2013
DOI: 10.14311/ap.2013.53.0534
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THE <sup>2</sup>H(α, γ)<sup>6</sup>LI REACTION AT LUNA AND BIG BANG NUCLEOSYNTHETIS

Abstract: Abstract.The 2 H(α, γ) 6 Li reaction is the leading process for the production of 6 Li in standard Big Bang Nucleosynthesis. Recent observations of lithium abundance in metal-poor halo stars suggest that there might be a 6 Li plateau, similar to the well-known Spite plateau of 7 Li. This calls for a re-investigation of the standard production channel for 6 Li. As the 2 H(α, γ) 6 Li cross section drops steeply at low energy, it has never before been studied directly at Big Bang energies. For the first time the … Show more

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Cited by 3 publications
(3 citation statements)
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“…The D( 4 He,γ) 6 Li cross section -which is the key reaction for the determination of the primordial abundance of 6 Li -has been measured (e.g. Gustavino, 2007Gustavino, , 2009Gustavino, , 2011aGustavino, ,b, 2012Gustavino, , 2013, as well as that of 2 H(α,γ) 6 Li (Anders et al, 2013), and 2 H(α,γ) 6 Li (Anders et al, 2014).…”
Section: Pos(golden2019)001mentioning
confidence: 99%
“…The D( 4 He,γ) 6 Li cross section -which is the key reaction for the determination of the primordial abundance of 6 Li -has been measured (e.g. Gustavino, 2007Gustavino, , 2009Gustavino, , 2011aGustavino, ,b, 2012Gustavino, , 2013, as well as that of 2 H(α,γ) 6 Li (Anders et al, 2013), and 2 H(α,γ) 6 Li (Anders et al, 2014).…”
Section: Pos(golden2019)001mentioning
confidence: 99%
“…The D( 4 He,γ) 6 Li cross section -which is the key reaction for the determination of the primordial abundance of 6 Li -has been measured (e.g. Gustavino, 2007Gustavino, , 2009Gustavino, , 2011Gustavino, , 2012Gustavino, , 2013, as well as that of 2 H(α,γ) 6 Li (Anders et al, 2013), and 2 H(α,γ) 6 Li (Anders et al, 2014).…”
Section: Nuclear Reactions In Starsmentioning
confidence: 99%
“…The D( 4 He,γ) 6 Li cross section-which is the key reaction for the determination of the primordial abundance of 6 Li-has been measured (e.g. Gustavino 2007Gustavino , 2009Gustavino , 2011Gustavino , 2012Gustavino , 2013, as well as that of 2 H(α,γ) 6 Li (Anders et al 2013), and 2 H(α,γ) 6 Li (Anders et al 2014).…”
Section: Nuclear Reactions In Starsmentioning
confidence: 99%