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Extreme brightness laser-based neutron pulses as a pathway for investigating nucleosynthesis in the laboratory
- Source :
- Matter and Radiation at Extremes, Matter and Radiation at Extremes, AIP Publishing 2019, 4 (5), pp.054402. ⟨10.1063/1.5081666⟩, Matter and Radiation at Extremes, Vol 4, Iss 5, Pp 054402-054402-10 (2019), Matter and Radiation at Extremes, 2019, 4 (5), pp.054402. ⟨10.1063/1.5081666⟩
- Publication Year :
- 2019
- Publisher :
- HAL CCSD, 2019.
-
Abstract
- With the much-anticipated multi-petawatt (PW) laser facilities that are coming online, neutron sources with extreme fluxes could soon be in reach. Such sources would rely on spallation by protons accelerated by the high-intensity lasers. These high neutron fluxes would make possible not only direct measurements of neutron capture and β-decay rates related to the r-process of nucleosynthesis of heavy elements, but also such nuclear measurements in a hot plasma environment, which would be beneficial for s-process investigations in astrophysically relevant conditions. This could, in turn, finally allow possible reconciliation of the observed element abundances in stars and those derived from simulations, which at present show large discrepancies. Here, we review a possible pathway to reach unprecedented neutron fluxes using multi-PW lasers, as well as strategies to perform measurements to investigate the r- and s-processes of nucleosynthesis of heavy elements in cold matter, as well as in a hot plasma environment.With the much-anticipated multi-petawatt (PW) laser facilities that are coming online, neutron sources with extreme fluxes could soon be in reach. Such sources would rely on spallation by protons accelerated by the high-intensity lasers. These high neutron fluxes would make possible not only direct measurements of neutron capture and β-decay rates related to the r-process of nucleosynthesis of heavy elements, but also such nuclear measurements in a hot plasma environment, which would be beneficial for s-process investigations in astrophysically relevant conditions. This could, in turn, finally allow possible reconciliation of the observed element abundances in stars and those derived from simulations, which at present show large discrepancies. Here, we review a possible pathway to reach unprecedented neutron fluxes using multi-PW lasers, as well as strategies to perform measurements to investigate the r- an...
- Subjects :
- Physics
Nuclear and High Energy Physics
Brightness
Astrophysics::High Energy Astrophysical Phenomena
Plasma
01 natural sciences
Atomic and Molecular Physics, and Optics
010305 fluids & plasmas
Nuclear physics
Stars
Neutron capture
Nuclear Energy and Engineering
Nucleosynthesis
[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]
0103 physical sciences
Neutron source
lcsh:QC770-798
Neutron
Spallation
lcsh:Nuclear and particle physics. Atomic energy. Radioactivity
Electrical and Electronic Engineering
010306 general physics
Nuclear Experiment
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
ComputingMilieux_MISCELLANEOUS
Subjects
Details
- Language :
- English
- ISBN :
- 978-92-0-150410-4
- ISSN :
- 2468080X
- ISBNs :
- 9789201504104
- Database :
- OpenAIRE
- Journal :
- Matter and Radiation at Extremes, Matter and Radiation at Extremes, AIP Publishing 2019, 4 (5), pp.054402. ⟨10.1063/1.5081666⟩, Matter and Radiation at Extremes, Vol 4, Iss 5, Pp 054402-054402-10 (2019), Matter and Radiation at Extremes, 2019, 4 (5), pp.054402. ⟨10.1063/1.5081666⟩
- Accession number :
- edsair.doi.dedup.....4f5a1e9fb102555097e4880d772095fe
- Full Text :
- https://doi.org/10.1063/1.5081666⟩