معرفی
Philip Adsley is an Assistant Professor at Texas A&M University's Department of Physics and Astronomy, affiliated with the Cyclotron Institute. His research focuses on nuclear astrophysics, particularly the interplay between nuclear structure and stellar processes. He investigates reaction rates critical for understanding nucleosynthesis in environments like massive stars, supernovae, and x-ray binaries. Key areas include carbon fusion via the Hoyle state, proton-capture reactions in the Mg-Al cycle, and neutron source reactions in the s-process.
His work combines experimental techniques such as transfer reactions and resonance scattering with advanced computational methods like Monte Carlo simulations. Collaborations include institutions like iThemba LABS (South Africa), University of the Witwatersrand, and international teams at TRIUMF (Canada) and INFN (Italy). Recent studies address reaction rates for 12C+12C fusion, 27Al(p,α)24Mg, and 30Si(p,γ)31P, impacting models of stellar evolution and abundance patterns in globular clusters.
Adsley has contributed to reevaluating key reaction rates using novel experimental data, reducing uncertainties in astrophysical predictions. His research often bridges nuclear physics and observational astronomy, with findings published in leading journals like Physical Review Letters and Physics Letters B.
