Revisiting the role of the streaming instability for the cosmic-ray spectrum in the GeV to TeV range
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866912764826484736 |
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| author | Thanh, Linh Han Dörner, Julien Fichtner, Horst Tjus, Julia Becker Amato, Elena |
| author_facet | Thanh, Linh Han Dörner, Julien Fichtner, Horst Tjus, Julia Becker Amato, Elena |
| contents | A complete understanding of the cosmic-ray energy spectrum remains a challenge to theory that must be met by comprehensive modeling efforts. One of these is the subject of the present study, namely, an explanation of the recently discovered spectral hardening at $\sim 300$ GeV with self-consistently treated cosmic-ray diffusion, where self-generated waves resulting from the streaming instability impact the diffusion of high-energy particles. We revisit the corresponding model by Blasi et al. (2012), perform an extensive parameter study, and determine an optimal range of parameters that best fit the cosmic-ray data. We conclude that self-consistently treated cosmic-ray transport remains a competitive alternative to explain the spectral hardening of the cosmic-ray energy spectrum at a few hundred GeV. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_13128 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Revisiting the role of the streaming instability for the cosmic-ray spectrum in the GeV to TeV range Thanh, Linh Han Dörner, Julien Fichtner, Horst Tjus, Julia Becker Amato, Elena High Energy Astrophysical Phenomena A complete understanding of the cosmic-ray energy spectrum remains a challenge to theory that must be met by comprehensive modeling efforts. One of these is the subject of the present study, namely, an explanation of the recently discovered spectral hardening at $\sim 300$ GeV with self-consistently treated cosmic-ray diffusion, where self-generated waves resulting from the streaming instability impact the diffusion of high-energy particles. We revisit the corresponding model by Blasi et al. (2012), perform an extensive parameter study, and determine an optimal range of parameters that best fit the cosmic-ray data. We conclude that self-consistently treated cosmic-ray transport remains a competitive alternative to explain the spectral hardening of the cosmic-ray energy spectrum at a few hundred GeV. |
| title | Revisiting the role of the streaming instability for the cosmic-ray spectrum in the GeV to TeV range |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2512.13128 |