Helium burning of 40Ca☆
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Cited by (27)
Nuclear Structure and Decay Data for A=44 Isobars
2023, Nuclear Data SheetsNuclear Data Sheets for A = 44
2011, Nuclear Data SheetsFirst results from the nuclear astrophysics AMS program at the NSL using the MANTIS system in gas-filled mode
2008, Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and AtomsThe <sup>40</sup>Ca(α, γ)<sup>44</sup>Ti reaction at DRAGON
2007, Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and AtomsCitation Excerpt :Since the reaction 40Ca(α, γ)44Ti is the main process for the nucleosynthesis of 44Ti, it has a strong influence on the final 44Ti yield. This reaction was studied in the past by prompt γ-ray spectrometry in the energy range of Eα = 3.5–4.6 MeV [8] and Eα = 2.75–4.00 MeV [9], which correspond to stellar temperatures of T9 = 1.7–2.2 and T9 = 1.2–2.1, respectively (T9 = T/109 K). Resonance strengths were measured for 12 isolated narrow resonances.
Experiments in Nuclear Astrophysics
2007, Nuclear Physics A
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