Carina Nebula JWST Image credit: NASA, ESA, CSA, and STScI

Artemis Tsantiri

I am a Postdoctoral Research Fellow at the University of Regina working with Prof. Gwen Grinyer on experiments at TRIUMF. I obtained my PhD in nuclear astrophysics at the Facility for Rare Isotope Beams at Michigan State University working under Prof. Artemis Spyrou in the SuN group. I received my diploma from the School of Applied Mathematical and Physical Sciences of the National Technical University of Athens with Prof. Mike Kokkoris as my supervisor.

I am interested nuclear astrophysics, the study of the mechanisms that form the chemical elements in the cosmos. By using experimental techniques I study nuclear reactions that take place inside stars.

News

    2025

    PhD thesis work published on Phys. Rev. Letters

    The main results of my PhD thesis have been published in Physical Review Letters. This work is the first measurement of the 73As(p,γ)74Se reaction, marking only the second measurement of a reaction relevant to the γ process in the astrophysically important energy range with a radioactive ion beam. The experiment was performed at the Facility for Rare Isotope Beams using the SuN detector. These measurements provide improved constraints for models describing the production of a rare group of nuclei known as the p nuclei in exploding massive stars.

    Invited Talk

    I was honored to give my first invited talk at the BRIDGCE-IReNA 2025 Annual Meeting, where I presented my PhD thesis work on the production of 74Se in the astrophysical γ process. It was a great opportunity to share my research and connect with many new researchers. I am grateful to the organizers for the invite and to IReNA for supporting my attendance.

    PhD Thesis Defense

    On March 17th, 2025, I successfully defended my PhD thesis!

    The work regards to proton-capture cross-section measurements for the astrophysical γ process, with main focus on the first measurement of 73As(p,γ)74Se, one of the main destruction mechanisms of the lightest p nucleus, 74Se. Using network calculations of the γ process in Type II supernovae, we showed that our measured cross section significantly reduces the uncertainty in 74Se production!

Publications

    2024

  • Spyrou et al, May 2024, Phys. Rev. Lett. 132, 202701
    First Study of the 139Ba(n,γ)140Ba Reaction to Constrain the Conditions for the Astrophysical i Process
  • Cox et al, April 2024, Phys. Rev. Lett. 132, 152503
    Proton Shell Gaps in N = 28 Nuclei from the First Complete Spectroscopy Study with FRIB Decay Station Initiator

    2023

  • Pogliano et al, June 2023, Phys. Rev. C 107, 064614
    Experimentally constrained 165,166Ho(n,γ) rates and implications for the s process
  • Tsantiri et al, March 2023, Phys. Rev. C 107, 035808
    Cross-section measurement of the 82Kr(p,γ)83Rb reaction in inverse kinematics

    2022

  • Palmisano-Kyle et al, June 2022, Phys. Rev. C 105, 065804
    Constraining the astrophysical p process: Cross section measurement of the 84Kr(p,γ)85Rb reaction in inverse kinematics

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