Advanced

Study of the (p, γ) and (α, γ) reactions for 96,98,104Ru and 112,114,116Sn at astrophysically relevant energies

Bajpeyi, Awanish; Shukla, A. LU ; Koning, A. J. and Åberg, Sven LU (2017) In Physics of Atomic Nuclei 80(3). p.402-411
Abstract

Cross section and S factor of the proton- and alpha-induced reactions have been studied for the Ruthenium and tin isotopes in the effective energy range, i.e. Gamow window. These reactions are important for developing the understanding for nucleosynthesis, particularly for the synthesis of p nuclei (p process). In this work, cross sections and S factor have been calculated through TALYS in Hauser–Feshbach formalism using nuclear densities calculated in relativistic mean field (RMF) formalism. Calculated results of cross sections, S factor and nuclear structure have been compared with existing theoretical as well as experimental results available and are found to be in good agreement.

Please use this url to cite or link to this publication:
author
organization
publishing date
type
Contribution to journal
publication status
published
subject
in
Physics of Atomic Nuclei
volume
80
issue
3
pages
10 pages
publisher
MAIK Nauka/Interperiodica
external identifiers
  • scopus:85021290402
  • wos:000404148500002
ISSN
1063-7788
DOI
10.1134/S1063778817030024
language
English
LU publication?
yes
id
22d43f3c-3645-4128-8c9a-47d60362b83f
date added to LUP
2017-07-12 12:32:37
date last changed
2017-09-18 11:38:12
@article{22d43f3c-3645-4128-8c9a-47d60362b83f,
  abstract     = {<p>Cross section and S factor of the proton- and alpha-induced reactions have been studied for the Ruthenium and tin isotopes in the effective energy range, i.e. Gamow window. These reactions are important for developing the understanding for nucleosynthesis, particularly for the synthesis of p nuclei (p process). In this work, cross sections and S factor have been calculated through TALYS in Hauser–Feshbach formalism using nuclear densities calculated in relativistic mean field (RMF) formalism. Calculated results of cross sections, S factor and nuclear structure have been compared with existing theoretical as well as experimental results available and are found to be in good agreement.</p>},
  author       = {Bajpeyi, Awanish and Shukla, A. and Koning, A. J. and Åberg, Sven},
  issn         = {1063-7788},
  language     = {eng},
  month        = {05},
  number       = {3},
  pages        = {402--411},
  publisher    = {MAIK Nauka/Interperiodica},
  series       = {Physics of Atomic Nuclei},
  title        = {Study of the (p, γ) and (α, γ) reactions for <sup>96,98,104</sup>Ru and <sup>112,114,116</sup>Sn at astrophysically relevant energies},
  url          = {http://dx.doi.org/10.1134/S1063778817030024},
  volume       = {80},
  year         = {2017},
}