Gail McLaughlin
0000-0001-6811-6657
3 papers found
Refreshing results…
Actinide-rich and Actinide-poor r-process-enhanced Metal-poor Stars Do Not Require Separate r-process Progenitors
Using excitation-energy dependent fission yields to identify key fissioning nuclei in r-process nucleosynthesis
Californium-254 and Kilonova Light Curves
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