Published June 2011 | Version v1
Journal article

The semiclassical small-(ℎ/2π) limit of loci of roots of subdominant solutions for polynomial potentials

  • 1. Jan Dlugosz University in Czestochowa, Institute of Physics, ul. Armii Krajowej 13/15, 42-200 Czestochowa (Poland)

Description

In this paper, a description of the small-(ℎ/2π) limit of loci of zeros of subdominant solutions for polynomial potentials is given called as fundamental solutions in our earlier papers. The considered potentials are those which provide us with the simple turning points only. Three types of Stokes graphs (SG's) associated with the potentials are investigated - the general non-critical ones, the general critical ones but with only single internal Stokes line (SL), and the Stokes graphs corresponding to arbitrary multiple-well real even degree polynomial potentials with internal Stokes lines distributed on the real axis only. All these cases are considered in their both versions of the quantized and not quantized (ℎ/2π). In particular due to the fact that the small-(ℎ/2π) limit is semiclassical it is shown that loci of roots of subdominant solutions in the cases considered are collected along Stokes lines. There are infinitely many roots of subdominant solutions on such lines escaping to infinity and a finite number of them on internal Stokes lines.

Additional details

Identifiers

Publishing Information

Journal Title
Journal of Mathematical Physics
Journal Volume
52
Journal Issue
6
Journal Page Range
p. 063514-063514.44
ISSN
0022-2488
CODEN
JMAPAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42093024
Subject category
S97: MATHEMATICAL METHODS AND COMPUTING;
Descriptors DEI
GRAPH THEORY; MATHEMATICAL SOLUTIONS; POLYNOMIALS; POTENTIALS; SCHROEDINGER EQUATION; SEMICLASSICAL APPROXIMATION
Descriptors DEC
APPROXIMATIONS; CALCULATION METHODS; DIFFERENTIAL EQUATIONS; EQUATIONS; FUNCTIONS; MATHEMATICS; PARTIAL DIFFERENTIAL EQUATIONS; WAVE EQUATIONS

Optional Information

Notes
(c) 2011 American Institute of Physics