• L. Varga
  • J. Glorius
  • M. Aliotta
  • K. Blaum
  • L. Bott
  • C. Brandau
  • B. Brückner
  • C. G. Bruno
  • X. Chen
  • R. Chen
  • S. Dababneh
  • T. Davinson
  • D. Dmytriiev
  • S. F. Dellmann
  • I. Dillmann
  • P. Erbacher
  • S. Fiebiger
  • O. Forstner
  • T. Gaßner
  • K. Göbel
  • S. Goriely
  • C. J. Griffin
  • R. E. Grisenti
  • M. Groothuis
  • A. Gumberidze
  • G. Gyürky
  • M. Heil
  • R. Hensch
  • R. Hess
  • P.-M. Hillenbrand
  • P. Hillmann
  • O. Hinrichs
  • R. Joseph
  • B. Jurado
  • T. Kausch
  • K. Khasawneh
  • A. Khodaparast
  • T. Kisselbach
  • N. Klapper
  • C. Kozhuharov
  • D. Kurtulgil
  • G. J. Lane
  • C. Langer
  • G. Leckenby
  • C. Lederer-Woods
  • M. Lestinsky
  • Yu. A. Litvinov
  • S. Litvinov
  • B. Löher
  • E. Lorenz
  • B. Lorentz
  • P. Marini
  • J. Marsh
  • E. Menz
  • T. Morgenroth
  • T. T. Nguyen
  • F. Nolden
  • N. Petridis
  • U. Popp
  • A. Psaltis
  • M. Reed
  • R. Reifarth
  • M. S. Sanjari
  • D. Savran
  • M. Sguazzin
  • H. Simon
  • R. S. Sidhu
  • Z. Slavkovská
  • U. Spillmann
  • M. Steck
  • T. Stöhlker
  • J. Stumm
  • A. Surzhykov
  • J. Swartz
  • T. Szücs
  • A. Taremi Zadeh
  • B. Thomas
  • H. Törnqvist
  • M. Träger
  • C. Trageser
  • S. Trotsenko
  • D. Vescovi
  • M. Volknandt
  • H. Weick
  • M. Weigand
  • C. Wolf
  • P. J. Woods
  • Y. M. Xing
  • T. Yamaguchi
We report the application of the new elimination of Rutherford elastic scattering technique for the measurement of proton-induced reaction cross sections utilizing stored ions decelerated to astrophysical energies. This approach results in a background reduction factor of about 1 order of magnitude, enabling the first measurement of a (p, n) cross section in a storage ring. Here, the reaction channels Xe124(p,n) and Xe124(p,γ) have been studied just above the neutron threshold energy. The new data provide valuable constraints for Hauser-Feshbach theory and extrapolation of the (p,γ) cross section to lower energies. Most importantly, for nuclei of limited availability, the method represents a powerful improvement to efficiently study proton-induced reactions at energies within or close to the astrophysical Gamow window, bringing many reaction measurements within reach that were previously inaccessible in the laboratory.
Original languageEnglish
Article number082701
Number of pages7
JournalPhysical Review Letters
Volume134
Issue number8
DOIs
StatePublished - 28 Feb 2025

ID: 133776791