Abstract
The differential photoneutron cross section for ${\mathrm{Mg}}^{26}$ at 135\ifmmode^\circ\else\textdegree\fi{} has been measured as a function of photon energy from 10 keV to 1.5 MeV above threshold by the threshold photoneutron technique. Several prominent resonances have observed, including one located at 54.3 keV above threshold. The existence of this resonance in the ${\mathrm{Mg}}^{26}$ compound system might provide, through the reaction ${\mathrm{Ne}}^{22}(\ensuremath{\alpha}, n){\mathrm{Mg}}^{25}$, the primary production mechanism for neutrons in stars.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
