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Main Authors: Wehmeyer, Benjamin, López, Andrés Yagüe, Côté, Benoit, Pető, Maria K., Kobayashi, Chiaki, Lugaro, Maria
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2510.13070
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author Wehmeyer, Benjamin
López, Andrés Yagüe
Côté, Benoit
Pető, Maria K.
Kobayashi, Chiaki
Lugaro, Maria
author_facet Wehmeyer, Benjamin
López, Andrés Yagüe
Côté, Benoit
Pető, Maria K.
Kobayashi, Chiaki
Lugaro, Maria
contents We run a three-dimensional Galactic chemical evolution (GCE) model to follow the propagation of Mn-53 from supernovae of type Ia (SNIa), Fe-60 from core-collapse supernovae (CCSNe), Hf-182 from intermediate mass stars (IMSs), and Pu-244 from neutron star mergers (NSMs) in the Galaxy. We compare the GCE of these short-lived radioactive isotopes (SLRs) to recent detections on the deep-sea floor. We find that although these SLRs originate from different sites, they often arrive conjointly on Earth.
format Preprint
id arxiv_https___arxiv_org_abs_2510_13070
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Galactic chemical evolution with the short-lived isotopes Mn-53, Fe-60, Hf-182, and Pu-244
Wehmeyer, Benjamin
López, Andrés Yagüe
Côté, Benoit
Pető, Maria K.
Kobayashi, Chiaki
Lugaro, Maria
Astrophysics of Galaxies
We run a three-dimensional Galactic chemical evolution (GCE) model to follow the propagation of Mn-53 from supernovae of type Ia (SNIa), Fe-60 from core-collapse supernovae (CCSNe), Hf-182 from intermediate mass stars (IMSs), and Pu-244 from neutron star mergers (NSMs) in the Galaxy. We compare the GCE of these short-lived radioactive isotopes (SLRs) to recent detections on the deep-sea floor. We find that although these SLRs originate from different sites, they often arrive conjointly on Earth.
title Galactic chemical evolution with the short-lived isotopes Mn-53, Fe-60, Hf-182, and Pu-244
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2510.13070