Two Laser-Driven Nuclear Physics (LDNP) flagship experiments have been identified for the NSF OPAL Laser Facility

Jul 3, 2024, 10:10 AM
40m
Aula Renzo Leonardi (ECT*)

Aula Renzo Leonardi

ECT*

Strada delle Tabarelle 286, I-38123 Villazzano (Trento)

Speaker

Dr Chad Forrest (University of Rochester)

Description

Laser-ion acceleration mechanisms provide a unique opportunity for generating radioactive tritium beams, which are currently not available at accelerator facilities. Few datasets exist of tritium-induced reactions involving light, neutron rich nuclei like 6He, 8Li and 11Be. However, these nuclei are of high interest for nuclear science because influence the r-process as “seed nuclei” [Ter01] and are also predicted to exhibit exotic structure [Qua18, Coc12, For05]. A new platform at the OMEGA-EP laser system at the University of Rochester (UR) Laboratory for Laser Energetics (LLE) is now in a position to support nuclear science experimentation [Sch22]. In a pilot study, 10x^13 tritons were accelerated to several MeV and directed onto a deuterated target, producing 108 fusion neutrons. Follow-up experiments using lithium and beryllium targets to measure the cross sections of di-neutron transfer reactions on these light nuclei will be discussed. This material is based upon work supported by the Department of Energy [National Nuclear Security Administration] University of Rochester “National Inertial Confinement Fusion Program” under Award Number(s) DE-NA0004144.

[Coc12] Cockrell et al: “Lithium isotopes within the ab-initio no-core full configuration approach” Physical Review C 86 (2012)
[For05] Forssen et al: “Large basis ab initio shell model investigation of 9Be and 11Be”, Physical Review C 71 (2005)
[Qua18] Quaglioni et al: “Three cluster dynamics within the ab initio no-core shell model with continuum: How many-body correlations and a clustering shape 6He”, Physical Review C 97 (2018)
[Sch22] A. Schwemmlein et al: “First Demonstration of a Triton Beam Using Target Normal
Sheath Acceleration”, Nuclear Inst. and Methods in Physics Research B 522 (2022)
[Ter01] M. Terasawa et al: “New nuclear reaction flow during r-process nucleosynthesis in supernovae: Critical role of light, neutron-rich nuclei’, The Astrophysical Journal, 562 (2001)

Primary authors

Dr Chad Forrest (University of Rochester) Dr Ani Aprahamian (University of Notre Dame) Dr Arnold Schwemmlein (University of Rochester) Dr Udo Schroeder (University of Rochester) Dr Michael Wiescher (University of Notre Dame)

Presentation materials