Matches in SemOpenAlex for { <https://semopenalex.org/work/W2031878470> ?p ?o ?g. }
- W2031878470 abstract "There is recent evidence that some SiC $X$ grains from the Murchison meteorite may contain supernova-produced $ensuremath{nu}$-process $^{11}mathrm{B}$ and or $^{7}mathrm{Li}$ encapsulated in the grains. The synthesis of $^{11}mathrm{B}$ and $^{7}mathrm{Li}$ via neutrino-induced nucleon emission (the $ensuremath{nu}$ process) in supernovas is sensitive to the neutrino mass hierarchy for finite ${sin}^{2}2{ensuremath{theta}}_{13}>0.001$. This sensitivity arises because, when there is 13 mixing, the average electron neutrino energy for charged-current neutrino reactions is larger for a normal mass hierarchy than for an inverted hierarchy. Recent constraints on ${ensuremath{theta}}_{13}$ from the Daya Bay, Double Chooz, MINOS, RENO, and T2K collaborations all suggest that indeed ${sin}^{2}2{ensuremath{theta}}_{13}>0.001$. We examine the possible implications of these new results based upon a Bayesian analysis of the uncertainties in the measured meteoritic material and the associated supernova nucleosynthesis models. We show that although the uncertainties are large, they hint at a marginal preference for an inverted neutrino mass hierarchy. We discuss the possibility that an analysis of more $X$ grains enriched in $mathrm{Li}$ and $mathrm{B}$ along with a better understanding of the relevant stellar nuclear and neutrino reactions could eventually reveal the neutrino mass hierarchy." @default.
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- W2031878470 date "2012-05-22" @default.
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- W2031878470 title "Exploring the neutrino mass hierarchy probability with meteoritic supernova material,<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>ν</mml:mi></mml:math>-process nucleosynthesis, and<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msub><mml:mi>θ</mml:mi><mml:mn>13</mml:mn></mml:msub></mml:math>mixing" @default.
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- W2031878470 doi "https://doi.org/10.1103/physrevd.85.105023" @default.
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