A2 Katsausartikkeli tieteellisessä aikausilehdessä
r-process nucleosynthesis : connecting rare-isotope beam facilities with the cosmos (2019)
Horowitz, C. J., Arcones, A., Côté, B., Dillmann, I., Nazarewicz, W., Roederer, U. I., Schatz, H., Aprahamian, A., Atanasov, D., Bauswein, A., Beers, T., Bliss, J., Brodeur, M., Clark, J. A., Frebel, A., Foucart, F., Hansen, C. J., Just, O., Kankainen, A., . . . Wang, M. (2019). r-process nucleosynthesis : connecting rare-isotope beam facilities with the cosmos. Journal of Physics G: Nuclear and Particle Physics, 46(8), Article 083001. https://doi.org/10.1088/1361-6471/ab0849
JYU-tekijät tai -toimittajat
Julkaisun tiedot
Julkaisun kaikki tekijät tai toimittajat: Horowitz, C. J.; Arcones, A; Côté, B.; Dillmann, I.; Nazarewicz, W.; Roederer, U. I.; Schatz, H.; Aprahamian, A.; Atanasov, D.; Bauswein, A.; et al.
Lehti tai sarja: Journal of Physics G: Nuclear and Particle Physics
ISSN: 0954-3899
eISSN: 1361-6471
Julkaisuvuosi: 2019
Volyymi: 46
Lehden numero: 8
Artikkelinumero: 083001
Kustantaja: Institute of Physics
Julkaisumaa: Britannia
Julkaisun kieli: englanti
DOI: https://doi.org/10.1088/1361-6471/ab0849
Julkaisun avoin saatavuus: Ei avoin
Julkaisukanavan avoin saatavuus:
Rinnakkaistallenteen verkko-osoite (pre-print): https://arxiv.org/abs/1805.04637
Tiivistelmä
This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and electromagnetic radiation from radio to gamma rays. The very red color of the associated kilonova suggests that neutron star mergers are an important r-process site. Astrophysical simulations of neutron star mergers and core collapse supernovae are making rapid progress. Detection of both electron neutrinos and antineutrinos from the next galactic supernova will constrain the composition of neutrino-driven winds and provide unique nucleosynthesis information. Finally, FRIB and other rare-isotope beam facilities will soon have dramatic new capabilities to synthesize many neutron-rich nuclei that are involved in the r-process. The new capabilities can significantly improve our understanding of the r-process and likely resolve one of the main outstanding problems in classical nuclear astrophysics. However, to make best use of the new experimental capabilities and to fully interpret the results, a great deal of infrastructure is needed in many related areas of astronomy, astrophysics, and nuclear theory. We place these experiments in context by discussing astrophysical simulations and observations of r-process sites, observations of stellar abundances, galactic chemical evolution, and nuclear theory for the structure and reactions of very neutron-rich nuclei. This review paper was initiated at a three-week International Collaborations in Nuclear Theory program in June 2016, where we explored promising r-process experiments and discussed their likely impact, and their astronomical, astrophysical, and nuclear theory context.
YSO-asiasanat: ydinfysiikka; astrofysiikka; alkuaineet
Vapaat asiasanat: nucleosynthesis; rare-isotope beam facilities; r-process nucleosynthesis; galactic chemical evolution
Liittyvät organisaatiot
Hankkeet, joissa julkaisu on tehty
- Harvinaisten ydinten tutkimuksia alkuaineiden syntyprosessien ymmärtämiseksi maailmankaikkeudessa
- Kankainen, Anu
- Suomen Akatemia
- Harvinaisten ydinten tutkimuksia alkuaineiden syntyprosessien ymmärtämiseksi maailmankaikkeudessa
- Kankainen, Anu
- Suomen Akatemia
- Harvinaisten ydinten tutkimuksia alkuaineiden syntyprosessien ymmärtämiseksi maailmankaikkeudessa
- Kankainen, Anu
- Suomen Akatemia
OKM-raportointi: Kyllä
Raportointivuosi: 2019
JUFO-taso: 2