Exploring laser-driven neutron sources for neutron capture cascades and the production of neutron-rich isotopes
arXiv:2004.07953 · doi:10.1103/PhysRevC.103.014602
Abstract
The production of neutron-rich isotopes and the occurrence of neutron capture cascades via laser-driven (pulsed) neutron sources are investigated theoretically. The considered scenario involves the interaction of a laser-driven neutron beam with a target made of a single type of seed nuclide. We present a comprehensive study over seed nuclides in the range from Li to Fm. For each element, the heaviest sufficiently-long-lived (half life h) isotope whose data is available in the recent ENDF-B-VIII.0 neutron sublibrary is considered. We identify interesting seed nuclides with good performance in the production of neutron-rich isotopes where neutron capture cascades may occur. The effects of the neutron number per pulse, the neutron-target interaction size and the number of neutron pulses are also analyzed. Our results show the possibility of observing up to successive neutron capture events leading to neutron-rich isotopes with more neutrons than the original seed nuclide. This hints at new experimental possibilities to produce neutron-rich isotopes and simulate neutron capture nucleosynthesis in the laboratory. With several selected interesting seed nuclides in the region of the branching point of the -process (Sb, Lu and Re) or the waiting point of the -process (Lu, Re, Os, Tm, Ir and Au), we expect that laser-driven experiments can shed light on our understanding of nucleosynthesis.
arXiv comment23 pages, 8 figures, 1 table; discussions added; accepted for publication in Physical Review C
References in corpus (44)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
- Astrophysical Reaction Rates From Statistical Model Calculations
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
- The s Process: Nuclear Physics, Stellar Models, Observations
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
- Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta
- The impact of individual nuclear properties on -process nucleosynthesis
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- Neutron Star Mergers and Nucleosynthesis of Heavy Elements
- Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger
- Tables of Nuclear Cross Sections and Reaction Rates: an Addendum to the Paper "Astrophysical Reaction Rates from Statistical Model Calculations"
- Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger
- Merger and Mass Ejection of Neutron-Star Binaries
- The Dynamics of Binary Neutron Star Mergers and of GW170817
- Current Status of r-Process Nucleosynthesis
- r-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutron Star Mergers
- From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
- The first direct double neutron star merger detection: implications for cosmic nucleosynthesis
- r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
- Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
- Current Status and Future Potential of Nuclide Discoveries
- On the Dynamics of Proto-Neutron Star Winds and r-Process Nucleosynthesis
- Physical conditions for the r-process I. radioactive energy sources of kilonovae
- Introducing the Fission-Fusion Reaction Process: Using a Laser-Accelerated Th Beam to produce Neutron-Rich Nuclei towards the N=126 Waiting Point of the r Process
- Early signal of emerging nuclear collectivity in neutron-rich Sb
- Determination of plasma screening effects for thermonuclear reactions in laser-generated plasmas
- 2014 Update of the Discoveries of Nuclides
- 2013 Update of the discoveries of nuclides
- 2018 Update of the Discoveries of Nuclides
- 2016 Update of the discovery of nuclides
- 2015 Update of the Discoveries of Isotopes
- Neutron production from thermonuclear reactions in laser-generated plasmas
- 2017 Update of the Discoveries of Nuclides