Impact of transport modeling on the Fe60 abundance inside Galactic cosmic ray sources-Reference-Cited by-同舟云学术

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Impact of transport modeling on the Fe60 abundance inside Galactic cosmic ray sources

Published:2020-04-13 Issue:8 Volume:101 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Morlino Giovanni,Amato Elena

Funder

Kavli Institute for Theoretical Physics, University of California, Santa Barbara

Istituto Nazionale di Astrofisica

National Science Foundation

International Space Science Institute

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.101.083017/fulltext

Reference37 articles.

1. Nucleosynthesis and remnants in massive stars of solar metallicity

2. PRE-SUPERNOVA EVOLUTION OF ROTATING SOLAR METALLICITY STARS IN THE MASS RANGE 13-120M☉AND THEIR EXPLOSIVE YIELDS

3. Observation of the 60 Fe nucleosynthesis-clock isotope in galactic cosmic rays

4. Galactic Cosmic Rays from Supernova Remnants. I. A Cosmic‐Ray Composition Controlled by Volatility and Mass‐to‐Charge Ratio

5. Galactic Cosmic Rays from Supernova Remnants. II. Shock Acceleration of Gas and Dust

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1. Mapping the AMS-02 and CALET data onto the source spectra and residence times of Galactic cosmic rays;Physical Review D;2024-07-19

2. Origin of 60Fe nuclei in cosmic rays: the contribution of local OB associations;Monthly Notices of the Royal Astronomical Society;2024-02-01

3. Cosmic Radioactivity and Galactic Chemical Evolution;Handbook of Nuclear Physics;2023

4. Cosmic Radioactivity and Galactic Chemical Evolution;Handbook of Nuclear Physics;2023

5. Cosmic nucleosynthesis: A multi-messenger challenge;Progress in Particle and Nuclear Physics;2022-11

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