New Phase Space Calculations for β-Decay Half-Lives

We revisit the computation of the phase space factors (PSF) involved in the positron decay and EC processes for a large number of nuclei of experimental interest. To obtain the electron/positron wave functions, we develop a code for solving accurately the Dirac equation with a nuclear potential deri...

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Main Authors: Sabin Stoica, Mihail Mirea, Ovidiu Niţescu, Jameel-Un Nabi, Mavra Ishfaq
Format: Article
Language:English
Published: Hindawi Limited 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/8729893
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spelling doaj-de919fb47c3f45a18296df9231e0b9c42020-11-24T21:07:17ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/87298938729893New Phase Space Calculations for β-Decay Half-LivesSabin Stoica0Mihail Mirea1Ovidiu Niţescu2Jameel-Un Nabi3Mavra Ishfaq4Horia Hulubei Foundation, P.O. MG6, 077125 Magurele, RomaniaHoria Hulubei Foundation, P.O. MG6, 077125 Magurele, RomaniaHoria Hulubei National Institute of Physics and Nuclear Engineering, P.O. Box MG6, 077125 Magurele, RomaniaGIK Institute of Engineering Sciences and Technology, Topi 23640, Khyber Pakhtunkhwa, PakistanGIK Institute of Engineering Sciences and Technology, Topi 23640, Khyber Pakhtunkhwa, PakistanWe revisit the computation of the phase space factors (PSF) involved in the positron decay and EC processes for a large number of nuclei of experimental interest. To obtain the electron/positron wave functions, we develop a code for solving accurately the Dirac equation with a nuclear potential derived from a realistic proton density distribution in the nucleus. The finite nuclear size (FNS) and screening effects are included through recipes which differ from those used in previous calculations. Comparing our results with previous calculations, performed with the same Q-values, we find a close agreement for positron decays, while, for the EC process, there are relevant differences. For the EC process, we also find that the screening effect has a notable influence on the computed PSF values especially for light nuclei. Further, we recomputed the same PSF values but using the most recent Q-values reported in literature. In several cases, the new Q-values differ significantly from the older ones, leading to large differences in the PSF values as compared with previous results. Our new PSF values can contribute to more reliable calculations of the beta-decay rates, used in the study of nuclei far from the stability line and stellar evolution.http://dx.doi.org/10.1155/2016/8729893
collection DOAJ
language English
format Article
sources DOAJ
author Sabin Stoica
Mihail Mirea
Ovidiu Niţescu
Jameel-Un Nabi
Mavra Ishfaq
spellingShingle Sabin Stoica
Mihail Mirea
Ovidiu Niţescu
Jameel-Un Nabi
Mavra Ishfaq
New Phase Space Calculations for β-Decay Half-Lives
Advances in High Energy Physics
author_facet Sabin Stoica
Mihail Mirea
Ovidiu Niţescu
Jameel-Un Nabi
Mavra Ishfaq
author_sort Sabin Stoica
title New Phase Space Calculations for β-Decay Half-Lives
title_short New Phase Space Calculations for β-Decay Half-Lives
title_full New Phase Space Calculations for β-Decay Half-Lives
title_fullStr New Phase Space Calculations for β-Decay Half-Lives
title_full_unstemmed New Phase Space Calculations for β-Decay Half-Lives
title_sort new phase space calculations for β-decay half-lives
publisher Hindawi Limited
series Advances in High Energy Physics
issn 1687-7357
1687-7365
publishDate 2016-01-01
description We revisit the computation of the phase space factors (PSF) involved in the positron decay and EC processes for a large number of nuclei of experimental interest. To obtain the electron/positron wave functions, we develop a code for solving accurately the Dirac equation with a nuclear potential derived from a realistic proton density distribution in the nucleus. The finite nuclear size (FNS) and screening effects are included through recipes which differ from those used in previous calculations. Comparing our results with previous calculations, performed with the same Q-values, we find a close agreement for positron decays, while, for the EC process, there are relevant differences. For the EC process, we also find that the screening effect has a notable influence on the computed PSF values especially for light nuclei. Further, we recomputed the same PSF values but using the most recent Q-values reported in literature. In several cases, the new Q-values differ significantly from the older ones, leading to large differences in the PSF values as compared with previous results. Our new PSF values can contribute to more reliable calculations of the beta-decay rates, used in the study of nuclei far from the stability line and stellar evolution.
url http://dx.doi.org/10.1155/2016/8729893
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