University of Hertfordshire

From the same journal

By the same authors

Measurement of the 91 Zr(p, γ ) 92 m Nb cross section motivated by type Ia supernova nucleosynthesis

Research output: Contribution to journalArticlepeer-review

Documents

  • pdf.pdf

    Final published version, 866 KB, PDF document

  • Gy Gyürky
  • Z Halász
  • G G Kiss
  • T Szücs
  • R Huszánk
  • Zs Török
  • Zs Fülöp
  • T Rauscher
  • C Travaglio
View graph of relations
Original languageEnglish
Pages (from-to)105202
JournalJournal of Physics G: Nuclear and Particle Physics
Volume48
Issue10
Early online date14 Sep 2021
DOIs
Publication statusE-pub ahead of print - 14 Sep 2021

Abstract

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 the early Solar System may be used to test the models. 92Nb is such an isotope and one of the reactions playing a role in its synthesis is 91Zr(p,γ)92Nb. As no experimental cross sections were available for this reaction so far, nucleosynthesis models had to solely rely on theoretical calculations. In the present work the cross section of 91Zr(p,γ)92m Nb has been measured at astrophysical energies by activation. The results excellently confirm the predictions of cross sections and reaction rates for 91Zr(p,γ)92Nb, as used in astrophysical simulations.

ID: 25973462