The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system

Diehl, R.; Lugaro, M.; Heger, A.; Sieverding, A.; Tang, X.; Li, K. A.; Li, E. T.; Doherty, C. L.; Krause, M. H.; Wallner, A.; Prantzos, N.; Brinkman, H. E.; den Hartogh, J. W.; Wehmeyer, B.; Yagüe López, A.; Pleintinger, M. M.; Banerjee, P.; Wang, W.

doi:10.1017/pasa.2021.48

Title: The radioactive nuclei ²⁶Al and ⁶⁰Fe in the Cosmos and in the solar system

Journal Article · Thu Dec 09 00:00:00 EST 2021 · Publications of the Astronomical Society of Australia

DOI:https://doi.org/10.1017/pasa.2021.48· OSTI ID:1855649

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Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Eotvos Lorand Univ., Budapest (Hungary); Monash Univ., Melbourne, VIC (Australia)
Monash Univ., Melbourne, VIC (Australia); Australian Research Council Centre of Excellence for Gravitational Wave Discovery, Clayton (Australia); Center of Excellence for Astrophysics in Three Dimensions (Australia); ; Michigan State Univ., East Lansing, MI (United States)
Univ. of Minnesota, Minneapolis, MN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Chinese Academy of Sciences (CAS), Lanzhou (China)
ShenZhen Univ., Shenzhen (China)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Monash Univ., Melbourne, VIC (Australia)
Univ. of Hertfordshire, Hatfield (United Kingdom)
Institute of Ion Beam Physics and Materials Research, Dresden (Germany); Australian National Univ., Canberra, ACT (Australia)
Institut d’Astrophysique, Paris (France)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Univ. of Szeged (Hungary)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Univ. of Hertfordshire, Hatfield (United Kingdom)
Indian Inst. of Technology (IIT), Palakkad (India)
Wuhan Univ. (China)

The cosmic evolution of the chemical elements from the Big Bang to the present time is driven by nuclear fusion reactions inside stars and stellar explosions. A cycle of matter recurrently re-processes metal-enriched stellar ejecta into the next generation of stars. The study of cosmic nucleosynthesis and this matter cycle requires the understanding of the physics of nuclear reactions, of the conditions at which the nuclear reactions are activated inside the stars and stellar explosions, of the stellar ejection mechanisms through winds and explosions, and of the transport of the ejecta towards the next cycle, from hot plasma to cold, star-forming gas. Due to the long timescales of stellar evolution, and because of the infrequent occurrence of stellar explosions, observational studies are challenging, as they have biases in time and space as well as different sensitivities related to the various astronomical methods. Here, we describe in detail the astrophysical and nuclear-physical processes involved in creating two radioactive isotopes useful in such studies, ²⁶Al and ⁶⁰Fe. Due to their radioactive lifetime of the order of a million years, these isotopes are suitable to characterise simultaneously the processes of nuclear fusion reactions and of interstellar transport. We describe and discuss the nuclear reactions involved in the production and destruction of ²⁶Al and ⁶⁰Fe, the key characteristics of the stellar sites of their nucleosynthesis and their interstellar journey after ejection from the nucleosynthesis sites. This allows us to connect the theoretical astrophysical aspects to the variety of astronomical messengers presented here, from stardust and cosmic-ray composition measurements, through observation of γ rays produced by radioactivity, to material deposited in deep-sea ocean crusts and to the inferred composition of the first solids that have formed in the Solar System. We show that considering measurements of the isotopic ratio of ²⁶Al to ⁶⁰Fe eliminate some of the unknowns when interpreting astronomical results, and discuss the lessons learned from these two isotopes on cosmic chemical evolution. This review paper has emerged from an ISSI-BJ Team project in 2017–2019, bringing together nuclear physicists, astronomers, and astrophysicists in this inter-disciplinary discussion.

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Research Organization:: Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)

Sponsoring Organization:: USDOE; European Cooperation in Science and Technology; Australian Research Council (ARC); National Science Foundation (NSF)

Grant/Contract Number:: AC05-00OR22725; FG02-87ER40328; 724560; CA16117; PHY-1430152

OSTI ID:: 1855649

Journal Information:: Publications of the Astronomical Society of Australia, Vol. 38, Issue 1; ISSN 1323-3580

Publisher:: CSIROCopyright Statement

Country of Publication:: United States

Language:: English

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Title: The radioactive nuclei ²⁶Al and ⁶⁰Fe in the Cosmos and in the solar system