T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*

We have studied the energy dependence of the reaction mechanism of the T(t,2n)[superscript 4] He reaction at stellar energies and of its charge symmetric analog reaction [superscript 3]He([superscript 3]He,2p)[superscript 4] He at energies up 10 MeV. We find that the reaction mechanism changes drama...

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Main Authors: Bacher, A.D., Brune, C.R, Sayre, D.B., Hale, G.M., Frenje, J.A., Gatu Johnson, Maria
Other Authors: Massachusetts Institute of Technology. Plasma Science and Fusion Center
Format: Article
Published: EDP Sciences 2018
Online Access:http://hdl.handle.net/1721.1/114267
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author Bacher, A.D.
Brune, C.R
Sayre, D.B.
Hale, G.M.
Frenje, J.A.
Gatu Johnson, Maria
author2 Massachusetts Institute of Technology. Plasma Science and Fusion Center
author_facet Massachusetts Institute of Technology. Plasma Science and Fusion Center
Bacher, A.D.
Brune, C.R
Sayre, D.B.
Hale, G.M.
Frenje, J.A.
Gatu Johnson, Maria
author_sort Bacher, A.D.
collection MIT
description We have studied the energy dependence of the reaction mechanism of the T(t,2n)[superscript 4] He reaction at stellar energies and of its charge symmetric analog reaction [superscript 3]He([superscript 3]He,2p)[superscript 4] He at energies up 10 MeV. We find that the reaction mechanism changes dramatically over this energy range in part due to the interference of the two identical fermions in the three-body final state.
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spelling mit-1721.1/1142672022-09-30T11:29:55Z T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV* Bacher, A.D. Brune, C.R Sayre, D.B. Hale, G.M. Frenje, J.A. Gatu Johnson, Maria Massachusetts Institute of Technology. Plasma Science and Fusion Center Gatu Johnson, Maria We have studied the energy dependence of the reaction mechanism of the T(t,2n)[superscript 4] He reaction at stellar energies and of its charge symmetric analog reaction [superscript 3]He([superscript 3]He,2p)[superscript 4] He at energies up 10 MeV. We find that the reaction mechanism changes dramatically over this energy range in part due to the interference of the two identical fermions in the three-body final state. 2018-03-23T17:36:21Z 2018-03-23T17:36:21Z 2016-03 2018-02-09T13:38:02Z Article http://purl.org/eprint/type/JournalArticle 2100-014X http://hdl.handle.net/1721.1/114267 Bacher, A. D., et al. “T(T,2n)[superscript 4] He and [superscript 3] He([superscript 3] He,2p)[superscript 4] He: The Reaction Mechanism from Solar Energies to 10 MeV.” EPJ Web of Conferences, edited by C. Elster et al., vol. 113, 2016, p. 03003. http://dx.doi.org/10.1051/epjconf/201611303003 EPJ Web of Conferences Creative Commons Attribution 4.0 International License https://creativecommons.org/licenses/by/4.0/ application/pdf EDP Sciences
spellingShingle Bacher, A.D.
Brune, C.R
Sayre, D.B.
Hale, G.M.
Frenje, J.A.
Gatu Johnson, Maria
T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title_full T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title_fullStr T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title_full_unstemmed T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title_short T(T,2n)[superscript 4]He and [superscript 3]He([superscript 3]He,2p)[superscript 4]He: The Reaction Mechanism from Solar Energies to 10 MeV*
title_sort t t 2n superscript 4 he and superscript 3 he superscript 3 he 2p superscript 4 he the reaction mechanism from solar energies to 10 mev
url http://hdl.handle.net/1721.1/114267
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