Energetics of ultrahigh-energy cosmic-ray nuclei

Yu Jiang, B. Theodore Zhang, Kohta Murase

Research output: Contribution to journalArticlepeer-review

8 Scopus citations


Energetics of the ultrahigh-energy cosmic rays (UHECRs) generated in the Universe is crucial for pinning down their candidate sources. Using the recent Auger data on UHECR spectra, we calculate the UHECR energy generation rate density for different species of nuclei at the injection, considering intermediate and heavy nuclei as well as protons, through scanning over source parameters on the spectral index, maximum energy and redshift evolution. We find the resulting UHECR energy generation rate density to be ≈(0.2-2)×1044 erg Mpc-3 yr-1 at 1019.5 eV with a nontrivial dependence on the spectral index. Nuclei other than protons and irons favor hard spectral indices at the injection, and the required value of energy budget is smaller for intermediate nuclei. Given significant uncertainties in hadronic interaction models and astrophysical models for the Galactic-extragalactic transition, our results can be regarded as conservative. The composition data on Xmax give additional constraints, but the results are consistent within the model uncertainties.

Original languageEnglish (US)
Article number043017
JournalPhysical Review D
Issue number4
StatePublished - Aug 15 2021

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics


Dive into the research topics of 'Energetics of ultrahigh-energy cosmic-ray nuclei'. Together they form a unique fingerprint.

Cite this