22.–23. Jan. 2026
GSI
Europe/Berlin Zeitzone

Oxygen Abundance in the Early Universe: A Storage Ring Experiment to Verify the Underlying Atomic Data

22.01.2026, 18:00
1 h 30m
Canteen Side Room (GSI)

Canteen Side Room

GSI

Sprecher

Michael Lestinsky (GSI Helmholtzzentrum für Schwerionenforschung GmbH(GSI))

Beschreibung

The energy-resolved merged beams recombination rate coefficient α(E) for dielectronic recombination (DR) of O2+ has been measured on an absolute scale in the energy range from 0 to 45 eV. The experimental data comprises all ∆N=0 DR series associated with 2s → 2p core excitations and the lowest ∆N=1 DR series limits associated with 2p → 3s and 2p → 3d core excitations. In addition, we have performed corresponding quantum theoretical calculations using a freely available atomic code. From the combined experimental and theoretical data, we have derived a temperature-dependent plasma recombination rate coefficient α(T) for dielectronic recombination. In comparison to previously published theoretical data, we find excellent agreement for the temperature range, where O2+ is abundant in high-temperature plasmas dominated by collisional ionization. However, in the temperature range where O2+ exits in photoionized plasmas, our DR rate coefficient is a factor of two larger than the previously published ones. This should be relevant, e.g., for an accurate determination of the recently discovered surprisingly large oxygen abundances in early galaxies.

Autor

Michael Lestinsky (GSI Helmholtzzentrum für Schwerionenforschung GmbH(GSI))

Co-Autoren

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