The CWKB approach to non-reflecting potential and cosmological implications
Abstract
We discuss the method of calculating the reflection coefficient using complex trajectory WKB (CWKB) approximation. This enables us to give an interpretation of non-reflecting nature of the potential under certain conditions and clarify some points, reported incorrectly elsewhere [vs:ejp] for the potential . We show that the repeated reflectios between the turning points are essential, which most authors overlooked, in obtaining the non-reflecting c ondition. We find that the considered repeated reflection paths are in conformity with Bogolubov transformation technique. We discuss the implications of the results when applied to the particle production scenario, considering as a time variable and also stress the cosmological implications of the result with reference to radiation domonated and de Sitter spacetime.
Keywords
Cite
@article{arxiv.gr-qc/0207015,
title = {The CWKB approach to non-reflecting potential and cosmological implications},
author = {S. Biswas and I. Chowdhury},
journal= {arXiv preprint arXiv:gr-qc/0207015},
year = {2008}
}
Comments
9 pages, latex