The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.
Non-linear amplification of a magnetic field driven by cosmic ray streaming
Open accessAbstract
One-, two- and three-dimensional numerical results of the non-linear interaction between cosmic rays and a magnetic field are presented. These show that cosmic ray streaming drives large-amplitude Alfvénic waves. The cosmic ray streaming energy is very efficiently transferred to the perturbed magnetic field of the Alfvén waves, and the non-linear time-scale of the growth of the waves is found to be very rapid, of the order of the gyro-period of the cosmic ray. Thus, a magnetic field of interstellar values, assumed in models of supernova remnant blast wave acceleration, would not be appropriate in the region of the shock. The increased magnetic field reduces the cosmic ray acceleration time and so increases the maximum cosmic ray energy, which may provide a simple and elegant resolution to the highest energy Galactic cosmic ray problem, where the cosmic rays themselves provide the fields necessary for their acceleration.
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Citations
Cites
Plasma Physics via Computer Simulation
Birdsall, C. K., & Langdon, A. B. (2018) · CRC Press eBooks · doi:10.1201/9781315275048 · Cited by 3,745
The acceleration of cosmic rays in shock fronts - I
Bell, A. R. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/182.2.147 · Cited by 2,679
Self-citationParticle acceleration by astrophysical shocks
Blandford, R. D., & Ostriker, J. P. (1978) · The Astrophysical Journal · doi:10.1086/182658 · Cited by 1,967
Particle acceleration at astrophysical shocks: A theory of cosmic ray origin
Blandford, R., & Eichler, D. (1987) · Physics Reports · doi:10.1016/0370-1573(87)90134-7 · Cited by 1,964
Drury, L. O. (1983) · Reports on Progress in Physics · doi:10.1088/0034-4885/46/8/002 · Cited by 1,713
The Origin of Ultra-High-Energy Cosmic Rays
Hillas, A. M. (1984) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.22.090184.002233 · Cited by 1,320
Numerical Methods in Fluid Dynamics
Brezzi, F. (1985) · Springer eBooks · doi:10.1007/bfb0074528 · Cited by 969
Cosmic Ray Streaming--I EFFECT OF ALFVEN WAVES ON PARTICLES
Skilling, J. (1975) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/172.3.557 · Cited by 501
Cosmic-Ray Propagation in the Galaxy: Collective Effects
Wentzel, D. G. (1974) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.12.090174.000443 · Cited by 337
Cosmic Ray Streaming--III SELF-CONSISTENT SOLUTIONS
Skilling, J. (1975) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/173.2.255 · Cited by 150
Cited by
The Astrophysics of Ultrahigh-Energy Cosmic Rays
Kotera, K., & Olinto, A. V. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102620 · Cited by 470
Aharonian, F., Akhperjanian, A. G., Bazer-Bachi, A. R., Beilicke, M., Benbow, W., Berge, D., Bernlöhr, K., Boisson, C., Bolz, O., Borrel, V., et al. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20054279 · Cited by 309
THE FERMI BUBBLES AS A SCALED-UP VERSION OF SUPERNOVA REMNANTS
Fujita, Y., Ohira, Y., & Yamazaki, R. (2013) · The Astrophysical Journal · doi:10.1088/2041-8205/775/1/l20 · Cited by 47
“CRs are accelerated in the shock neighborhood, where some nonlinear effects generate strong magnetic waves or cause strong amplification of magnetic fields (Lucek & Bell 2000; Bell 2004).”
Background
Metadata
- Authors
- Lucek, S. G., & Bell, A. R.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2000-05-01
- Volume
- 314
- Issue
- 1
- Pages
- 65-74
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1969092613
- Cited by
- 377
- References
- 11
- FWCI
- 6.60
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Lucek, S. G., & Bell, A. R. (2000). Non-linear amplification of a magnetic field driven by cosmic ray streaming. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2000.03363.x
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
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.
