1994
DOI: 10.1086/173783
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New measurement of the (12)C(n, gamma)(13)C reaction cross section

Abstract: The cross section of 12 C+ 12 C fusion reactions determines the conditions of carbon ignition in stars. The presence of structures, which are likely to extend to low energies, makes the extrapolation of data collected at high energy to the stellar energy difficult and potentially inaccurate, so a direct measurement is desirable. Here we report on an extremely improbable two-step background process which prohibits the measurement of the 12 C(12 C,p) 23 Na carbon fusion reaction at low energies in the presence o… Show more

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Cited by 66 publications
(46 citation statements)
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“…6). It should be mentioned here that the latter two γ-rays were not observed clearly in the previous experiment at E n ≤ 200 keV [2].…”
Section: 3mentioning
confidence: 50%
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“…6). It should be mentioned here that the latter two γ-rays were not observed clearly in the previous experiment at E n ≤ 200 keV [2].…”
Section: 3mentioning
confidence: 50%
“…In spite of this, we have recently succeeded to detect discrete γ-rays from the 12 C(n, γ) 13 C reaction for incident neutron energies in the keV region by developing a highly sensitive discrete γ-ray detection system. We have already reported on the measurement performed at neutron energies up to E n = 200 keV [2]. Here we report on the results obtained at much higher energy, E n = 550 keV.…”
Section: Introductionmentioning
confidence: 85%
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