Frontiers in Physics (Jan 2023)

High deuteron and neutron yields from the interaction of a petawatt laser with a cryogenic deuterium jet

  • X. Jiao,
  • C. B. Curry,
  • C. B. Curry,
  • M. Gauthier,
  • H.-G. J. Chou,
  • H.-G. J. Chou,
  • F. Fiuza,
  • J. B. Kim,
  • D. D. Phan,
  • E. McCary,
  • E. C. Galtier,
  • G. M. Dyer,
  • B. K. Ofori-Okai,
  • L. Labun,
  • O. Z. Labun,
  • C. Schoenwaelder,
  • C. Schoenwaelder,
  • R. Roycroft,
  • G. Tiwari,
  • G. D. Glenn,
  • G. D. Glenn,
  • F. Treffert,
  • F. Treffert,
  • S. H. Glenzer,
  • B. M. Hegelich,
  • B. M. Hegelich

DOI
https://doi.org/10.3389/fphy.2022.964696
Journal volume & issue
Vol. 10

Abstract

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A compact high-flux, short-pulse neutron source would have applications from nuclear astrophysics to cancer therapy. Laser-driven neutron sources can achieve fluxes much higher than spallation and reactor neutron sources by reducing the volume and time in which the neutron-producing reactions occur by orders of magnitude. We report progress towards an efficient laser-driven neutron source in experiments with a cryogenic deuterium jet on the Texas Petawatt laser. Neutrons were produced both by laser-accelerated multi-MeV deuterons colliding with Be and mixed metallic catchers and by d (d,n)3He fusion reactions within the jet. We observed deuteron yields of 1013/shot in quasi-Maxwellian distributions carrying ∼8−10% of the input laser energy. We obtained neutron yields greater than 1010/shot and found indications of a deuteron-deuteron fusion neutron source with high peak flux (>1022 cm−2 s−1). The estimated fusion neutron yield in our experiment is one order of magnitude higher than any previous laser-induced dd fusion reaction. Though many technical challenges will have to be overcome to convert this proof-of-principle experiment into a consistent ultra-high flux neutron source, the neutron fluxes achieved here suggest laser-driven neutron sources can support laboratory study of the rapid neutron-capture process, which is otherwise thought to occur only in astrophysical sites such as core-collapse supernova, and binary neutron star mergers.

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