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• W4285093018 abstract "Evidence for the presence of short-lived radioactive isotopes when the Solar System formed is preserved in meteorites, providing insights into the conditions at the birth of our Sun. A low-mass core-collapse supernova had been postulated as a candidate for the origin of $^{10}mathrm{Be}$, reinforcing the idea that a supernova triggered the formation of the Solar System. We present a detailed study of the production of $^{10}mathrm{Be}$ by the $ensuremath{nu}$ process in supernovae, which is very sensitive to the reaction rate of the major destruction channel, $^{10}mathrm{Be}{(p,ensuremath{alpha})}^{7}text{Li}$. With data from recent nuclear experiments that show the presence of a resonant state in $^{11}mathrm{B}$ at $ensuremath{approx}193$ keV, we derive new values for the $^{10}mathrm{Be}{(p,ensuremath{alpha})}^{7}text{Li}$ reaction rate, which are significantly higher than previous estimates. We show that, with the new $^{10}mathrm{Be}{(p,ensuremath{alpha})}^{7}text{Li}$ reaction rate, a low-mass CCSN is unlikely to produce enough $^{10}mathrm{Be}$ to explain the observed $^{10}mathrm{Be}/^{9}mathrm{Be}$ ratio in meteorites, even for a wide range of neutrino spectra considered in our models." @default.
• W4285093018 created "2022-07-14" @default.
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• W4285093018 date "2022-07-12" @default.
• W4285093018 modified "2023-10-18" @default.
• W4285093018 title "Role of low-lying resonances for the <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts /><mml:none /><mml:mn>10</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>α</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts /><mml:none /><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction rate and implications for the formation of the Solar System" @default.
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• W4285093018 doi "https://doi.org/10.1103/physrevc.106.015803" @default.
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