Quantum star-graph analogues of PT-symmetric square wells. II: Spectra
arXiv:1411.3828 · doi:10.1139/cjp-2014-0475
Abstract
For non-Hermitian equilateral q-pointed star-shaped quantum graphs of paper I [Can. J. Phys. 90, 1287 (2012), arXiv 1205.5211] we show that due to certain dynamical aspects of the model as controlled by the external, rotation-symmetric complex Robin boundary conditions, the spectrum is obtainable in a closed asymptotic-expansion form, in principle at least. Explicit formulae up to the second order are derived for illustration, and a few comments on their consequences are added.
arXiv comment12 pages, 1 figure, a complement of part I (arXiv 1205.5211)
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