and 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}
}
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https://doi.org/10.1016/j.physletb.2016.04.021
https://doi.org/10.1016/j.physletb.2016.04.021
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Cited by: 48 works
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Works referencing / citing this record:
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- Gales, S.; Tanaka, K. A.; Balabanski, D. L.
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- Physical Review C, Vol. 100, Issue 5
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