Direct Measurement of 59Cu(p,α)56Ni Precludes a Strong NiCu Cycle in Type-I X-Ray Bursts

Model-observation comparisons of type-I X-ray bursts (XRBs) can reveal the properties of accreting neutron star systems, including the neutron star compactness. XRBs are powered by nuclear burning, and a handful of reactions have been shown to impact the model results. Reactions in the NiCu cycles,...

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Autors principals:	N. Bhathi, J. S. Randhawa, R. Kanungo, J. Refsgaard, M. Alcorta, T. Ahn, C. Andreoiu, D. Bardayan, S. S. Bhattacharjee, B. Davids, G. Christian, A. A. Chen, R. Coleman, P. E. Garrett, G. F. Grinyer, E. Gyabeng Fuakye, G. Hackman, R. Jain, K. Kapoor, R. Krücken, A. Laffoley, A. Lennarz, J. Liang, Z. Meisel, A. Psaltis, A. Radich, M. Rocchini, J. S. Rojo, N. Saei, M. Saxena, M. Singh, C. E. Svensson, P. Subramaniam, A. Talebitaher, S. Upadhyayula, C. Waterfield, J. Williams, M. Williams, M. A. Zubair
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	X-ray bursts Nuclear astrophysics Explosive nucleosynthesis
Accés en línia:	https://doi.org/10.3847/1538-4357/ae3de6
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