2021
DOI: 10.1103/physrevc.103.014602
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Exploring laser-driven neutron sources for neutron capture cascades and the production of neutron-rich isotopes

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Cited by 11 publications
(6 citation statements)
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“…The stable Au isotope represents a waiting point within the nuclear astrophysical r-process heavy element nucleosynthesis. Within the experimental accuracy, the 198m Au yield reached in the present work is in a good agreement with the theoretical study by Hill et al 32 .…”
Section: Resultssupporting
confidence: 93%
See 1 more Smart Citation
“…The stable Au isotope represents a waiting point within the nuclear astrophysical r-process heavy element nucleosynthesis. Within the experimental accuracy, the 198m Au yield reached in the present work is in a good agreement with the theoretical study by Hill et al 32 .…”
Section: Resultssupporting
confidence: 93%
“…Therefore, especially for laboratory nuclear astrophysical studies the development of neutron sources with high neutron-fluxes and neutron energies from tens of keV to several hundreds of keV are of great importance. Recent theoretical studies of the neutron capture cascade using laser-driven neutron sources have shown the feasibility for neutron capture nucleosynthesis in the laboratory 32 .…”
Section: Introductionmentioning
confidence: 99%
“…For this reason, high-flux neutron sources remain an important subject of research and development. Laser-driven neutron sources in particular are a promising approach [5], having already achieved much higher peak neutron fluxes than fission reactors (~10 15 /cm 2 /s) or spallation (~10 17 /cm 2 /s) sources in laboratory experiments, potentially in a more compact facility [6].…”
Section: Introductionmentioning
confidence: 99%
“…It has been proposed to simulate phenomena in stellar plasma [24] and to measure nuclear reaction cross sections in stellar environments [25][26][27][28][29][30]. Pioneer studies using high power lasers were carried out at the University of Texas at Austin [26] and at the National Ignition Facility [29] to study astrophysical S factors.…”
Section: Introductionmentioning
confidence: 99%
“…It has also been suggested to measure stellar (n, γ) reaction cross sections using LDNSs to study the s-process [27]. Furthermore, it has been proposed to produce neutron-rich nuclei heavier than an initial nuclide by at least four neutrons by LDNSs to study the s and r processes [30].…”
Section: Introductionmentioning
confidence: 99%