Cosmological Fine Tuning, Supersymmetry, and the Gauge Heirarchy Problem
arXiv:hep-ph/9811284 · doi:10.1016/S0370-2693(99)00168-9
Abstract
We study the extent to which the cosmological fine-tuning problem - why the relic density of neutralino cold dark matter particles is similar to that of baryons - is related to the fine-tuning aspect of the gauge hierarchy problem - how one arranges that M_W << M_P without unnatural choices of MSSM parameters. Working in the minimal supergravity framework with universal soft supersymmetry-breaking parameters as inputs, we find that the hierarchical fine tuning is minimized for Ω_χ h^2 \sim 0.1. Conversely, imposing Ω_χ h^2 < 1 does not require small hierarchical fine tuning, but the exceptions to this rule are rather special, with parameters chosen such that m_χ\sim M_Z/2 or M_h/2, or else m_χ \simgt m_t. In the first two cases, neutralino annihilation receives a large contribution from a direct-channel pole, whereas in the third case it is enhanced by the large top Yukawa coupling.
9 pages, latex, 7 ps figures
References in corpus (4)
Cited by in corpus (11)
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