The DOI matches its Crossref record; 185 of the 185 references it cites were found in a registry or an index.
COSMIC RAYS IN GALAXY CLUSTERS AND THEIR NONTHERMAL EMISSION
Open accessAbstract
Radio observations prove the existence of relativistic particles and magnetic field associated with the intra-cluster-medium (ICM) through the presence of extended synchrotron emission in the form of radio halos and peripheral relics. This observational evidence has fundamental implications on the physics of the ICM. Nonthermal components in galaxy clusters are indeed unique probes of very energetic processes operating within clusters that drain gravitational and electromagnetic energy into cosmic rays (CRs) and magnetic fields. These components strongly affect the (micro-)physical properties of the ICM, including viscosity and electrical conductivities, and have also potential consequences on the evolution of clusters themselves. The nature and properties of CRs in galaxy clusters, including the origin of the observed radio emission on cluster-scales, have triggered an active theoretical debate in the last decade. Only recently we can start addressing some of the most important questions in this field, thanks to recent observational advances, both in the radio and at high energies. The properties of CRs and of cluster nonthermal emissions depend on the dynamical state of the ICM, the efficiency of particle acceleration mechanisms in the ICM and on the dynamics of these CRs. In this paper, we discuss in some detail the acceleration and transport of CRs in galaxy clusters and the most relevant observational milestones that have provided important steps on our understanding of this physics. Finally, looking forward to the possibilities from new generations of observational tools, we focus on what appear to be the most important prospects for the near future from radio and high-energy observations.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
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
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
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
Spontaneously Growing Transverse Waves in a Plasma Due to an Anisotropic Velocity Distribution
Weibel, E. S. (1959) · Physical Review Letters · doi:10.1103/physrevlett.2.83 · Cited by 1,699
Atmospheric diffusion shown on a distance-neighbour graph
Richardson, L. F. (1926) · Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character · doi:10.1098/rspa.1926.0043 · Cited by 1,673
Cosmic-Ray Propagation. I. Charged Particles in a Random Magnetic Field
Jokipii, J. R. (1966) · The Astrophysical Journal · doi:10.1086/148912 · Cited by 1,367
Heating Hot Atmospheres with Active Galactic Nuclei
McNamara, B. R., & Nulsen, P. E. J. (2007) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110625 · Cited by 1,326
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
Bell, A. R. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08097.x · Cited by 1,148
Cosmology with the Sunyaev-Zel’dovich Effect
Carlstrom, J. E., Holder, G. P., & Reese, E. D. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093803 · Cited by 958
Cited by
The LOFAR Two-metre Sky Survey: I. Survey description and preliminary data release⋆
Shimwell, T. W., Röttgering, H. J. A., Best, P. N., Williams, W. L., Dijkema, T. J., de Gasperin, F., Hardcastle, M. J., Heald, G. H., Hoang, D. N., Horneffer, A., et al. (2017) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629313 · Cited by 640
Self-citationEuclid: I. Overview of the Euclid mission
Euclid Collaboration, Mellier, Y., Abdurro’uf, Acevedo Barroso, J. A., Achúcarro, A., Adamek, J., Adam, R., Addison, G. E., Aghanim, N., Aguena, M., et al. (2025) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202450810 · Cited by 616
The LOFAR Two-metre Sky Survey: II. First data release
Shimwell, T. W., Tasse, C., Hardcastle, M. J., Mechev, A. P., Williams, W. L., Best, P. N., Röttgering, H. J. A., Callingham, J. R., Dijkema, T. J., de Gasperin, F., et al. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833559 · Cited by 585
Self-citationDiffuse Radio Emission from Galaxy Clusters
van Weeren, R. J., de Gasperin, F., Akamatsu, H., Brüggen, M., Feretti, L., Kang, H., Stroe, A., & Zandanel, F. (2019) · Space Science Reviews · doi:10.1007/s11214-019-0584-z · Cited by 481
Crocker, R. M., Bicknell, G. V., Taylor, A. M., & Carretti, E. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/808/2/107 · Cited by 120
“…grounds (Bell 1978), on the basis of analysis of the Galaxy’s global cosmic-ray and nonthermal radiation budget (Strong et al. 2010), and from observations and analysis of nonthermal radiation associated with giant cluster shocks (Pinzke et al. 2013; Brunetti & Jones 2014, and references therein).”
Background
Metadata
- Authors
- BRUNETTI, G., & JONES, T. W.
- Venue
- International Journal of Modern Physics D
- Publisher
- World Scientific Pub Co Pte Lt
- Published
- 2014-03-18
- Volume
- 23
- Issue
- 04
- Pages
- 1430007
- ISSN
- 0218-2718 (ISSN-L)
- 1793-6594
- OpenAlex
- W2139505492
- Cited by
- 577
- References
- 185
- FWCI
- 19.06
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: COSMIC RAYS IN GALAXY CLUSTERS AND THEIR NONTHERMAL EMISSION. https://app.cochat.ai/papers/10.1142/s0218271814300079
- The paper
- BRUNETTI, G., & JONES, T. W. (2014). COSMIC RAYS IN GALAXY CLUSTERS AND THEIR NONTHERMAL EMISSION. International Journal of Modern Physics D. https://doi.org/10.1142/s0218271814300079
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.
