The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.
Gamma ray signals from dark matter: Concepts, status and prospects
Open accessAbstract
Weakly interacting massive particles (WIMPs) remain a prime candidate for the cosmological dark matter (DM), even in the absence of current collider signals that would unambiguously point to new physics below the TeV scale. The self-annihilation of these particles in astronomical targets may leave observable imprints in cosmic rays of various kinds. In this review, we focus on gamma rays which we argue to play a pronounced role among the various possible messengers. We discuss the most promising spectral and spatial signatures to look for, give an update on the current state of gamma-ray searches for DM and an outlook concerning future prospects. We also assess in some detail the implications of a potential signal identification for particle DM models as well as for our understanding of structure formation. Special emphasis is put on the possible evidence for a 130 GeV line-like signal that we recently identified in the data of the Fermi gamma-ray space telescope.
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Cites
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“The commonly used Navarro-Frenk-White (NFW) profile [74], for example, is obtained for (α, β, γ) = (1, 3, 1) (with rs ≃ 20 kpc in case of the Milky Way); the cored isothermal profile follows when setting (α, β, γ) = (2, 2, 0) and rs ≃ 3.”
MethodParticle dark matter: evidence, candidates and constraints
Bertone, G., Hooper, D., & Silk, J. (2005) · Physics Reports · doi:10.1016/j.physrep.2004.08.031 · Cited by 4,979
Contraction of dark matter galactic halos due to baryonic infall
Blumenthal, G. R., Faber, S. M., Flores, R., & Primack, J. R. (1986) · The Astrophysical Journal · doi:10.1086/163867 · Cited by 1,213 · cited 1×
“In particular, the cooling and infall of baryons could – by a mechanism known as adiabatic contraction – lead to a steepening of the inner DM profile [84–86].”
BackgroundMcMillan, P. J. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18564.x · Cited by 789
Microwave Interstellar Medium Emission Observed by the Wilkinson Microwave Anisotropy Probe
Finkbeiner, D. P. (2004) · The Astrophysical Journal · doi:10.1086/423482 · Cited by 331
Extended Anomalous Foreground Emission in the WMAP Three‐Year Data
Dobler, G., & Finkbeiner, D. P. (2008) · The Astrophysical Journal · doi:10.1086/587862 · Cited by 223
Cited by
The Dark Energy Survey: more than dark energy – an overview
(2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw641 · Cited by 1,019
Update on scalar singlet dark matter
Cline, J. M., Scott, P., Kainulainen, K., & Weniger, C. (2013) · Physical Review D · doi:10.1103/physrevd.88.055025 · Cited by 580
Self-citationFundamental physics with the Square Kilometre Array
Weltman, A., Bull, P., Camera, S., Kelley, K., Padmanabhan, H., Pritchard, J., Raccanelli, A., Riemer-Sørensen, S., Shao, L., Andrianomena, S., et al. (2020) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2019.42 · Cited by 384
Self-citationAckermann, M., Ajello, M., Albert, A., Anderson, B., Atwood, W. B., Baldini, L., Barbiellini, G., Bastieri, D., Bellazzini, R., Bissaldi, E., et al. (2015) · Physical Review D · doi:10.1103/physrevd.91.122002 · Cited by 311
Metadata
- Authors
- Bringmann, T., & Weniger, C.
- Venue
- Physics of the Dark Universe
- Publisher
- Elsevier BV
- Published
- 2012-11
- Volume
- 1
- Issue
- 1-2
- Pages
- 194-217
- ISSN
- 2212-6864 (ISSN-L)
- OpenAlex
- W2043914286
- Cited by
- 225
- References
- 6
- FWCI
- 13.76
- Type
- journal article
- Language
- en
- Open access
- hybrid
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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.