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Measurement of the 91 Zr(p, γ ) 92 m Nb cross section motivated by type Ia supernova nucleosynthesis
(2021-09-14)
Abstract: The synthesis of heavy, proton rich isotopes is a poorly understood astrophysical process. Thermonuclear (type Ia) supernova explosions are among the suggested sites and the abundance of some isotopes present in ...