also, all supercommutative algebras are automatically       r-commutative.              In fact, I believe that there is a deep relation between       braids (or r-commutativity) and quantization. This goes back to       Kaufmann's observation that the skein relation for the Conway polynomial              \ / \ / | |        \ / \ / | |        \ - / = -i hbar | |        / \ / \ | |       / \ / \ | |              and the canonical commutation relations               pq - qp = -i hbar.              It was made more clear by the discovery of the relation between quantum       groups and knot invariants (which I haven't really touched upon yet --       here I highly recommend Louis Kaufmann's book KNOTS AND PHYSICS, by       World Scientific Press). It was made still more clear (in my opinion)       by the work of Frohlich, Gabbiani, Rehren, Schroer, and many others on       the appearance of braid group statistics in low-dimensional quantum       field theory. (Essentially, these authors show that every nice quantum       field theory gives rise to a "fusion algebra" for the conserved charges,       and that these fusion algebras are r-algebras.) But I suspect that at       the root of it all is something rather simpler which we haven't       understood yet. A clue, I think, lies in the "classical       Yang-Baxter equations." These are what physicists would call a       "semiclassical limit" of the Yang-Baxter equations. Namely, take       R: V x V -> V x V of the form R = T(1 + hbar r), where T is the usual       twist map              T(v x w) = w x v,              and r: V x V -> V x V, write down the Yang-Baxter equation for R, and       collect all terms of order hbar^2. This equation is identical to the       equation that a "Poisson structure" must satisfy. For details, see       Drinfeld's famous review paper on quantum groups. The point here is       that a Poisson structure, which defines the Poisson bracket of classical       observables, is a semiclassical limit of the commutator which appears in       quantum mechanics. Thus an infinitesimal deformation of the usual twist       map that is required to satisfy the Yang-Baxter equation is THE SAME       THING as an infinitesimal deformation of the commutative product in the       classical algebra of observables (i.e., a Poisson bracket).              More later...                     r-Algebras              So... let's say we have an r-algebra. That's an       algebra with an invertible linear map R: A x A -> A x A (again, "x"       denotes tensor product), which we draw as a right-crossing:              \ /        \ /        \        / \       / \              which satisfies 1) the Yang-Baxter equations:                     \ / | | \ /        \ / | | \        \ | | / \        / \ | | / \       / \ | \ / |       | \ / \ / |       | \ = \ |        | / \ / \ |       \ / | | \ /        \ / | | \ /        \ | | \        / \ | | / \       / \ | | / \              2) R(1 x a) = a x 1 and R(a x 1) = 1 x a, and              3) the quasitriangularity conditions; writing multiplication as the       joining of strands these are                     \ / / \ \ /        \ / / \ \ /        | / \ \        \ / \ / \        \ / = \ \        \ / \ |        / \ / \ /        / \ / |        / \ / |              and              \ \ / \ / /        \ \ / \ / /        \ | \ /        \ / = / \ /        \ / \        / \ | / \        / \ \ / \        / \ | \       / \ | \              We say an r-algebra is "r-commutative" if              \ / \ /        \ / \ /        \ \ /        / \ |        \ / = |        | |        | |              and "strong" if R^2 is the identity, or R equals its inverse, i.e.:              \ / \ /        \ / \ /        \ = /        / \ / \       / \ / \              (Note that a left-crossing              \ /        \ /        \        / \       / \              is the inverse of a right-crossing.)              All sorts of noncommutative analogs of manifolds are r-commutative       algebras: quantum groups, noncommutative tori, quantum vector spaces,       the Weyl and Clifford algebras, certain universal enveloping algebras,       supermanifolds, etc.. It seems that the ones with direct relevance to       quantum theory in 4 dimensions are "strong," while the non-strong ones,       like quantum groups, are primarily relevant to 2- and 3-dimensional       physics. I would now like to describe an analog of differential forms       for strong r-commutative algebras, and illustrate it for the case of the       Heisenberg algebra - i.e., the algebra defined by the canonical commutation       relations: pq - qp = -i hbar.              What are differential forms? Of course, they're the basis of a lot of       differential geometry, and there are lots of equivalent ways of defining       them, but let me take an algebraic viewpoint. Let A be the algebra of       smooth functions on a manifold M. We define differential forms as       follows. Each function f in A has a "differential" df, and the       functions and their differentials generate an algebra in which we impose       the following relations:              1) Linearity: d(f+g) = df + dg, d(cf) = c(df) for any scalar c.              2) The product rule: d(fg) = (df)g + f(dg).              3) The derivative of a constant vanishes: d1 = 0.              4) Commutation relations: f(dg) = (dg)f and (df)(dg) = -(dg)(df).              This algebra is called the algebra of differential forms on M.              That's all, folks! If you've taken a course in differential geometry       you were probably exposed to tangent planes and all that stuff, but if       you want to get calculating with differential forms as soon as possible       this is all you need to start with.              Note that rule 4) is the only one in which we SWITCH elements of A --       moving f to the right of g. This is the rule we'll need to modify for       an r-commutative algebra. You could, of course, just leave out rule 4):       given any algebra A, the algebra whose relations are just given by 1)-3)       is called the "universal differential calculus" for A. It's a       reasonable substitute for differential forms when A is any old       noncommutative algebra, and (from one viewpoint) it's the basis of Alain       Connes' approach to noncommutative differential geometry. But when you       have a strong r-commutative algebra one can replace rule 3) with              4') Commutation relations: f(dg) = (dg^i)f_i and       (df)(dg) = -(dg^i)(df_i).              Here I should explain that I'm writing R(f x g) as the sum over i of       tensor products of the form g^i x f_i (one can always do this), and       I'm using the Einstein summation convention (sum over repeated indices)       to avoid writing the summation sign. What we're doing in rule 4') is       just what we should do: use R to "switch" f and g instead of "naively"       switching them as in 4).              Now let me show what this buys you in the case of the Heisenberg       algebra. Actually I'm going to be sneaky and use a variant of the       Heisenberg algebra where we stick in a square root of hbar, which I'll       call h, just to confuse the heck out of the physicists. (Actually, it's       because it's a pain to write square roots in ASCII!) This is the       algebra over C generated by 3 formal variables, p, q, and h, subject to       the relations that              pq - qp = -i h^2              p h = h p              q h = h q              Note that we're NOT treating h (the square root of hbar) as a number       here, but as a variable, so I have to explicitly SAY that it commutes       with everything.                     [continued in next message]              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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