THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS

The <sup>2</sup>H(α, γ)<sup>6</sup>Li reaction is the leading process for the production of <sup>6</sup>Li in standard Big Bang Nucleosynthesis. Recent observations of lithium abundance in metal-poor halo stars suggest that there might be a 6Li plateau, similar to...

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Main Author: Carlo Gustavino
Format: Article
Language:English
Published: CTU Central Library 2013-12-01
Series:Acta Polytechnica
Online Access:https://ojs.cvut.cz/ojs/index.php/ap/article/view/1892
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author Carlo Gustavino
author_facet Carlo Gustavino
author_sort Carlo Gustavino
collection DOAJ
description The <sup>2</sup>H(α, γ)<sup>6</sup>Li reaction is the leading process for the production of <sup>6</sup>Li in standard Big Bang Nucleosynthesis. Recent observations of lithium abundance in metal-poor halo stars suggest that there might be a 6Li plateau, similar to the well-known Spite plateau of <sup>7</sup>Li. This calls for a re-investigation of the standard production channel for <sup>6</sup>Li. As the <sup>2</sup>H(α, γ)<sup>6</sup>Li cross section drops steeply at low energy, it has never before been studied directly at Big Bang energies. For the first time the reaction has been studied directly at Big Bang energies at the LUNA accelerator. The preliminary data and their implications for Big Bang nucleosynthesis and the purported <sup>6</sup>Li problem will be shown.
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spelling doaj.art-0d3cb02f793149aeac08b9f36ae223502022-12-21T18:52:08ZengCTU Central LibraryActa Polytechnica1210-27091805-23632013-12-0153A10.14311/AP.2013.53.05341882THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETISCarlo Gustavino0INFN Sezione di Roma, I-00185 RomaThe <sup>2</sup>H(α, γ)<sup>6</sup>Li reaction is the leading process for the production of <sup>6</sup>Li in standard Big Bang Nucleosynthesis. Recent observations of lithium abundance in metal-poor halo stars suggest that there might be a 6Li plateau, similar to the well-known Spite plateau of <sup>7</sup>Li. This calls for a re-investigation of the standard production channel for <sup>6</sup>Li. As the <sup>2</sup>H(α, γ)<sup>6</sup>Li cross section drops steeply at low energy, it has never before been studied directly at Big Bang energies. For the first time the reaction has been studied directly at Big Bang energies at the LUNA accelerator. The preliminary data and their implications for Big Bang nucleosynthesis and the purported <sup>6</sup>Li problem will be shown.https://ojs.cvut.cz/ojs/index.php/ap/article/view/1892
spellingShingle Carlo Gustavino
THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
Acta Polytechnica
title THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
title_full THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
title_fullStr THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
title_full_unstemmed THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
title_short THE <sup>2</sup>H(alpha, gamma)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS
title_sort sup 2 sup h alpha gamma sup 6 sup li reaction at luna and big bang nucleosynthetis
url https://ojs.cvut.cz/ojs/index.php/ap/article/view/1892
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