Maria Gatu Johnson
Gerald Hale
Mark Paris
Michael Wiescher
Alex Zylstra- 1Massachusetts Institute of Technology, Cambridge, MA, United States
- 2Los Alamos National Laboratory (DOE), Los Alamos, NM, United States
- 3Department of Physics and Astronomy, University of Notre Dame, Notre Dame, IN, United States
- 4Lawrence Livermore National Laboratory (DOE), Livermore, CA, United States
Editorial on the Research Topic
Using high energy density plasmas for nuclear experiments relevant to nuclear astrophysics
Thermonuclear reaction rates and nuclear processes have traditionally been explored by means of accelerator experiments, which are difficult to execute at conditions relevant to nucleosynthesis. High energy density (HED) plasmas generated using lasers, such as the inertial confinement fusion (ICF) platform, more closely mimic astrophysical environments in several ways, including with thermal distributions of reacting ions as opposed to mono-energetic ions impinging on a cold target; stellar-relevant plasma temperatures and densities; and neutron flux densities not found anywhere else on earth [1]. The most extreme conditions can currently be achieved at the National Ignition Facility (NIF) laser in the US, where densities of 103 g/cm3 and neutron fluxes up to 5⋅1027 neutrons/cm/s [2, 3] have been demonstrated over a time period of a few tens of picoseconds. The HED platform is emerging as an interesting complement to accelerator experiments.
This Research Topic explores the potential of this new platform for helping address questions including nuclear rates in plasmas, plasma effects on nuclear reactions, electron screening, and neutron reactions on excited states, with emphasis placed on how accelerator and HED experiments can complement each other to generate answers. For example, Aliotta and Langanke summarize the current understanding of screening effects in stellar environments. They identify an open question in that accelerator measurements suggest a higher screening potential than expected in the adiabatic limit, and discuss how laser facilities hold promise for solving this problem. In particular, accelerator measurements of charged particle-induced reactions are handicapped by the rapidly declining cross section and the uncertainties in the screening. Thomson describes how the high neutron flux environment in ICF plasmas opens up possibilities for second neutron scattering or reactions on excited states at much higher energies than previously possible. To study these unique reaction paths, the lifetimes of the newly accessible excited states must be understood; he uses statistical Hauser-Feshbach decay models to calculate relevant lifetimes.
At large laser facilities such as the NIF and OMEGA [4], stellar-like conditions are achieved by symmetrically illuminating a target using a large number of high-energy laser beams. This leads to compression of the target materials, which subsequently generates a high-density, high-temperature plasma environment. Using deuterium and tritium as fuel in the target, this process can also produce high neutron yields (up to 1⋅1018 at the NIF) over a short (∼100 ps) time window through fusion reactions. The platform has been successfully used for studying rates of low-Z reactions, using the reactants as fuel in the target, as reported in [5–7] and in Mohamed et al. Future directions for this path of research are explored by Casey et al., who lay the foundations for using this platform to study plasma screening including discussion of practical constraints, and Wiescher et al., who examine feasibility of studying three charged-particle-induced reactions involving mid-Z reactants using this platform. Despotopulos et al. review available techniques for adding small amounts of seed nuclei of interest for stellar nucleosynthesis into or in close proximity to the target for exposure to stellar-like conditions or nucleosynthesis-relevant neutron fluxes.
High neutron fluxes in short time periods can also be achieved using high-power, short-pulse lasers based on chirped pulse amplification [8]. This path to stellar-relevant experiments is the subject of two of the papers in this Research Topic, Jiao et al. and Burggraf and Zylstra.
The HED platform comes with its own challenges. Rapid gradients in space and time must be considered. In some cases, thermalization rates may be lower than plasma confinement times, which means standard hydrodynamic and Maxwellian assumptions must be examined. Crilly et al. address these challenges by theoretically investigating impact of hydrodynamic and kinetic effects on S-factors inferred from ICF-type experiments.
The new platform cannot be exploited without state-of-the-art diagnostics [1, 9, 10]. Despotopulos et al. review the radiochemistry diagnostic suite available at the NIF. Mohamed et al. review gamma detection capabilities available at OMEGA and the NIF, and identify a gamma spectrometer as an additional tool that would enable many more experiments. Additional nuclear diagnostics are also available at the various facilities, and should be exploited as research continues (see, e.g., Refs. [11, 12]).
