New approach to folding with the Coulomb wave function
dc.contributor.author | Blokhintsev, L. | |
dc.contributor.author | Kadyrov, Alisher | |
dc.contributor.author | Mukhamedzhanov, A. | |
dc.contributor.author | Savin, D. | |
dc.date.accessioned | 2017-01-30T10:40:00Z | |
dc.date.available | 2017-01-30T10:40:00Z | |
dc.date.created | 2015-10-29T04:09:18Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Blokhintsev, L. and Kadyrov, A. and Mukhamedzhanov, A. and Savin, D. 2015. New approach to folding with the Coulomb wave function. Journal of Mathematical Physics. 56 (5): Article ID 052102. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/4546 | |
dc.identifier.doi | 10.1063/1.4919674 | |
dc.description.abstract |
© 2015 AIP Publishing LLC. Due to the long-range character of the Coulomb interaction theoretical description of low-energy nuclear reactions with charged particles still remains a formidable task. One way of dealing with the problem in an integral-equation approach is to employ a screened Coulomb potential. A general approach without screening requires folding of kernels of the integral equations with the Coulomb wave. A new method of folding a function with the Coulomb partial waves is presented. The partial-wave Coulomb function both in the configuration and momentum representations is written in the form of separable series. Each term of the series is represented as a product of a factor depending only on the Coulomb parameter and a function depending on the spatial variable in the configuration space and the momentum variable if the momentum representation is used. Using a trial function, the method is demonstrated to be efficient and reliable. | |
dc.publisher | American Institute of Physics Inc. | |
dc.title | New approach to folding with the Coulomb wave function | |
dc.type | Journal Article | |
dcterms.source.volume | 56 | |
dcterms.source.number | 5 | |
dcterms.source.issn | 0022-2488 | |
dcterms.source.title | Journal of Mathematical Physics | |
curtin.department | Department of Physics and Astronomy | |
curtin.accessStatus | Fulltext not available |
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