Pith. sign in

REVIEW

Centaurus A as a source of extragalactic cosmic rays with arrival energies well beyond the GZK cutoff

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv gr-qc/9511031 v2 pith:G7RR7AME submitted 1995-11-10 gr-qc

classification gr-qc
keywords arrivalcosmicenergyextragalacticrayssourceapproxcentaurus
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

The ultra--high energy cosmic rays recently detected by several air shower experiments could have an extragalactic origin. In this case, the nearest active galaxy Centaurus A might be the source of the most energetic particles ever detected on Earth. We have used recent radio observations in order to estimate the arrival energy of the protons accelerated by strong shock fronts in the outer parts of this southern radio source. We expect detections corresponding to particles with energies up to $\sim 2.2 \times 10^{21}$ eV and an arrival direction of ($l \approx 310^{\circ}$, $b \approx 20^{\circ}$) in galactic coordinates. The future Southern Hemisphere Pierre Auger Observatory might provide a decisive test for extragalactic models of the origin of the ultra--high energy cosmic rays.

Discussion (0). Continue with ORCID to comment.

Pith tools