Events in our system are self-managed.  Group and event managers are encouraged to review privacy and security settings, and adjust them if needed.  If you need assistance please contact Indico Support - contact Help at bottom of page. https://learn.getindico.io/categories/managing/

16–19 Feb 2023
Banff Centre
Canada/Mountain timezone

Bound-state beta-decay of Thallium-205 to constrain s-process predictions for the early Solar System

18 Feb 2023, 16:15
15m
KC 303 (Banff Centre)

KC 303

Banff Centre

Contributed Oral Nuclear Physics February 18 Afternoon Session

Speaker

Guy Leckenby (TRIUMF)

Description

Bound-state $\beta$-decay ($\beta_b^-$-decay) is a radically transformative decay mode that can change the stability of a nucleus and generate temperature- and density-dependent decay rates. In this decay mode the $\beta$-electron is created directly in a bound atomic orbital of the daughter nucleus instead of being emitted into the continuum, so the decay channel is only significant in almost fully stripped ions during extreme astrophysical conditions. The $\beta_b^-$-decay of $^{205}$Tl$^{81+}$ could influence our understanding of the production of $^{205}$Pb, a short-lived radioactive (SLR) nucleus that is fully produced by the s-process in stars. In the context of the early Solar system, SLRs are defined by half-lives of 0.1-100 My and their abundance in meteorites can be used to constrain the formation of the Solar System [1]. Historically, it has been noted that thermal population of the 2.3 keV state of $^{205}$Pb in stellar conditions could dramatically reduce the abundance of s-process $^{205}$Pb by speeding up the EC-decay to $^{205}$Tl. This destruction of $^{205}$Pb is potentially balanced by the $\beta_b^-$-decay of $^{205}$Tl$^{81+}$ [2]. Currently, a theoretical prediction for the half-life of fully stripped $^{205}$Tl is used in stellar models, but given the importance of the $^{205}$Pb/$^{205}$Pb chronometer, a measurement of the $\beta_b^-$-decay for $^{205}$Tl$^{81+}$ was conducted at the GSI Heavy Ion Facility in March 2020. A $^{205}$Tl$^{81+}$ beam was stored in the Experimental Storage Ring, and the growth of $^{205}$Pb$^{81+}$ daughters with storage time was directly attributable to the $\beta^-_b$-decay channel. The authors will report a preliminary measured half-life and detail how this half-life can be used to more accurately predict the $^{205}$Pb abundance in the early Solar System.
[1] M. Lugaro, et al. Progress in Particle and Nuclear Physics, 102:1–47, 2018.
[2] K. Yokoi, et al. Astronomy and Astrophysics, 145:339–346, 1985.

Your Email gleckenby@triumf.ca
Supervisor Iris Dillmann
Supervisor Email dillmann@triumf.ca
Funding Agency NSERC

Primary authors

Guy Leckenby (TRIUMF) Dr Rui Jiu Chen (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Ragandeep Singh Sidhu (GSI Helmholtzzentrum für Schwerionenforschung GmbH(GSI)) Dr Riccardo Mancino (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Prof. Yuri Litvinov (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Prof. Kohji Takahashi (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Jan Glorius (GSI Helmholtz Center Darmstadt) Prof. Gabriel Martinez Pinedo (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Dr Helmut Weick (GSI Helmholtzzentrum für Schwerionenforschung GmbH) Iris Dillmann (TRIUMF) Chris Griffin (TRIUMF) Dr Marco Pignatari (Konkoly Observatory) Dr Maria Lugaro (Konkoly Observatory) Dr Umberto Battino (University of Hull) Ms Tejpreet Kaur (Panjab University Chandigarh) Dr Sergio Cristallo (National Institute of Astrophysics INAF, Abruzzo Observatory) Dr Diego Vescovi (Goethe University Frankfurt) Dr Thomas Faestermann (Technische Universitat Munchen) Dr Roman Gernhauser (Technische Universitat Munchen)

Presentation materials

There are no materials yet.