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Nuclear cosmochronometers for supernova neutrino-process

  • Takehito Hayakawa*
  • , Heamin Ko
  • , Myung Ki Cheoun
  • , Motohiko Kusakabe
  • , Toshitaka Kajino
  • , Satoshi Chiba
  • , Ken'ichi Nomoto
  • , Masa Aki Hashimoto
  • , Masaomi Ono
  • , Toshihiko Kawano
  • , Grant J. Mathews
  • *Corresponding author for this work
  • National Institutes for Quantum Science and Technology
  • The University of Osaka
  • Soongsil University
  • Beihang University
  • National Astronomical Observatory of Japan
  • The University of Tokyo
  • Institute of Science Tokyo
  • Kyushu University
  • RIKEN
  • Los Alamos National Laboratory Theoretical Division
  • University of Notre Dame

Research output: Contribution to conferencePaperpeer-review

Abstract

The short-lived unstable isotopes with half-lives of 0.1−10 My have been used as nuclear cosmochronometers to evaluate from an astrophysical event such as supernova (SN) explosion or AGB s-process to the solar system formation. We have proposed shorted-lived radioisotopes of 92Nb and 98Tc as the nuclear cosmochronometers for supernova neutrino-process.

Original languageEnglish
DOIs
StatePublished - 24 Feb 2022
Event16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 - Chengdu, China
Duration: 21 Sep 202125 Sep 2021

Conference

Conference16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021
Country/TerritoryChina
CityChengdu
Period21/09/2125/09/21

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