1956
DOI: 10.1143/ptp.16.507
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Helium Capturing Reactions in Stars

Abstract: 507The generation of 12C, 16() and 20Ne by successive a-capturing proc•sses in the helium core of stars is calculated under the condition at temperature-10°°K. The rat Show more

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Cited by 14 publications
(20 citation statements)
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(23 reference statements)
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“…The synthesis of helium into carbon in stars proceeds via resonant reaction, namely the three α particles fuse into an excited energy level in the 12 C nucleus. The rate of the reaction was calculated before the existence of this level was known and was found to be very low compared to the rate of destruction of 12 C by collisions with α particles.…”
Section: What Is the Hoyle Levelmentioning
confidence: 99%
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“…The synthesis of helium into carbon in stars proceeds via resonant reaction, namely the three α particles fuse into an excited energy level in the 12 C nucleus. The rate of the reaction was calculated before the existence of this level was known and was found to be very low compared to the rate of destruction of 12 C by collisions with α particles.…”
Section: What Is the Hoyle Levelmentioning
confidence: 99%
“…The rate of the reaction was calculated before the existence of this level was known and was found to be very low compared to the rate of destruction of 12 C by collisions with α particles. As a consequence, it was impossible to predict the evolution off the main sequence towards the Red-Giant branch and the calculation implied that all the 12 C is converted into 16 O.…”
Section: What Is the Hoyle Levelmentioning
confidence: 99%
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