Samuel Turner

Samuel Turner is a Postdoctoral Research Associate at the Department of Applied Mathematics and Theoretical Physics (DAMTP) within the Faculty of Mathematics at the University of Cambridge. He previously completed his PhD in Astrophysics at the Institute of Astronomy, University of Cambridge (2019–2023). His research focuses on understanding accretion disc dynamics through stochastic modeling and high-energy astrophysical phenomena, including tidal disruption events and X-ray variability.

Education:

• PhD in Astrophysics, Institute of Astronomy, University of Cambridge (2019–2023)

Research Interests: Turner’s work centers on astrophysical accretion discs, utilizing stochastic methods to model their variability and structure. He investigates high-energy phenomena such as X-ray eruptions following tidal disruption events and explores the turbulent processes in accretion discs around compact objects. His studies also extend to white dwarf atmospheric pollution and the composition of accreted planetesimals.

Publications: His recent works include groundbreaking studies on quasi-periodic X-ray eruptions linked to tidal disruption events and the development of 2D stochastic methodologies to simulate accretion disc fluctuations. These contributions highlight his expertise in combining theoretical models with observational data to advance understanding of astrophysical systems.

Awards: No scientific awards listed.

Advising and Grants: No advising roles or grants mentioned. Turner’s current position at DAMTP positions him within the Astrophysics research group, contributing to cutting-edge studies in high-energy astrophysics and accretion processes.

Labs/Teams: Affiliated with the Astrophysics group at DAMTP, University of Cambridge.