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Prompt neutrino fluxes from atmospheric charm
Open accessAbstract
We calculate the prompt neutrino flux from atmospheric charm production by cosmic rays, using the dipole picture in a perturbative QCD framework, which incorporates the parton saturation effects present at high energies. We compare our results with the next-to-leading-order perturbative QCD result and find that saturation effects are large for neutrino energies above ${10}^{6}\text{ }\text{ }\mathrm{GeV}$, leading to a substantial suppression of the prompt neutrino flux. We comment on the range of prompt neutrino fluxes due to theoretical uncertainties.
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Metadata
- Authors
- Enberg, R., Reno, M. H., & Sarcevic, I.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2008-08-20
- Volume
- 78
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W2161978723
- Cited by
- 302
- References
- 0
- FWCI
- 6.19
- Type
- journal article
- Language
- en
- Open access
- green
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- Enberg, R., Reno, M. H., & Sarcevic, I. (2008). Prompt neutrino fluxes from atmospheric charm. Physical Review D. https://doi.org/10.1103/physrevd.78.043005
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