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The RADIOSTAR Project

Lugaro, Maria; Côté, Benoit; Pignatari, Marco; Yagüe López, Andrés; Brinkman, Hannah; Cseh, Borbála; Den Hartogh, Jacqueline; Doherty, Carolyn Louise; Karakas, Amanda Irene; Kobayashi, Chiaki; Lawson, Thomas; Pető, Mária; Soós, Benjámin; Trueman, Thomas; Világos, Blanka

Authors

Maria Lugaro

Benoit Côté

Marco Pignatari

Andrés Yagüe López

Hannah Brinkman

Borbála Cseh

Jacqueline Den Hartogh

Carolyn Louise Doherty

Amanda Irene Karakas

Chiaki Kobayashi

Mária Pető

Benjámin Soós

Thomas Trueman

Blanka Világos



Abstract

Radioactive nuclei are the key to understanding the circumstances of the birth of our Sun because meteoritic analysis has proven that many of them were present at that time. Their origin, however, has been so far elusive. The ERC-CoG-2016 RADIOSTAR project is dedicated to investigating the production of radioactive nuclei by nuclear reactions inside stars, their evolution in the Milky Way Galaxy, and their presence in molecular clouds. So far, we have discovered that: (i) radioactive nuclei produced by slow (107Pd and182Hf) and rapid (129 I and247Cm) neutron captures originated from stellar sources —asymptotic giant branch (AGB) stars and compact binary mergers, respectively—within the galactic environment that predated the formation of the molecular cloud where the Sun was born; (ii) the time that elapsed from the birth of the cloud to the birth of the Sun was of the order of 107 years, and (iii) the abundances of the very short-lived nuclei26Al,36Cl, and41Ca can be explained by massive star winds in single or binary systems, if these winds directly polluted the early Solar System. Our current and future work, as required to finalise the picture of the origin of radioactive nuclei in the Solar System, involves studying the possible origin of radioactive nuclei in the early Solar System from core-collapse supernovae, investigating the production of107Pd in massive star winds, modelling the transport and mixing of radioactive nuclei in the galactic and molecular cloud medium, and calculating the galactic chemical evolution of53Mn and60Fe and of the p-process isotopes92Nb and146Sm.

Citation

Lugaro, M., Côté, B., Pignatari, M., Yagüe López, A., Brinkman, H., Cseh, B., Den Hartogh, J., Doherty, C. L., Karakas, A. I., Kobayashi, C., Lawson, T., Pető, M., Soós, B., Trueman, T., & Világos, B. (2022). The RADIOSTAR Project. Universe, 8(2), Article 130. https://doi.org/10.3390/universe8020130

Journal Article Type Article
Acceptance Date Feb 7, 2022
Online Publication Date Feb 17, 2022
Publication Date Feb 1, 2022
Deposit Date May 2, 2024
Publicly Available Date May 3, 2024
Journal Universe
Electronic ISSN 2218-1997
Publisher MDPI
Peer Reviewed Peer Reviewed
Volume 8
Issue 2
Article Number 130
DOI https://doi.org/10.3390/universe8020130
Keywords Short-lived radioactivity; Early Solar System; Stellar nucleosynthesis; Galactic chemical evolution
Public URL https://hull-repository.worktribe.com/output/3928514

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Copyright Statement
© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).





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