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Title: He 3 ( α , γ ) Be 7 and H 3 ( α , γ ) Li 7 astrophysical S factors from the no-core shell model with continuum

Abstract

The 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical S factors are calculated within the no-core shell model with continuum using a renormalized chiral nucleon–nucleon interaction. The 3He(α,γ)7Be astrophysical S factors agree reasonably well with the experimental data while the 3H(α,γ)7Li ones are overestimated. The seven-nucleon bound and resonance states and the α + 3He/3H elastic scattering are also studied and compared with experiment. Here, the low-lying resonance properties are rather well reproduced by our approach. At low energies, the s-wave phase shift, which is non-resonant, is overestimated.

Authors:
; ; ; ; ;
Publication Date:
Research Org.:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP)
OSTI Identifier:
1247077
Alternate Identifier(s):
OSTI ID: 1343010
Report Number(s):
LLNL-JRNL-678557
Journal ID: ISSN 0370-2693; S0370269316300946; PII: S0370269316300946
Grant/Contract Number:  
AC52-07NA27344; SCW1158
Resource Type:
Published Article
Journal Name:
Physics Letters B
Additional Journal Information:
Journal Name: Physics Letters B Journal Volume: 757 Journal Issue: C; Journal ID: ISSN 0370-2693
Publisher:
Elsevier
Country of Publication:
Netherlands
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; nuclear physics; light-nuclei radiative captures; Ab initio calculation

Citation Formats

Dohet-Eraly, Jérémy, Navrátil, Petr, Quaglioni, Sofia, Horiuchi, Wataru, Hupin, Guillaume, and Raimondi, Francesco. He 3 ( α , γ ) Be 7 and H 3 ( α , γ ) Li 7 astrophysical S factors from the no-core shell model with continuum. Netherlands: N. p., 2016. Web. doi:10.1016/j.physletb.2016.04.021.
Dohet-Eraly, Jérémy, Navrátil, Petr, Quaglioni, Sofia, Horiuchi, Wataru, Hupin, Guillaume, & Raimondi, Francesco. He 3 ( α , γ ) Be 7 and H 3 ( α , γ ) Li 7 astrophysical S factors from the no-core shell model with continuum. Netherlands. https://doi.org/10.1016/j.physletb.2016.04.021
Dohet-Eraly, Jérémy, Navrátil, Petr, Quaglioni, Sofia, Horiuchi, Wataru, Hupin, Guillaume, and Raimondi, Francesco. Wed . "He 3 ( α , γ ) Be 7 and H 3 ( α , γ ) Li 7 astrophysical S factors from the no-core shell model with continuum". Netherlands. https://doi.org/10.1016/j.physletb.2016.04.021.
@article{osti_1247077,
title = {He 3 ( α , γ ) Be 7 and H 3 ( α , γ ) Li 7 astrophysical S factors from the no-core shell model with continuum},
author = {Dohet-Eraly, Jérémy and Navrátil, Petr and Quaglioni, Sofia and Horiuchi, Wataru and Hupin, Guillaume and Raimondi, Francesco},
abstractNote = {The 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical S factors are calculated within the no-core shell model with continuum using a renormalized chiral nucleon–nucleon interaction. The 3He(α,γ)7Be astrophysical S factors agree reasonably well with the experimental data while the 3H(α,γ)7Li ones are overestimated. The seven-nucleon bound and resonance states and the α + 3He/3H elastic scattering are also studied and compared with experiment. Here, the low-lying resonance properties are rather well reproduced by our approach. At low energies, the s-wave phase shift, which is non-resonant, is overestimated.},
doi = {10.1016/j.physletb.2016.04.021},
journal = {Physics Letters B},
number = C,
volume = 757,
place = {Netherlands},
year = {Wed Jun 01 00:00:00 EDT 2016},
month = {Wed Jun 01 00:00:00 EDT 2016}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1016/j.physletb.2016.04.021

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