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- W2316109510 endingPage "1970" @default.
- W2316109510 startingPage "1967" @default.
- W2316109510 abstract "We have searched for the reaction d(ensuremath{alpha},ensuremath{gamma}${)}^{6}$Li at an ensuremath{alpha}-d center-of-mass energy of 53 keV. An upper limit on the reaction S factor is 2.0ifmmodetimeselsetexttimesfi{}${10}^{mathrm{ensuremath{-}}7}$ MeV b at the 90% confidence level, corresponding to a limit on the synthesis of $^{6}mathrm{Li}$ from a standard big bang of 0.9% of the present abundance for a total baryon-to-photon ratio 2.86${mathrm{ensuremath{eta}}}_{10}$3.77. Equivalently, the $^{6}mathrm{ensuremath{-}}^{7}$Li isotopic abundance ratio immediately after a standard big bang is constrained to be less than 0.85%, considerably less than a recent measurement of this ratio in a metal-poor, Population II halo star. textcopyright{} 1996 The American Physical Society." @default.
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- W2316109510 date "1996-04-01" @default.
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- W2316109510 title "The reaction<i>d</i>(α,γ<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>Li at low energies and the primordial nucleosynthesis 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…" @default.
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- W2316109510 doi "https://doi.org/10.1103/physrevc.53.1967" @default.
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