Broad interdisciplinary nuclear, plasma and astrophysical expertise will be required to tap the potential of this new line of research. The intent with this Research Topic is to advertise the platform’s capabilities to attract the necessary expertise to this emerging field, and to gather momentum behind the efforts to utilize these new capabilities to answer questions previously impossible to address in terrestrial experiments.
Author contributions
MGJ, GH, MP, MW, and AZ co-edited the Research Topic. MGJ wrote the editorial text with feedback and input from MW, GH, MP, and AZ.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.
References
1. Cerjan CJ, Bernstein L, Berzak Hopkins L, Bionta RM, Bleuel DL, Caggiano JA, et al. Dynamic high energy density plasma environments at the National Ignition Facility for nuclear science research. J Phys G: Nucl Part Phys (2018) 45:033003. doi:10.1088/1361-6471/aa8693
2. Abu-Shawareb H, Acree R, Adams P, Adams J, Addis B, Aden R, et al. Lawson criterion for ignition exceeded in an inertial fusion experiment. Phys Rev Lett (2022) 129:075001. doi:10.1103/PhysRevLett.129.075001
3. Zylstra AB, Kritcher AL, Hurricane OA, Callahan DA, Ralph JE, Casey DT, et al. Experimental achievement and signatures of ignition at the national ignition facility. Phys Rev E (2022) 106:025202. doi:10.1103/PhysRevE.106.025202
4. Boehly TR, Brown DL, Craxton RS, Keck RL, Knauer JP, Kelly JH, et al. Initial performance results of the OMEGA laser system. Opt Commun (1997) 133:495. doi:10.1016/s0030-4018(96)00325-2
5. Casey DT, Sayre DB, Brune CR, Smalyuk VA, Weber CR, Tipton RE, et al. Thermonuclear reactions probed at stellar-core conditions with laser-based inertial-confinement fusion. Nat Phys (2017) 13(12):1227. doi:10.1038/nphys4220
6. Zylstra AB, Herrmann HW, Gatu Johnson M, Kim YH, Frenje JA, Hale G, et al. Using inertial fusion implosions to measure the T + 3He fusion cross section at nucleosynthesis-relevant energies. Phys Rev Lett (2016) 117:035002. doi:10.1103/PhysRevLett.117.035002
7. Zylstra AB, Herrmann HW, Kim YH, McEvoy A, Frenje JA, Johnson MG, et al. 2H(ρ,γ)3He cross section measurement using high-energy-density plasmas. Phys Rev C (2020) 101:042802(R). doi:10.1103/physrevc.101.042802
8. Strickland D, Mourou G. Compression of amplified chirped optical pulses. Opt Commun (1985) 56:219. doi:10.1016/0030-4018(85)90120-8
9. Gatu Johnson M, Zylstra AB, Bacher A, Brune CR, Casey DT, Forrest C, et al. Development of an inertial confinement fusion platform to study charged-particle-producing nuclear reactions relevant to nuclear astrophysics. Phys Plasmas (2017) 24:041407. doi:10.1063/1.4979186
10. Gatu Johnson M, Casey DT, Hohenberger M, Zylstra AB, Bacher A, Brune CR, et al. Optimization of a high-yield, low-areal-density fusion product source at the National Ignition Facility with applications in nucleosynthesis experiments. Phys Plasmas (2018) 25:056303. doi:10.1063/1.5017746
11. Moore AS, Schlossberg DJ, Appelbe BD, Chandler GA, Crilly AJ, Eckart MJ, et al. Neutron time of flight (nToF) detectors for inertial fusion experiments. Rev Sci Instrum (2023).
Keywords: nuclear astrophysics, nucleosynthesis, plasma screening, high energy density physics (HEDP), national ignition facility (NIF), omega laser facility, short-pulse laser experiments, charged-particle-induced reactions
Citation: Gatu Johnson M, Hale G, Paris M, Wiescher M and Zylstra A (2023) Editorial: Using high energy density plasmas for nuclear experiments relevant to nuclear astrophysics. Front. Phys. 11:1180821. doi: 10.3389/fphy.2023.1180821
Received: 06 March 2023; Accepted: 13 March 2023;
Published: 20 March 2023.
Edited and reviewed by:
Jie Meng, Peking University, ChinaCopyright © 2023 Gatu Johnson, Hale, Paris, Wiescher and Zylstra. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Maria Gatu Johnson, Z2F0dUBwc2ZjLm1pdC5lZHU=