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1. Proton branching ratios of Mg23 levels

   https://doi.org/10.1103/PhysRevC.105.025801  

   Kim, C. H. ; Chae, K. Y. ; Ahn, S. ; Bardayan, D. W. ; Chipps, K. A. ; Cizewski, J. A. ; Howard, M. E. ; Kozub, R. L. ; Kwag, M. S. ; Kwak, K. ; et al ( February 2022 , Physical Review C)
2. Two-neutron knockout as a probe of the composition of states in Mg22,Al23 , and Si24

   https://doi.org/10.1103/PhysRevC.101.031303  

   Longfellow, B. ; Gade, A. ; Tostevin, J. A. ; Simpson, E. C. ; Brown, B. A. ; Magilligan, A. ; Bazin, D. ; Bender, P. C. ; Bowry, M. ; Elman, B. ; et al ( March 2020 , Physical Review C)
3. Investigation of direct capture in the Na23(p,γ)Mg24 reaction

   https://doi.org/10.1103/PhysRevC.106.045801  

   Boeltzig, A. ; deBoer, R. J. ; Chen, Y. ; Best, A. ; Couder, M. ; Di Leva, A. ; Frentz, B. ; Görres, J. ; Gyürky, Gy. ; Imbriani, G. ; et al ( October 2022 , Physical Review C)
4. New Experimental 23 Na(α, p) 26 Mg Reaction Rate for Massive Star and Type Ia Supernova Models

   https://doi.org/10.3847/1538-4357/abee91  

   Hubbard, N. J. ; Diget, C. Aa. ; Fox, S. P. ; Fynbo, H. O. U. ; Howard, A. M. ; Kirsebom, O. S. ; Laird, A. M. ; Munch, M. ; Parikh, A. ; Pignatari, M. ; et al ( May 2021 , The Astrophysical Journal)

   The²³Na(α,p)²⁶Mg reaction has been identified as having a significant impact on the nucleosynthesis of several nuclei between Ne and Ti in Type Ia supernovae, and of²³Na and²⁶Al in massive stars. The reaction has been subjected to renewed experimental interest recently, motivated by high uncertainties in early experimental data and in the statistical Hauser-Feshbach models used in reaction rate compilations. Early experiments were affected by target deterioration issues and unquantifiable uncertainties. Three new independent measurements instead are utilizing inverse kinematics and Rutherford scattering monitoring to resolve this. In this work we present directly measured angular distributions of the emitted protons to eliminate a discrepancy in the assumptions made in the recent reaction rate measurements, which results in cross sections differing by a factor of 3. We derive a new combined experimental reaction rate for the²³Na(α,p)²⁶Mg reaction with a total uncertainty of 30% at relevant temperatures. Using our new²³Na(α,p)²⁶Mg rate, the²⁶Al and²³Na production uncertainty is reduced to within 8%. In comparison, using the factor of 10 uncertainty previously recommended by the rate compilation STARLIB,²⁶Al and²³Na production was changing by more than a factor of 2. In Type Ia supernova conditions, the impact on production of²³Na is constrained to within 15%.

    

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5. First Direct Measurement of C12(C12,n)Mg23 at Stellar Energies

   https://doi.org/10.1103/PhysRevLett.114.251102  

   Bucher, B. ; Tang, X. D. ; Fang, X. ; Heger, A. ; Almaraz-Calderon, S. ; Alongi, A. ; Ayangeakaa, A. D. ; Beard, M. ; Best, A. ; Browne, J. ; et al ( June 2015 , Physical Review Letters)