Measurements of the T+T neutron energy spectrum from magnetically confined fusion plasmas

ORAL

Abstract

Neutron spectroscopy can be used to study fuel composition and velocity distributions in fusion plasmas. To this end, it is necessary to have a good understanding of the nuclear physics processes at play in the fusion reactions between the fuel ions deuterium (D) and tritium (T). The fusion of two tritons, T + T → n + n + 4He, is particularly challenging in this regard, as it involves a three-body final state; the neutron energy spectrum is therefore not only determined by the velocity distributions of the reactants, but is also affected by interactions between the three reaction products.



In this contribution we present measurements of the T+T neutron spectrum from JET, and their interpretation in terms of an R-matrix model [1] for the three-body final state. The analysis builds on results presented in [2], now including a more careful investigation of the angular dependence of the neutron energy spectrum, caused by the fact that the majority of the T+T neutrons from these JET plasmas were produced in beam-target reactions.



The results show how neutron spectroscopy measurements of magnetically confined fusion plasmas can contribute to the understanding of the nuclear physics processes involved in the T+T reaction, but also highlights that fusion neutron spectroscopy could benefit from further studies of the T+T fusion reactions in more controlled environments, e.g. accelerator facilities.



[1] C. Brune et al, Phys. Rev. C 92 014003 (2015)

[2] B. Eriksson et al, Phys. Rev. C 109 054620 (2024)

*This work has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Programme (Grant Agreement No 101052200 — EUROfusion). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them.This work was supported by the U.S. Department of Energy, Grants No. DE-FG02-88ER40387 and No. DE-NA0004065

Publication: B. Eriksson et al, Phys. Rev. C, vol 109, 054620 (2024) [https://doi.org/10.1103/PhysRevC.109.054620]

Presenters

  • Jacob Eriksson

    • Uppsala University

Authors

  • Jacob Eriksson

    • Uppsala University
  • Benjamin Eriksson

    • Uppsala University
  • Carl Richard Brune

    • Ohio University
  • Sean Conroy

    • Uppsala University
  • Göran Ericsson

    • Uppsala University
  • Maria Gatu Johnson

    • Massachusetts Institute of Technology
    • MIT Plasma Science and Fusion Center
  • Zamir Ghani

    • UKAEA
  • Anders Hjalmarsson

    • Uppsala University
  • Marco Malosti

    • Uppsala University
  • Massimo Nocente

    • University of Milan, Bicocca