Observation of the Capture Reaction<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi> </mml:mi><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Li</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>6</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>and Its Role in Production of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Li</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>6</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>in the Big Bang
R. G. H. RobertsonP. DyerR. A. WarnerR. C. MelinT. J. BowlesA. B. McDonaldG. C. BallW.G. DaviesE. D. Earle
1995lv
ABI
Abstract
The conclusion that, even if the baryon density is no higher than the density of observable matter in galaxies (about 3 X 10 ' gcm ), less than 2% of the universal Li can be primordial in origin was based on the abundance of Li in old, Population-II stars. For those objects, Li/H = 1.2 X 10 'o [1]. In fact, the present-day galactic abundance of Li is much higher (Reeves
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Cited by 80 references