دورية أكاديمية

57 Zn β-delayed proton emission establishes the 56 Ni rp-process waiting point bypass

التفاصيل البيبلوغرافية
العنوان: 57 Zn β-delayed proton emission establishes the 56 Ni rp-process waiting point bypass
المؤلفون: Saxena, M., J Ong, W., Meisel, Z., Hoff, D. E.M., Smirnova, N., Bender, P. C., Burcher, S. P., Carpenter, M. P., Carroll, J. J., Chester, A., Chiara, C. J., Conaway, R., Copp, P. A., Crider, B. P., Derkin, J., Estradé, A., Hamad, G., Harke, J. T., Jain, R., Jayatissa, H., Liddick, S. N., Longfellow, B., Mogannam, M., Montes, F., Nepal, N., Ogunbeku, T. H., Richard, A. L., Schatz, H., Soltesz, D., Subedi, S. K.
المصدر: Physics & Astronomy Open Access Publications
بيانات النشر: OHIO Open Library
سنة النشر: 2022
المجموعة: OHIO Open Library (Ohio University)
مصطلحات موضوعية: Type-1 X-ray bursts, Waiting-point, β-decay measurement of proton rich isotope
الوصف: We measured the Zn57 β-delayed proton (βp) and γ emission at the National Superconducting Cyclotron Laboratory. We find a Zn57 half-life of 43.6±0.2 ms, βp branching ratio of (84.7±1.4)%, and identify four transitions corresponding to the exotic β-γ-p decay mode, the second such identification in the fp-shell. The p/γ ratio was used to correct for isospin mixing while determining the Zn57 mass via the isobaric multiplet mass equation. Previously, it was uncertain as to whether the rp-process flow could bypass the textbook waiting point Ni56 for astrophysical conditions relevant to Type-I X-ray bursts. Our results definitively establish the existence of the Ni56 bypass, with 14-17% of the rp-process flow taking this route.
نوع الوثيقة: text
وصف الملف: text/html
اللغة: unknown
العلاقة: https://ohioopen.library.ohio.edu/physics-astronomy-oapub/168Test; https://doi.org/10.1016/j.physletb.2022.137059Test
DOI: 10.1016/j.physletb.2022.137059
الإتاحة: https://doi.org/10.1016/j.physletb.2022.137059Test
https://ohioopen.library.ohio.edu/physics-astronomy-oapub/168Test
رقم الانضمام: edsbas.98B5387A
قاعدة البيانات: BASE