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- W2970086707 abstract "The existence of $^{12}{rm C} + {}^{16}{rm O}$ molecular resonances at sub-barrier energy has been a significant problem in nuclear astrophysics because they strongly affect the $^{12}{rm C} + {}^{16}{rm O}$ fusion reaction rate in type Ia supernovae and heavy stars. However, experimental surveys have been limited to 4~MeV and cannot access the deep sub-barrier energy due to a very small fusion cross section. Here we predict a couple of resonances with $J^pi=0^+$, $2^+$, and $4^+$ in the deep sub-barrier energy based on the antisymmetrized molecular dynamics calculation that reproduces the known resonances and low-lying spectrum of $^{28}{rm Si}$." @default.
- W2970086707 created "2019-09-05" @default.
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- W2970086707 date "2020-01-01" @default.
- W2970086707 modified "2023-09-26" @default.
- W2970086707 title "<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML altimg=si1.svg><mml:mmultiscripts><mml:mrow><mml:mi mathvariant=normal>C</mml:mi></mml:mrow><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>12</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo linebreak=goodbreak linebreakstyle=after>+</mml:mo><mml:msup><mml:mrow /><mml:mrow><mml:mn>16</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant=normal>O</mml:mi></mml:math> molecular resonances at deep sub-barrier energy" @default.
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- W2970086707 doi "https://doi.org/10.1016/j.physletb.2019.135086" @default.
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