Abstract
Although the existence of Dark Matter (DM) is well-established to explain a range of astrophysical and cosmological measurements, its nature and particle properties still remain one of the greatest unsolved puzzles of particle and astroparticle physics (Bertone and Hooper, Phys Rept 405:279 (2005), [1]).
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Notes
- 1.
In QCD there could be a violation of CP symmetry in the strong interactions not observed in nature. As there is no known reason for it to be conserved in QCD specifically, this is a “fine tuning” problem known as the strong CP problem.
- 2.
In NWA the integral of the square propagator \(\int \frac{\text {d}s}{(s-M_{med}^2)^2+M_{med}\Gamma ^2} = \frac{\pi }{M_{med}\Gamma }\) is non-zero only for a small region of s, where the PDFs can be taken as constant.
- 3.
The mediator is assumed to not couple with the leptons to avoid the tight limits set by the dilepton searches.
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Gustavino, G. (2017). The Dark Matter Paradigm. In: Search for New Physics in Mono-jet Final States in pp Collisions . Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-58871-1_4
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