تقرير
Single-particle shell strengths near the doubly magic nucleus $^{56}$Ni and the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate in explosive astrophysical burning
العنوان: | Single-particle shell strengths near the doubly magic nucleus $^{56}$Ni and the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate in explosive astrophysical burning |
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المؤلفون: | Kahl, D., Woods, P. J., Poxon-Pearson, T., Nunes, F. M., Brown, B. A., Schatz, H., Baumann, T., Bazin, D., Belarge, J. A., Bender, P. C., Elman, B., Estrade, A., Gade, A., Kankainen, A., Lederer-Woods, C., Lipschutz, S., Longfellow, B., Lonsdale, S. -J., Lunderberg, E., Montes, F., Ong, W. J., Perdikakis, G., Pereira, J., Sullivan, C., Taverner, R., Weisshaar, D., Zegers, R. |
المصدر: | Physics Letters B 797 (2019) 134803 |
سنة النشر: | 2019 |
المجموعة: | Astrophysics Nuclear Experiment Nuclear Theory |
مصطلحات موضوعية: | Nuclear Experiment, Astrophysics - Solar and Stellar Astrophysics, Nuclear Theory |
الوصف: | Angle-integrated cross-section measurements of the $^{56}$Ni(d,n) and (d,p) stripping reactions have been performed to determine the single-particle strengths of low-lying excited states in the mirror nuclei pair $^{57}$Cu-$^{57}$Ni situated adjacent to the doubly magic nucleus $^{56}$Ni. The reactions were studied in inverse kinematics utilizing a beam of radioactive $^{56}$Ni ions in conjunction with the GRETINA $\gamma$-array. Spectroscopic factors are compared with new shell-model calculations using a full $pf$ model space with the GPFX1A Hamiltonian for the isospin-conserving strong interaction plus Coulomb and charge-dependent Hamiltonians. These results were used to set new constraints on the $^{56}$Ni(p,$\gamma$)$^{57}$Cu reaction rate for explosive burning conditions in x-ray bursts, where $^{56}$Ni represents a key waiting point in the astrophysical rp-process. Comment: Final version accepted and published. 5 pages, 2 figures |
نوع الوثيقة: | Working Paper |
DOI: | 10.1016/j.physletb.2019.134803 |
URL الوصول: | http://arxiv.org/abs/1907.11665 |
رقم الأكسشن: | edsarx.1907.11665 |
قاعدة البيانات: | arXiv |
DOI: | 10.1016/j.physletb.2019.134803 |
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