A review of indirect searches for particle dark matter
By J. Gaskins. 2016
329 citations recorded by the source corpus.
The indirect detection of dark matter annihilation and decay using observations of photons, charged cosmic rays and neutrinos offers a promising means of identifying the particle nature of this elusive component of the universe. The last decade has seen substantial advances in observational data-sets, complemented by new insights from numerical simulations, which together have enabled for the first time strong constraints on dark matter particle models, and have revealed several intriguing hints of possible signals. This review provides an introduction to indirect detection methods and an overview of recent results in the field.
Subfields: Materials Chemistry, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/c3fe95641a0415a766767afe53e50582bd595489
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In Materials Chemistry
- Gopolang Mohlabeng
- L. Mantani
- C. Arina
- Olivier Mattelaer
- Fabio Maltoni
- Federico Ambrogi
- Jan Heisig
- Mihailo Backovic
In Nuclear and High Energy Physics
- Olivier Mattelaer
- Fabio Maltoni
- Mihailo Backovic
- Gopolang Mohlabeng
- L. Mantani
- C. Arina
- E. M. Sessolo
- Federico Ambrogi
Citations in the corpus
- WIMP dark matter candidates and searches—current status and future prospects (2017, background): “d models see, e.g., [209] and references therein. 3.2 Gamma rays: limits and Galactic Center excess Gamma-rays represent a promising channel in which to search for dark matter (for reviews see, e.g., [10,11,210]). WIMPs are expected to annihilate at present leading to the possibility of detecting an”
- MadDM v.3.0: A comprehensive tool for dark matter studies (2018, methodology): “t; 95% CL upper limit for sigmav from Fermi-LAT dSphs for final state y0 y0 # [31] : tot_Xsec --> total sigmav # [32] : tot_SM_xsec ---> total sigmav for annihilation into all SM final states # [33] : Fermi_sigmav ---> 95% CL Fermi-LAT upper limit for annihilation into SM final states # [34”