arXiv · 0810.3012
Supersymmetric superheavy dark matter
Abstract
We propose the lightest supersymmetric particle (LSP) as a well-suited candidate for superheavy dark matter (SHDM). Various production mechanisms at the end of inflation can produce SHDM with the correct abundance, $Ω_{LSP} h^2 \sim 0.1$, if its mass is sufficiently high. In particular, gravitational production requires that the mass $m_{LSP}$ of the LSP is above $3\times 10^{11} GeV$. Weak interactions remain perturbative despite the large mass hierarchy, $m_{LSP}\gg m_Z$, because of the special decoupling properties of supersymmetry. As a result the model is predictive and we discuss the relevant cosmological processes for the case of a superheavy neutralino within this scheme.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
V. Berezinsky, M. Kachelriess, M. Aa. Solberg. 2008-12-12. Supersymmetric superheavy dark matter. https://doi.org/10.1103/physrevd.78.123535
Cite the original work for its findings. Save a collection to share your selection of sources.