Charge spectrum of galactic cosmic ray nuclei as measured in meteorite olivines

Aleksandrov, A. B.; Bagulya, A. V.; Vladimirov, M. S.; Goncharova, L. A.; Ivliev, A. I.; Kalinina, G. V.; Kashkarov, L. L.; Konovalova, N. S.; Okateva, N.; Polukhina, N.; Rusetskiĭ, A. S.; Старков, Н. И.

doi:10.3367/ufne.0180.201008c.0839

Cited by 10 publications

(1 citation statement)

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“…Except for the relatively recent superTIGER experiment in the Z = 30 − 40 range [65], the experiments in the high charge range date back to the end of the seventies (Ariel6 [63], HEAO3-HNE [66,67]), the early eighties (UHCRE-LDEF [3,68,69]), or at best the nineties (Trek [70,71]). The most recent results on subactinides and actinides come from indirect measurements of the CRs from their impact on meteorite olivines [72][73][74], namely the Olimpiya Experiment (not implemented yet in CRDB). The solution to the origin of these elements may come from yet another route: recently, optical follow-up observations of a gravitational wave event have shown that binary star mergers could be a major r-process contributor to UHCRs [75].…”

Section: Very Heavy and Ultra-heavy Crsmentioning

confidence: 99%

Cosmic-Ray Database Update: Ultra-High Energy, Ultra-Heavy, and Antinuclei Cosmic-Ray Data (CRDB v4.0)

et al. 2020

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We present an update on CRDB, the cosmic-ray database for charged species. CRDB is based on MySQL, queried and sorted by jquery and table-sorter libraries, and displayed via PHP web pages through the AJAX protocol. We review the modifications made on the structure and outputs of the database since the first release (Maurin et al., 2014). For this update, the most important feature is the inclusion of ultra-heavy nuclei (Z>30), ultra-high energy nuclei (from 1015 to 1020 eV), and limits on antinuclei fluxes (Z≤−1 for A>1); more than 100 experiments, 350 publications, and 40,000 data points are now available in CRDB. We also revisited and simplified how users can retrieve data and submit new ones. For questions and requests, please contact crdb@lpsc.in2p3.fr.

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