Microquasar jet-cocoon systems as PeVatrons
The origin of Galactic cosmic rays (CRs), particularly around the knee region ($\ensuremath{\sim}3\text{ }\text{ }\mathrm{PeV}$), remains a major unanswered question. Recent observations by LHAASO suggest that the knee is shaped mainly by protons, with a transition to heavier elements at higher energies. Microquasars---compact jet-emitting sources---have emerged as possible PeV CR accelerators, especially after detections of ultrahigh-energy gamma rays from these systems. We propose that the observed proton spectrum (hard below a few PeV, steep beyond) arises from the reacceleration of sub-TeV Galactic CRs via shear acceleration in large-scale microquasar jet-cocoon structures. Our model also naturally explains the observed spectrum of energies around a few tens of PeV by summing up heavier nuclei contributions. Additionally, similar reacceleration processes in radio galaxies can contribute to ultrahigh-energy CRs, bridging Galactic and extragalactic origins. Combined with low-energy CRs from supernova remnants and galaxy clusters around the second knee region, this scenario could provide a unified explanation for CRs across the entire energy spectrum.
Authors
- Kohta Murase (ORCID: https://orcid.org/0000-0002-5358-5642)
- B. Theodore Zhang (ORCID: https://orcid.org/0000-0003-2478-333X)
- Shigeo S. Kimura (ORCID: https://orcid.org/0000-0003-2579-7266)
Institutions
- Pennsylvania State University (US)
- Chinese Academy of Sciences (CN)
- Tohoku University (JP)
- Kyoto University (JP)
- Instituto de Física Teórica (ES)
- Institute of High Energy Physics (CN)
- Yukawa Institute for Theoretical Physics (JP)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2025-11-07
- DOI
- https://doi.org/10.1103/p6r1-qg5q
- Citations
- 3
- Primary Topic
- Astrophysics and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 5.61