[ Home ] | Feynman's path integral method in quantum mechanics. | Numerical Methods. Note « 14 » |
Feynmans path integral.' Consider a one-dimentional motion of a particle with mass m, coordinate x and Lagrangian L(x,x´ )=m/2x´2-V(x). Suppose |xa〉 and |xb〉 are the eigenfunctions of the coordinate operator with the eigenvalues xa and xb. Suppose U(tb,ta)=e-iH(tb-ta) is the time-evolution operator: Ψ(x,tb)=U(tb,ta)Ψ(x,ta). Then the propagator Kxbxa(tb,ta) ≡ 〈xb|U(tb,ta)|xa〉 is intuitively defined defined as the Feynman's integral over all classical paths x(t) connecting (xa,ta) and (xb,tb),
Kxbxa(tb,ta) = ∫ x(t) D[x(t)]
ei/ |
Connection to classical mechanics. The stationary phase approach
says that when h→0 only the stationary path, that is where
δS/δx=0, gives nonvanishing contribution to the
integral. This is apparently the classical variational principle which
defines the classical path.
Lattice discretization (and regularization). Let us discretize time in N equidistant slices t0=ta,t1,...,tN=tb, with Δt=(tb-ta)/N
Kxbxa(tb,ta) ≈
(m/2π i |
Sn = Δt L[1/2(xn+xn-1),1/Δt(xn-xn-1)] |
Monte-Carlo evaluation of the path integral: generate random paths {x(t1),x(t2),...,x(tN-1)} using some algorithm and add up their contributions to the path integral.
Space discretization With the space discretized also, x={x0,x1,...,xD}, the short-time propagator becomes a complex matrix
Kij(Δt)=(m/2π i |
Imaginary time propagation. Partition function e-βH.
Real time propagation. The energy levels can be extracted by a Fourier transform of the trace of the propagator:
Tr U(t) = ∑n 〈 n | exp(-i/ |
Problems