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

Authors :
Jiao, X.
Curry, C. B.
Gauthier, M.
Chou, H.-G. J.
Fiuza, F.
Kim, J. B.
Phan, D. D.
McCary, E.
Galtier, E. C.
Dyer, G. M.
Ofori-Okai, B. K.
Labun, L.
Labun, O. Z.
Schoenwaelder, C.
Roycroft, R.
Tiwari, G.
Glenn, G. D.
Treffert, F.
Glenzer, S. H.
Hegelich, B. M.
Jiao, X.
Curry, C. B.
Gauthier, M.
Chou, H.-G. J.
Fiuza, F.
Kim, J. B.
Phan, D. D.
McCary, E.
Galtier, E. C.
Dyer, G. M.
Ofori-Okai, B. K.
Labun, L.
Labun, O. Z.
Schoenwaelder, C.
Roycroft, R.
Tiwari, G.
Glenn, G. D.
Treffert, F.
Glenzer, S. H.
Hegelich, B. M.
Publication Year :
2023

Abstract

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.

Details

Database :
OAIster
Notes :
text, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1372646374
Document Type :
Electronic Resource