4–9 Sept 2022
CERN
Europe/Zurich timezone

$^{40}$Ar proposed as probe of neutron-induced reactions in a high-density stellar-like plasma at the National Ignition Facility

5 Sept 2022, 12:15
15m
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium

CERN

400
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Speaker

Michael Paul

Description

The plasma density, temperature and pressure in laser-induced deuterium-tritium (DT) inertial fusion implosions at the National Ignition Facility (NIF) are comparable to those in the center of stars. Neutrons are produced within a radius of $\approx$50 $\mu$m and a time of $\approx$100 ps, representing a uniquely high neutron density approaching 10$^{22}$ cm$^{-3}$, close to that of the astrophysical $r$ process, and fluxes of 10$^{31}$ cm$^{-2}$s$^{-1}$ [1]. Recent experiments at NIF first passed the burning-plasma threshold [2,3], where self-heating exceeded the external heating applied to the fuel and produced record fusion yields of $\approx$1 MJ . In a dedicated NIF high-power laser shot, we plan to investigate neutron-induced reactions on $^{40}$Ar incorporated in the capsule gas. The choice of Ar as probe of such reactions is motivated by the chemical inertness of noble gas Ar allowing for reliable collection of Ar isotopic reaction products and by the existence of three convenient neighboring isotopes $^{39}$Ar ($t_{1/2}=$ 268 y), $^{41}$Ar (110 min) and $^{42}$Ar (33 y). The $^{40}$Ar($n,2n)^{39}$Ar reaction is a direct monitor of the fast-neutron flux; the $^{40}$Ar$(n,\gamma)^{41}$Ar and a potential $^{40}$Ar$(2n,\gamma)^{42}$Ar capture reactions are sensitive to energy downgraded neutrons. A search for $^{42}$Ar may provide an indication of the feasibility to study the important astrophysical $^{58}$Fe$(2n,\gamma)^{60}$Fe reaction [4] in the laboratory. The long-lived $^{39}$Ar and $^{42}$Ar nuclides are detected and counted by Noble-Gas Accelerator Mass Spectrometry (NOGAMS) at Argonne National Laboratory. We report here on a separate first measurement of the total yield of the $^{40}$Ar$(n,2n)^{39}$Ar reaction in a 14 MeV neutron activation. The neutron activation was performed with the DT neutron generator of Technical University Dresden located at Helmholtz-Zentrum Dresden-Rossendorf. First direct ultra-sensitive detection of the $^{42}$Ar nuclide by NOGAMS in a $^{40}$Ar sample activated by the slow double-neutron capture reaction $^{40}$Ar$(n,\gamma)^{41}$Ar$(n,\gamma)^{42}$Ar is demonstrated. The latter activation (8 days) was performed at the high-flux nuclear reactor of Institut Laue-Langevin (Grenoble, France). Preliminary results of these experiments, which will help calibrate the $^{40}$Ar activation at NIF, are presented.

Support from the Pazy Foundation (Israel) and USA-Israel Binational Science Foundation is gratefully acknowledged. This work was supported by the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357. This research used resources of ANL’s ATLAS facility, which is a DOE Office of Science User Facility.

[1] Ch. J. Cerjan et al., J. Phys. G Nucl. Part. Phys. 45, 033003 (2018).
[2] A. B. Zylstra et al., Nature 93, 542 (2022).
[3] A. L. Kritcher et al., Nature Phys. 18, 251 (2022).
[4] W. Wang et al., Astrophys. J. 889, 169 (2020).

Authors

Michael Paul R. N. Sahoo (The Hebrew University of Jerusalem, Jerusalem, Israel 91904) Moshe Tessler (Soreq NRC, Israel) Dr Carol A. Velsko (Lawrence Livermore National Laboratory) Dr Alex B. Zylstra (Lawrence Livermore Natinal Laboratory) Melina Avila (ANL) Clayton Dickerson (Argonne National Lab) Heshani Jayatissa Jake McLain Richard Pardo (Argonne National Laboratory) Dr K. Ernst Rehm (Argonne National Laboratory) Robert Scott (Argonne National Laboratory) Dr Ivan Toltsukhin (Argonne National Laboratory) Richard Vondrasek (Argonne National Laboratory) Mr Thomas Bailey (University of Notre Dame) Ms Lauren Callahan (University of Notre Dame) Mr Adam M. Clark (University of Notre Dame) Prof. Philippe A. Collon (University of Notre Dame) Y. Kashiv ( University of Notre Dame, Notre Dame, IN 46556, USA) Mr Austin Nelson (University of Notre Dame) Ulli Koester (Institut Laue-Langevin (FR)) Mr Hans F. R. Hoffmann (Technical University Dresden) Ms Marie Pichotta Kai Zuber (Technische Universitaet Dresden) Mr Toralf Doering (Helmholtz-Zentrum Dresden-Rossendorf) Ronald Schwengner (Helmholtz-Zentrum Dresden-Rossendorf)

Presentation materials