Journal Article
Evaluation of the N 13 (a,p) O 16 thermonuclear reaction rate and its impact on the isotopic composition of supernova grains
Meyer, A., De Séréville, N., Laird, A. M., Hammache, F., Longland, R., Lawson, T., …Tatischeff, V. (2020). Evaluation of the N 13 (a,p) O 16 thermonuclear reaction rate and its impact on the isotopic composition of supernova grains. Physical Review C, 102(3), https://doi.org/10.1103/PhysRevC.102.035803
Shell-model studies of the astrophysical rp -process reactions S 34 (p,?) Cl 35 and Cl 34g,m (p,?) Ar 35
Richter, W. A., Brown, B. A., Longland, R., Wrede, C., Denissenkov, P., Fry, C., …Reifarth, R. (2020). Shell-model studies of the astrophysical rp -process reactions S 34 (p,?) Cl 35 and Cl 34g,m (p,?) Ar 35. Physical Review C, 102(2), https://doi.org/10.1103/PhysRevC.102.025801
Origin of Large Meteoritic SiC Stardust Grains in Metal-rich AGB Stars
Dell'Agli, F., D'Orazi, V., Schönb chler, M., Lugaro, M., Cseh, B., Világos, B., …Nittler, L. R. (2020). Origin of Large Meteoritic SiC Stardust Grains in Metal-rich AGB Stars. The Astrophysical journal, 898(2), https://doi.org/10.3847/1538-4357/ab9e74
The Nucleosynthetic Yields of Core-collapse Supernovae: Prospects for the Next Generation of Gamma-Ray Astronomy
Andrews, S., Fryer, C., Even, W., Jones, S., & Pignatari, M. (2020). The Nucleosynthetic Yields of Core-collapse Supernovae: Prospects for the Next Generation of Gamma-Ray Astronomy. The Astrophysical journal, 890(1), https://doi.org/10.3847/1538-4357/ab64f8
Research interests
My main research interest is about how elements are made in stars, from small stars like our Sun, to the biggest stars that will explode as supernovae.
I am a member of several international collaborations focused on nuclear astrophysics, galactic archaeology and cosmochemistry, including NuGrid, the UK network BRIDGCE, JINA-CEE, the COST Action ChETEC, and the NSF Accelnet network IReNA.
Postgraduate supervision
Nuclear astrophysics, cosmochemistry, stellar evolution and nucleosynthesi