The DOI matches its Crossref record; 72 of the 72 references it cites were found in a registry or an index.
Cosmic-Ray Propagation and Interactions in the Galaxy
Open accessAbstract
We survey the theory and experimental tests for the propagation of cosmic rays in the Galaxy up to energies of 10 15 eV. A guide to the previous reviews and essential literature is given, followed by an exposition of basic principles. The basic ideas of cosmic-ray propagation are described, and the physical origin of its processes is explained. The various techniques for computing the observational consequences of the theory are described and contrasted. These include analytical and numerical techniques. We present the comparison of models with data, including direct and indirect—especially γ-ray—observations, and indicate what we can learn about cosmic-ray propagation. Some important topics, including electron and antiparticle propagation, are chosen for discussion.
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Cites
Toward a theory of interstellar turbulence. 2: Strong alfvenic turbulence
Goldreich, P., & Sridhar, S. (1995) · The Astrophysical Journal · doi:10.1086/175121 · Cited by 2,240
Veilleux, S., Cecil, G., & Bland-Hawthorn, J. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.072103.150610 · Cited by 1,504
Energy levels of A = 21–44 nuclei (VII)
Endt, P. M. (1990) · Nuclear Physics A · doi:10.1016/0375-9474(90)90598-g · Cited by 1,310
Interstellar Turbulence I: Observations and Processes
Elmegreen, B. G., & Scalo, J. (2004) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.41.011802.094859 · Cited by 1,175
Березинский, В. С., Буланов, С. В., Ginzburg, V. L., Dogel, V. A., & Птускин, В. С. (1984) · Cited by 1,139
Energy levels of A = 21–44 nuclei (VI)
Endt, P. M., & Van Der Leun, C. (1978) · Nuclear Physics A · doi:10.1016/0375-9474(78)90611-5 · Cited by 1,066
Propagation of Cosmic‐Ray Nucleons in the Galaxy
Strong, A. W., & Moskalenko, I. V. (1998) · The Astrophysical Journal · doi:10.1086/306470 · Cited by 1,051
Self-citationKelner, S. R., Aharonian, F. A., & Bugayov, V. V. (2006) · Physical Review D · doi:10.1103/physrevd.74.034018 · Cited by 916
Schlickeiser, R. (2002) · Astronomy and Astrophysics Library · doi:10.1007/978-3-662-04814-6 · Cited by 904
Production and Propagation of Cosmic‐Ray Positrons and Electrons
Moskalenko, I. V., & Strong, A. W. (1998) · The Astrophysical Journal · doi:10.1086/305152 · Cited by 766
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Cited by
PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra
Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S., et al. (2011) · Science · doi:10.1126/science.1199172 · Cited by 894
Theoretical Challenges in Galaxy Formation
Naab, T., & Ostriker, J. P. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040019 · Cited by 722
Acceleration of petaelectronvolt protons in the Galactic Centre
HESS Collaboration (2016) · Nature · doi:10.1038/nature17147 · Cited by 503
THE FERMI HAZE: A GAMMA-RAY COUNTERPART TO THE MICROWAVE HAZE
Dobler, G., Finkbeiner, D. P., Cholis, I., Slatyer, T., & Weiner, N. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/717/2/825 · Cited by 285
“A schematic of the relative importance of these emission mechanisms in the Galactic plane (|ℓ| ≤ 30, |b| ≤ 5) generated by the GALPROP code, version 50p (Strong et al. 2000; Porter & Strong 2005; Strong et al. 2007) is shown in Figure 2.”
MethodPlanck 2015 results: X. Diffuse component separation: Foreground maps
Planck Collaboration, Adam, R., Ade, P. A. R., Aghanim, N., Alves, M. I. R., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201525967 · Cited by 278
Self-citation
Metadata
- Authors
- Strong, A. W., Moskalenko, I. V., & Ptuskin, V. S.
- Venue
- Annual Review of Nuclear and Particle Science
- Publisher
- Annual Reviews
- Published
- 2007-11-01
- Volume
- 57
- Issue
- 1
- Pages
- 285-327
- ISSN
- 0163-8998 (ISSN-L)
- 1545-4134
- OpenAlex
- W2107415832
- Cited by
- 1,161
- References
- 72
- FWCI
- 3.91
- Type
- journal article
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
