Experimental Evidence of a Variant Neutron Spectrum from the T(t,2n)α Reaction at Center-of-Mass Energies in the Range of 16–50 keV
Author(s)
Forrest, C. J.; Sayre, D. B.; Bacher, A.; Bourgade, J.-L.; Brune, C. R.; Caggiano, J. A.; Casey, D. T.; Glebov, V. Yu.; Hale, G. M.; Hatarik, R.; Herrmann, H. W.; Janezic, R.; Kim, Y. H.; Knauer, J. P.; Landoas, O.; McNabb, D. P.; Paris, M. W.; Pino, J. E.; Quaglioni, S.; Rosse, B.; Sanchez, J.; Sangster, T. C.; Shmayda, W.; Stoeckl, C.; Thompson, I.; Zylstra, A. B.; Gatu Johnson, Maria; Frenje, Johan A; Petrasso, Richard D; Sio, Hong Weng; ... Show more Show less
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Full calculations of six-nucleon reactions with a three-body final state have been elusive and a long-standing issue. We present neutron spectra from the T(t,2n)α (TT) reaction measured in inertial confinement fusion experiments at the OMEGA laser facility at ion temperatures from 4 to 18 keV, corresponding to center-of-mass energies (E[subscript c.m.]) from 16 to 50 keV. A clear difference in the shape of the TT-neutron spectrum is observed between the two E[subscript c.m.], with the ⁵He ground state resonant peak at 8.6 MeV being significantly stronger at the higher than at the lower energy. The data provide the first conclusive evidence of a variant TT-neutron spectrum in this E[subscript c.m.] range. In contrast to earlier available data, this indicates a reaction mechanism that must involve resonances and/or higher angular momenta than L=0. This finding provides an important experimental constraint on theoretical efforts that explore this and complementary six-nucleon systems, such as the solar ³He(³He,2p)α reaction.
Date issued
2018-07Department
Massachusetts Institute of Technology. Department of Physics; Massachusetts Institute of Technology. Plasma Science and Fusion CenterJournal
Physical Review Letters
Publisher
American Physical Society
Citation
Gatu Johnson, M. et al. "Experimental Evidence of a Variant Neutron Spectrum from the T(t,2n)α Reaction at Center-of-Mass Energies in the Range of 16–50 keV." Physical Review Letters 121, 4 (July 2018): 042501 © 2018 American Physical Society
Version: Final published version
ISSN
0031-9007
1079-7114