A general, energy-separable Faber polynomial representation of the full time-independent Green operator is presented. Non-Hermitian Hamiltonians are included, allowing treatment of negative imaginary absorbing potentials. A connection between the Faber polynomial expansion and our earlier Chebychev
Analytic continuation of the polynomial representation of the full, interacting time-independent Green function
β Scribed by Youhong Huang; Wei Zhu; Donald J. Kouri; David K. Hoffman
- Publisher
- Elsevier Science
- Year
- 1993
- Tongue
- English
- Weight
- 389 KB
- Volume
- 214
- Category
- Article
- ISSN
- 0009-2614
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β¦ Synopsis
We present an analytic continuation of a polynomial representation of the fti, interacting time-independent Green function, thereby enabling the use of negative, imaginary absorbing potentials to shorten the grid necessary to treat scattering problems. The approach retains the clean separation of the energy and Hamiltonian dependences characteristic of our earlier orthogonal polynomial representation of the operator (E-H+iO+)-'. This treatment, combined with our time-independent wavepacket Lippmann-Schwinger equation method, leads to a computational approach in which all of the energy dependence resides in known analytical expansion coeefficients. The Hamiltonian operator appears as the argument of other orthogonal polynomials.
These act solely on an initial wavepacket which provides a "universal source" of scattered waves, independent of the particular energies of interest. This energy independence, combined with highly truncated grids, results in an extremely efficient procedure for scattering calculations.
π SIMILAR VOLUMES
to continue the result to the real axis. Numerical analytic continuation, however, is notoriously difficult, and most The need to calculate the spectral properties of a Hermitian operator H frequently arises in the technical sciences. A common ap-techniques developed thus far are useful only for sp